<?xml version="1.0" encoding="UTF-8"?>
<!DOCTYPE article PUBLIC "-//NLM//DTD JATS (Z39.96) Journal Publishing DTD v1.1d1 20130915//EN" "JATS-journalpublishing1.dtd">
<article article-type="research-article" xmlns:xlink="http://www.w3.org/1999/xlink">
<front>
<journal-meta>
<journal-id journal-id-type="publisher-id">ptep</journal-id>
<journal-id journal-id-type="hwp">ptep</journal-id>
<journal-title-group>
<journal-title>Progress of Theoretical and Experimental Physics</journal-title>
</journal-title-group>
<issn pub-type="epub">2050-3911</issn>
<publisher>
<publisher-name>Oxford University Press</publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.1093/ptep/ptv155</article-id>
<article-id pub-id-type="publisher-id">ptv155</article-id>
<article-categories>
<subj-group subj-group-type="heading">
<subject>Papers</subject>
<subj-group subj-group-type="heading">
<subject>Theoretical Particle Physics</subject>
</subj-group>
</subj-group>
<subj-group subj-group-type="hwp-journal-coll">
<subject>B12</subject>
<subject>B13</subject>
<subject>B53</subject>
</subj-group>
</article-categories>
<title-group>
<article-title>Signal of doubly charged Higgs at <italic>e</italic><sup>&plus;</sup><italic>e</italic><sup>&minus;</sup> colliders</article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name><surname>Hue</surname><given-names>L. T.</given-names></name>
<xref ref-type="aff" rid="af1">1</xref>
<xref ref-type="corresp" rid="cor1">&#x002A;</xref>
</contrib>
<contrib contrib-type="author">
<name><surname>Huong</surname><given-names>D. T.</given-names></name>
<xref ref-type="aff" rid="af1">1</xref>
</contrib>
<contrib contrib-type="author">
<name><surname>Long</surname><given-names>H. N.</given-names></name>
<xref ref-type="aff" rid="af1">1</xref>
</contrib>
<contrib contrib-type="author">
<name><surname>Hung</surname><given-names>H. T.</given-names></name>
<xref ref-type="aff" rid="af2">2</xref>
</contrib>
<contrib contrib-type="author">
<name><surname>Thao</surname><given-names>N. H.</given-names></name>
<xref ref-type="aff" rid="af2">2</xref>
</contrib>
<aff id="af1"><label>1</label><addr-line>Institute of Physics, Vietnam Academy of Science and Technology, 10 Dao Tan, Ba Dinh, 10000 Hanoi, Vietnam</addr-line></aff>
<aff id="af2"><label>2</label><addr-line>Department of Physics, Hanoi University of Education 2, Phuc Yen, 11000 Vinh Phuc, Vietnam</addr-line></aff>
</contrib-group>
<author-notes>
<corresp id="cor1"><label>&#x002A;</label>E-mail: <email>lthue@iop.vast.ac.vn</email></corresp>
</author-notes>
<pub-date pub-type="ppub"><month>11</month><year>2015</year></pub-date>
<pub-date pub-type="epub"><day>25</day><month>11</month><year>2015</year></pub-date>
<volume>2015</volume>
<issue>11</issue>
<elocation-id>113B05</elocation-id>
<history>
<date date-type="received"><day>6</day><month>4</month><year>2015</year></date>
<date date-type="rev-recd"><day>1</day><month>8</month><year>2015</year></date>
<date date-type="accepted"><day>28</day><month>9</month><year>2015</year></date>
</history>
<permissions>
<copyright-statement>&#x00A9; The Author(s) 2015. Published by Oxford University Press on behalf of the Physical Society of Japan.</copyright-statement>
<copyright-year>2015</copyright-year>
<license xmlns:xlink="http://www.w3.org/1999/xlink" license-type="creative-commons" xlink:href="http://creativecommons.org/licenses/by/4.0/"><license-p>This is an Open Access article distributed under the terms of the Creative Commons Attribution License (<ext-link xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://creativecommons.org/licenses/by/4.0/" ext-link-type="uri">http://creativecommons.org/licenses/by/4.0/</ext-link>), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited.</license-p>
<license-p>Funded by SCOAP<sup>3</sup></license-p></license>
</permissions>
<self-uri content-type="pdf" xlink:href="ptv155.pdf"/>
<self-uri xlink:role="archival-pdf" xlink:href="ptv155-hires.pdf"/>
<abstract>
<p>The masses and signals of the production of doubly charged Higgses (DCH) in the framework of the supersymmetric reduced minimal 3-3-1 model are investigated. In the DCH sector, we prove that there always exists a region of the parameter space where the mass of the lightest DCH is of the order of <inline-formula><tex-math notation="LaTeX" id="ImEquation2"><![CDATA[$\mathcal {O}(100)$]]></tex-math></inline-formula>&#x2009;GeV even when all other new particles are very heavy. The lightest DCH mainly decays to two same-sign leptons while the dominant decay channels of the heavy DCHs are those decaying to heavy particles. We analyze each production cross section for <inline-formula><tex-math notation="LaTeX" id="ImEquation3"><![CDATA[$e^+e^- \rightarrow H^{++} H^{--}$]]></tex-math></inline-formula> as a function of a few kinematic variables, which are useful to discuss the creation of DCHs in <inline-formula><tex-math notation="LaTeX" id="ImEquation4"><![CDATA[$e^+e^-$]]></tex-math></inline-formula> colliders as an indicator of new physics beyond the Standard Model. A numerical study shows that the cross sections for creating the lightest DCH can reach values of a few pb. The other two DCHs are too heavy, beyond the observable range of experiments. The lightest DCH may be detected by the International Linear Collider or the Compact Linear Collider by searching for its decay to a same-sign charged lepton pair.</p>
</abstract>
<kwd-group kwd-group-type="jel">
<title>Subject Index</title>
<kwd>B12</kwd>
<kwd>B13</kwd>
<kwd>B53</kwd>
</kwd-group>
<funding-group>
<award-group id="funding-1"><funding-source>SCOAP<sup>3</sup></funding-source></award-group>
</funding-group>
<counts><page-count count="36"/></counts>
<custom-meta-group>
<custom-meta>
<meta-name>arxiv-id</meta-name>
<meta-value>arXiv:1404.5038</meta-value>
</custom-meta>
</custom-meta-group>
</article-meta>
</front>
<body>
<sec id="s1"><label>1.</label><title>Introduction</title>
<p>The detection of the Higgs boson, with a mass around 125 GeV, by experiments at the Large Hadron Collider (LHC) [<xref ref-type="bibr" rid="PTV155C1">1</xref>&#x2013;<xref ref-type="bibr" rid="PTV155C4">4</xref>] has again confirmed the success of the Standard Model (SM). However, this model needs to be extended to cover other problems that cannot be explained in this framework, particularly small neutrino mass and mixing, dark matter (DM), asymmetry of matter and antimatter, etc. Theories that lie beyond the SM not only solve the SM problems but also predict the signals of new physics that can be searched for in the future. Many well known models beyond the SM have Higgs spectra containing doubly charged Higgses (DCHs), e.g., the left&#x2013;right model [<xref ref-type="bibr" rid="PTV155C5">5</xref>&#x2013;<xref ref-type="bibr" rid="PTV155C7">7</xref>], the Zee&#x2013;Babu model [<xref ref-type="bibr" rid="PTV155C8">8</xref>, <xref ref-type="bibr" rid="PTV155C9">9</xref>], the 3-3-1 models [<xref ref-type="bibr" rid="PTV155C10">10</xref>&#x2013;<xref ref-type="bibr" rid="PTV155C13">13</xref>], etc, and their supersymmetric versions [<xref ref-type="bibr" rid="PTV155C14">14</xref>&#x2013;<xref ref-type="bibr" rid="PTV155C21">21</xref>]. The appearance of the DCHs will really be one of the signals of new physics. Hence, there have been a number of publications predicting this signal in colliders such as the LHC, International Linear Collider (ILC) [<xref ref-type="bibr" rid="PTV155C22">22</xref>, <xref ref-type="bibr" rid="PTV155C23">23</xref>], and Compact Linear Collider (CLIC) [<xref ref-type="bibr" rid="PTV155C24">24</xref>, <xref ref-type="bibr" rid="PTV155C25">25</xref>]. Recent experimental searches for the DCHs have been done at the LHC [<xref ref-type="bibr" rid="PTV155C26">26</xref>&#x2013;<xref ref-type="bibr" rid="PTV155C29">29</xref>], through their decays into a pair of same-sign charged leptons. This decay channel has been investigated in many of the above models: the left&#x2013;right symmetric model [<xref ref-type="bibr" rid="PTV155C30">30</xref>, <xref ref-type="bibr" rid="PTV155C31">31</xref>] and the supersymmetric version [<xref ref-type="bibr" rid="PTV155C32">32</xref>], and the 3-3-1 models [<xref ref-type="bibr" rid="PTV155C33">33</xref>, <xref ref-type="bibr" rid="PTV155C34">34</xref>]. On the other hand, some other SM extensions, including Higgs triplets, have shown that the DCHs may have main decay channels of <inline-formula><tex-math notation="LaTeX" id="ImEquation5"><![CDATA[$H^{\pm \pm }\rightarrow W^{\pm }W^{\pm }$]]></tex-math></inline-formula> [<xref ref-type="bibr" rid="PTV155C35">35</xref>, <xref ref-type="bibr" rid="PTV155C36">36</xref>], or <inline-formula><tex-math notation="LaTeX" id="ImEquation6"><![CDATA[$H^{\pm }W^{\pm }$]]></tex-math></inline-formula> [<xref ref-type="bibr" rid="PTV155C37">37</xref>], leading to lower bounds of DCH masses than those obtained by searching for DCH decay into leptons. It is noted that the Higgs sectors in the supersymmetric (SUSY) models seem to be very interesting because they do not contain unknown self-couplings of four Higgses in the superpotential, unlike the case of non-SUSY models, where these kinds of couplings directly contribute to the Higgs masses. As a consequence, some Higgses will get masses mainly from the D-term, namely, from the electroweak breaking scale, leading to values of Higgs masses being of the order of <inline-formula><tex-math notation="LaTeX" id="ImEquation7"><![CDATA[$\mathcal {O}(100)$]]></tex-math></inline-formula>&#x2009;GeV at the tree level. This happens in SUSY models such as the minimal supersymmetric standard model (MSSM) and supersymmetric versions of the economical 3-3-1 (SUSYE331) and reduced minimal 3-3-1 (SUSYRM331) models [<xref ref-type="bibr" rid="PTV155C20">20</xref>, <xref ref-type="bibr" rid="PTV155C21">21</xref>, <xref ref-type="bibr" rid="PTV155C38">38</xref>]. It has been shown that there is at least one neutral CP-even Higgs inheriting a tree-level mass below the mass of the <inline-formula><tex-math notation="LaTeX" id="ImEquation8"><![CDATA[$Z$]]></tex-math></inline-formula> boson, <inline-formula><tex-math notation="LaTeX" id="ImEquation9"><![CDATA[$m_Z=92$]]></tex-math></inline-formula>&#x2009;GeV. Fortunately, the loop-correction contributions increase the full mass of this Higgs up to the recent experimental value. This suggests that some other Higgses may be light with masses of the order of <inline-formula><tex-math notation="LaTeX" id="ImEquation10"><![CDATA[$\mathcal {O}(100)$]]></tex-math></inline-formula>&#x2009;GeV. In the MSSM, this cannot happen if soft parameters such as the <inline-formula><tex-math notation="LaTeX" id="ImEquation11"><![CDATA[$b_{\mu }$]]></tex-math></inline-formula> term, related to the mass of the neutral CP-odd Higgs, are large. Other SUSY versions, such as the 3-3-1 models, are different because of the appearance of the <inline-formula><tex-math notation="LaTeX" id="ImEquation12"><![CDATA[${\rm SU}(3)_L$]]></tex-math></inline-formula> scale apart from the SUSY scale. For SUSYE331, the parameters characterizing these two scales may cancel each other to create the light mass of the lightest singly charged Higgs [<xref ref-type="bibr" rid="PTV155C38">38</xref>]. In this work, we will investigate the DCHs in SUSYRM331 and prove that there may exist a light DCH, even if both the soft and <inline-formula><tex-math notation="LaTeX" id="ImEquation13"><![CDATA[${\rm SU}(3)_L$]]></tex-math></inline-formula> parameters are very large. Apart from inheriting the lepton number two, this light DCH is also lighter than almost all of the new particles in the model, and therefore will decay mainly to a same-sign lepton pair. So the possibility of detection of the lightest DCH will increase at colliders such as the LHC, ILC, and CLIC. In the left&#x2013;right symmetric model, the cross sections for DCH creation at the LHC are predicted below 5&#x2009;fb for mass values greater than 200&#x2009;GeV. In the SUSY left&#x2013;right model, they are estimated below 10&#x2009;fb with a collision energy of 14&#x2009;TeV at LHC [<xref ref-type="bibr" rid="PTV155C30">30</xref>] and a DCH mass smaller than 450&#x2009;GeV. The cross sections for the DCH creation will decrease if their masses increase. In the framework of the 3-3-1 model, the cross sections for creating DCHs can reach a value smaller than <inline-formula><tex-math notation="LaTeX" id="ImEquation14"><![CDATA[$10^{2}$]]></tex-math></inline-formula>&#x2009;fb in <inline-formula><tex-math notation="LaTeX" id="ImEquation15"><![CDATA[$e^+e^-$]]></tex-math></inline-formula> colliders [<xref ref-type="bibr" rid="PTV155C33">33</xref>, <xref ref-type="bibr" rid="PTV155C34">34</xref>]. Our work will concentrate on the signals of detecting DCHs at the ILC and CLIC because of their very high precision. In addition, the collision energies of the ILC and CLIC are smaller than that of the LHC but the total cross sections for creating DCHs at the ILC and CLIC are larger than those at the LHC.</p>
<p>Let us remind ourselves of the reason for studying 3-3-1 models. The 3-3-1 models not only contain the great success of the SM but can also solve many problems of the SM. In particular, the 3-3-1 models can provide small neutrino masses as well as candidates for the DM [<xref ref-type="bibr" rid="PTV155C39">39</xref>, <xref ref-type="bibr" rid="PTV155C40">40</xref>]. The decays of some new particles can solve the matter&#x2013;antimatter asymmetry via leptogenesis mechanisms [<xref ref-type="bibr" rid="PTV155C41">41</xref>&#x2013;<xref ref-type="bibr" rid="PTV155C43">43</xref>]. The 3-3-1 models can connect to the cosmological inflation [<xref ref-type="bibr" rid="PTV155C41">41</xref>&#x2013;<xref ref-type="bibr" rid="PTV155C43">43</xref>]. In addition, the 3-3-1 models [<xref ref-type="bibr" rid="PTV155C10">10</xref>, <xref ref-type="bibr" rid="PTV155C11">11</xref>, <xref ref-type="bibr" rid="PTV155C13">13</xref>, <xref ref-type="bibr" rid="PTV155C44">44</xref>&#x2013;<xref ref-type="bibr" rid="PTV155C49">49</xref>] have many intriguing properties. In order to make the models anomaly free, one of the quark families must transform under <inline-formula><tex-math notation="LaTeX" id="ImEquation16"><![CDATA[$\hbox {SU}(3)_L$]]></tex-math></inline-formula> in a different way from the other two. This leads to a consequence that the number of fermion generations has to be a multiple of the color number, which is three. In combination with the QCD asymptotic freedom requiring the number of quark generations to be less than five, the solution is exactly three for the number of fermion generations required. Furthermore, the 3-3-1 models give a good explanation of the electric charge quantization [<xref ref-type="bibr" rid="PTV155C50">50</xref>&#x2013;<xref ref-type="bibr" rid="PTV155C54">54</xref>].</p>
<p>It is to be noted that the unique disadvantage of the 3-3-1 models is the complication in the Higgs sector, which reduces their predictability. Recently, there have been some efforts to reduce the Higgs contents of the models. The first successful attempt was with the 3-3-1 model with right-handed neutrinos [<xref ref-type="bibr" rid="PTV155C44">44</xref>&#x2013;<xref ref-type="bibr" rid="PTV155C49">49</xref>], giving a model with just two Higgs triplets. The model is called the economical 3-3-1 model [<xref ref-type="bibr" rid="PTV155C55">55</xref>&#x2013;<xref ref-type="bibr" rid="PTV155C57">57</xref>]. A similar version to the minimal 3-3-1 model with a Higgs sector containing three triplets and one sextet is the reduced minimal 3-3-1 model with again just two Higgs triplets [<xref ref-type="bibr" rid="PTV155C12">12</xref>, <xref ref-type="bibr" rid="PTV155C58">58</xref>]. However, to give masses to all fermions in the 3-3-1 models with the minimal Higgs sector, one has to introduce effective couplings that are nonrenormalizable. On the other hand, by investigating the one-loop <inline-formula><tex-math notation="LaTeX" id="ImEquation17"><![CDATA[$\beta $]]></tex-math></inline-formula>-function in the minimal 3-3-1 model and its supersymmetric version, we can predict the existence of Landau poles that make these theories lose their perturbative character. In order to solve this problem, the cut-off <inline-formula><tex-math notation="LaTeX" id="ImEquation18"><![CDATA[$\Lambda \simeq \mathcal {O}(1)$]]></tex-math></inline-formula>&#x2009;TeV should be implied [<xref ref-type="bibr" rid="PTV155C59">59</xref>, <xref ref-type="bibr" rid="PTV155C60">60</xref>]. For the nonsupersymmetric version, the upper bound of <inline-formula><tex-math notation="LaTeX" id="ImEquation19"><![CDATA[$\Lambda < 5$]]></tex-math></inline-formula>&#x2009;TeV seems inconsistent with recent data from precision tests [<xref ref-type="bibr" rid="PTV155C61">61</xref>, <xref ref-type="bibr" rid="PTV155C62">62</xref>]. As a solution to this problem, the SUSY version predicts a less restrictive upper bound. Additionally, the <inline-formula><tex-math notation="LaTeX" id="ImEquation20"><![CDATA[$\rho $]]></tex-math></inline-formula> parameter, one of the most important parameters for checking the precision test at low energy [<xref ref-type="bibr" rid="PTV155C63">63</xref>, <xref ref-type="bibr" rid="PTV155C64">64</xref>], still satisfies the current data if SUSY contributions are considered [<xref ref-type="bibr" rid="PTV155C65">65</xref>]. In any case, discussions on the non-SUSY version predict that the valid scale of the SUSYRM331 should be large, resulting in very heavy masses for the new particles, except a light neutral CP-even Higgs and maybe the lightest DCH. Therefore, apart from the light neutral Higgs, which can be identified with the one observed at LHC recently, the lightest DCH is the only one that may be observed by recent experiments.</p>
<p>Once again, we would like to emphasize that the RM331 model contains the minimal number of Higgses; the first way to generate consistent masses for fermions is to introduce effective operators working at the TeV scale [<xref ref-type="bibr" rid="PTV155C21">21</xref>, <xref ref-type="bibr" rid="PTV155C66">66</xref>]. Besides that, in the SUSY versions the fermion masses can be generated by including radiative corrections through the mixing of fermions and their superpartners [<xref ref-type="bibr" rid="PTV155C20">20</xref>, <xref ref-type="bibr" rid="PTV155C67">67</xref>, <xref ref-type="bibr" rid="PTV155C68">68</xref>]. Of course, in this case, the well known <inline-formula><tex-math notation="LaTeX" id="ImEquation21"><![CDATA[$R$]]></tex-math></inline-formula> parity has to be broken. Based on these results, many supersymmetric versions have been built and studied, such as SUSYE331 [<xref ref-type="bibr" rid="PTV155C69">69</xref>&#x2013;<xref ref-type="bibr" rid="PTV155C72">72</xref>], SUSYRM331 [<xref ref-type="bibr" rid="PTV155C20">20</xref>, <xref ref-type="bibr" rid="PTV155C21">21</xref>], etc. One of the intriguing features of supersymmetric theories is that the Higgs spectrum is quite constrained.</p>
<p>Our paper is organized as follows. In Sect. <xref ref-type="sec" rid="s2">2</xref>, we will briefly review the SUSYRM331 model, particularly concentrating on the Higgs and gauge boson sectors and their effect on the <inline-formula><tex-math notation="LaTeX" id="ImEquation22"><![CDATA[$\rho $]]></tex-math></inline-formula> parameter, which may indirectly affect the lower bound of the <inline-formula><tex-math notation="LaTeX" id="ImEquation23"><![CDATA[${\rm SU}(3)_L$]]></tex-math></inline-formula> scale. Furthermore, some important and interesting properties of SUSYRM331 are discussed, e.g., (i) the soft and <inline-formula><tex-math notation="LaTeX" id="ImEquation24"><![CDATA[${\rm SU}(3)_L$]]></tex-math></inline-formula> parameters should be of the same order; (ii) the model contains a light neutral CP-even Higgs with the values of the squared tree-level mass of <inline-formula><tex-math notation="LaTeX" id="ImEquation25"><![CDATA[$m^2_Z|\cos 2\gamma |+ m^2_W\times \mathcal {O}(\epsilon )$]]></tex-math></inline-formula>. Here <inline-formula><tex-math notation="LaTeX" id="ImEquation26"><![CDATA[$\gamma $]]></tex-math></inline-formula> is defined as the ratio of the two vacuum expectation values of two Higgses <inline-formula><tex-math notation="LaTeX" id="ImEquation27"><![CDATA[$\rho $]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation28"><![CDATA[$\rho '$]]></tex-math></inline-formula>, while <inline-formula><tex-math notation="LaTeX" id="ImEquation29"><![CDATA[$\epsilon $]]></tex-math></inline-formula> is defined as a quantity characterizing the ratio of the electroweak and <inline-formula><tex-math notation="LaTeX" id="ImEquation30"><![CDATA[${\rm SU}(3)_L$]]></tex-math></inline-formula> scales. Section <xref ref-type="sec" rid="s3">3</xref> is devoted to investigating in detail the masses and other properties of the DCHs. We will discuss the constraint of the DCH masses under the recent experimental value of the decay of the lightest CP-even neutral Higgs to two photons. From this, we prove that there exists a region of parameter space containing a light DCH. In Sect. <xref ref-type="sec" rid="s4">4</xref>, we discuss the creation of DCHs in <inline-formula><tex-math notation="LaTeX" id="ImEquation31"><![CDATA[$e^+e^-$]]></tex-math></inline-formula> colliders such as the ILC and CLIC. Specifically, we establish formulas for the cross sections of reactions <inline-formula><tex-math notation="LaTeX" id="ImEquation32"><![CDATA[$e^+e^-\rightarrow H^{++}H^{--}$]]></tex-math></inline-formula> in collision energies from 1&#x2013;3&#x2009;TeV and calculate the number of events for DCH creation. These cross sections and the Higgs masses are represented as functions of very convenient parameters such as the masses of neutral CP-odd Higgses, the mass of the heavy singly charged gauge boson, and <inline-formula><tex-math notation="LaTeX" id="ImEquation33"><![CDATA[$\tan \gamma $]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation34"><![CDATA[$\tan \beta $]]></tex-math></inline-formula> as ratios of Higgs vacuum expectation values (VEV), which will be defined in the work. This will help one more easily predict many properties relating to the DCHs as well as relations among the masses of particles in the model. With each collision energy level of 1.5, 2, and 3&#x2009;TeV, we discuss the parameter space where the masses of three DCHs can satisfy the allowed kinetic condition; namely, the mass of each DCH must be smaller than half of the collision energy. Then we estimate the amplitudes of the cross sections in these regions of parameter space. Finally, the branching ratios of the DCH decay to pairs of same-sign leptons are briefly discussed.</p>
</sec>
<sec id="s2"><label>2.</label><title>Review of the SUSYRM331 model</title>
<p>This work is based on the models represented in Refs. [<xref ref-type="bibr" rid="PTV155C20">20</xref>, <xref ref-type="bibr" rid="PTV155C21">21</xref>]. For convenience, we summarize the important results that will be used in our calculation. Throughout this work, we will use the notation of the two-component spinor for fermions, where <inline-formula><tex-math notation="LaTeX" id="ImEquation35"><![CDATA[$\psi $]]></tex-math></inline-formula> denotes a particle and <inline-formula><tex-math notation="LaTeX" id="ImEquation36"><![CDATA[$\psi ^c$]]></tex-math></inline-formula> denotes the corresponding antiparticle. Both <inline-formula><tex-math notation="LaTeX" id="ImEquation37"><![CDATA[$\psi $]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation38"><![CDATA[$\psi ^c$]]></tex-math></inline-formula> are left-handed spinors. In the case of Majorana fields, where <inline-formula><tex-math notation="LaTeX" id="ImEquation39"><![CDATA[$\psi =\psi ^c$]]></tex-math></inline-formula>, we will use <inline-formula><tex-math notation="LaTeX" id="ImEquation40"><![CDATA[$\psi $]]></tex-math></inline-formula> notation.</p>
<sec id="s2a"><label>2.1.</label><title>Lepton and quark sectors</title>
<p>The lepton sector is arranged based on the original nonsupersymmetric version [<xref ref-type="bibr" rid="PTV155C13">13</xref>], namely,
<disp-formula id="PTV155M1"><label>(1)</label><tex-math notation="LaTeX" id="DmEquation1"><![CDATA[\begin{equation} \hat{L}_{l} = \left(\begin{matrix} \hat{\nu}, & \hat{l}, & \hat{l}^{c} \\ \end{matrix}\right)^T\sim (\textbf{1}, \textbf{3}, 0), \quad l= e, \mu , \tau. \end{equation}]]></tex-math>
</disp-formula>
The transformation properties under the respective factors <inline-formula><tex-math notation="LaTeX" id="ImEquation41"><![CDATA[$({\rm SU(3)}_C$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation42"><![CDATA[${\rm SU(3)}_L$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation43"><![CDATA[${\rm U(1)}_X)$]]></tex-math></inline-formula> appear in parentheses.</p>
<p>In the quark sector, the first quark family is put in a superfield that transforms as a triplet of the <inline-formula><tex-math notation="LaTeX" id="ImEquation44"><![CDATA[$ {\rm SU(3)}_L$]]></tex-math></inline-formula> group:
<disp-formula id="PTV155M2"><label>(2)</label><tex-math notation="LaTeX" id="DmEquation2"><![CDATA[\begin{equation} \hat{Q}_{1L} =\left(\begin{matrix} \hat{u}_{1}, & \hat{d}_{1},& \hat{J}_{1} \\ \end{matrix} \right)\sim \left(\textbf{3},\textbf{3},\tfrac{2}{3}\right). \end{equation}]]></tex-math>
</disp-formula>
The three respective antiquark superfields are singlets of the <inline-formula><tex-math notation="LaTeX" id="ImEquation45"><![CDATA[$ {\rm SU(3)}_L$]]></tex-math></inline-formula> group:
<disp-formula id="PTV155M3"><label>(3)</label><tex-math notation="LaTeX" id="DmEquation3"><![CDATA[\begin{equation} \hat{u}^{c}_{1} \sim \left(\textbf{3}^*,\textbf{1},-\tfrac{2}{3}\right),\quad \hat{d}^{c}_{1} \sim \left(\textbf{3}^*,\textbf{1},\tfrac{1}{3}\right),\quad \hat{J}^{c}_{1} \sim \left(\textbf{3}^*,\textbf{1},-\tfrac{5}{3}\right). \end{equation}]]></tex-math>
</disp-formula>
The two remaining quark families are included in the two corresponding superfields, transforming as antitriplets:
<disp-formula id="PTV155M4"><label>(4)</label><tex-math notation="LaTeX" id="DmEquation4"><![CDATA[\begin{equation} \hat{Q}_{iL} = \left(\begin{matrix} \hat{d}_{i}, & - \hat{u}_{i} & \hat{j}_{i} \\ \end{matrix}\right)^T \sim \left(\textbf{3},\textbf{3}^{*},-\tfrac{1}{3}\right), \quad i = 2, 3. \end{equation}]]></tex-math>
</disp-formula>
and the respective antiquark superfields are singlets:
<disp-formula id="PTV155M5"><label>(5)</label><tex-math notation="LaTeX" id="DmEquation5"><![CDATA[\begin{equation} \hat{u}^{c}_{i} \sim \left(\textbf{3}^*,\textbf{1},-\tfrac{2}{3}\right),\quad \hat{d}^{c}_{i} \sim \left(\textbf{3}^*,\textbf{1},\tfrac{1}{3}\right), \quad \hat{j}^{c}_{i} \sim \left(\textbf{3}^*,\textbf{1},\tfrac{4}{3} \right), \quad i = 2, 3. \end{equation}]]></tex-math>
</disp-formula>
The SUSYRM331 needs four Higgs superfields in order to generate all masses of leptons and quarks, but radiative corrections [<xref ref-type="bibr" rid="PTV155C20">20</xref>] or effective operators [<xref ref-type="bibr" rid="PTV155C21">21</xref>] must be added. For convenience in investigating the couplings between leptons and DCHs, in this work we will use the effective approach.</p>
</sec>
<sec id="s2b"><label>2.2.</label><title>Gauge bosons and lepton&#x2013;lepton&#x2013;gauge boson vertices</title>
<p>The gauge boson sector of the SUSYRM331 model was thoroughly investigated in Refs. [<xref ref-type="bibr" rid="PTV155C20">20</xref>, <xref ref-type="bibr" rid="PTV155C21">21</xref>] and this sector is similar to that of the non-SUSY version [<xref ref-type="bibr" rid="PTV155C12">12</xref>]. According to these works, the gauge sector includes three neutral (<inline-formula><tex-math notation="LaTeX" id="ImEquation46"><![CDATA[$A$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation47"><![CDATA[$Z$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation48"><![CDATA[$Z'$]]></tex-math></inline-formula>), four singly charged (<inline-formula><tex-math notation="LaTeX" id="ImEquation49"><![CDATA[$W^{\pm }$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation50"><![CDATA[$V^{\pm }$]]></tex-math></inline-formula>), and two doubly charged <inline-formula><tex-math notation="LaTeX" id="ImEquation51"><![CDATA[$U^{\pm \pm }$]]></tex-math></inline-formula> gauge bosons. Of these, <inline-formula><tex-math notation="LaTeX" id="ImEquation52"><![CDATA[$A$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation53"><![CDATA[$Z$]]></tex-math></inline-formula>, and <inline-formula><tex-math notation="LaTeX" id="ImEquation54"><![CDATA[$W^{\pm }$]]></tex-math></inline-formula> are SM particles, while the rest are <inline-formula><tex-math notation="LaTeX" id="ImEquation55"><![CDATA[${\rm SU(3)}_L$]]></tex-math></inline-formula> particles with masses being on the <inline-formula><tex-math notation="LaTeX" id="ImEquation56"><![CDATA[${\rm SU(3)}_L$]]></tex-math></inline-formula> scale. The new charged gauge bosons <inline-formula><tex-math notation="LaTeX" id="ImEquation57"><![CDATA[$V^{\pm }$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation58"><![CDATA[$U^{\pm \pm }$]]></tex-math></inline-formula> have a lepton number of two; hence, they are also called bileptons. According to the analysis in Ref. [<xref ref-type="bibr" rid="PTV155C73">73</xref>], the mass of the charged bilepton <inline-formula><tex-math notation="LaTeX" id="ImEquation59"><![CDATA[$U$]]></tex-math></inline-formula> is always less than <inline-formula><tex-math notation="LaTeX" id="ImEquation60"><![CDATA[$0.5 m_{Z'}$]]></tex-math></inline-formula>. Therefore, we expect the decays <inline-formula><tex-math notation="LaTeX" id="ImEquation61"><![CDATA[$ Z' \rightarrow U^{++} U^{--} $]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation62"><![CDATA[$U^{\pm \pm } \rightarrow 2 l^{\pm } (l=e, \mu , \tau ) $]]></tex-math></inline-formula> to be allowed, leading to spectacular signals in future colliders. The DCHs are also bileptons, leading to a very interesting consequence: the lightest DCH may be the lightest bilepton; it only decays to a charged lepton pair. This is exactly the case in the SUSYRM331, as we will prove through this work. All the masses of the gauge bosons can be written as functions of the <inline-formula><tex-math notation="LaTeX" id="ImEquation63"><![CDATA[$W$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation64"><![CDATA[$V$]]></tex-math></inline-formula> gauge boson masses. There is a simple relation between <inline-formula><tex-math notation="LaTeX" id="ImEquation65"><![CDATA[$m_W$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation66"><![CDATA[$m_{V}$]]></tex-math></inline-formula>, and <inline-formula><tex-math notation="LaTeX" id="ImEquation67"><![CDATA[$m_{U}$]]></tex-math></inline-formula>, namely, <inline-formula><tex-math notation="LaTeX" id="ImEquation68"><![CDATA[$m^2_{U}=m^2_{W}+m^2_{V}$]]></tex-math></inline-formula>, which will be summarized in the Higgs sector. Therefore, we can define <inline-formula><tex-math notation="LaTeX" id="ImEquation69"><![CDATA[$m_V$]]></tex-math></inline-formula> as a parameter characterized for the <inline-formula><tex-math notation="LaTeX" id="ImEquation70"><![CDATA[${\rm SU(3)}_L$]]></tex-math></inline-formula> scale. Recently, the studies of flavor-neutral changing-current processes and the muon anomalous magnetic moment in the reduced minimal 3-3-1 model [<xref ref-type="bibr" rid="PTV155C74">74</xref>, <xref ref-type="bibr" rid="PTV155C75">75</xref>] have set the lower limits of <inline-formula><tex-math notation="LaTeX" id="ImEquation71"><![CDATA[$m_V$]]></tex-math></inline-formula>, namely, <inline-formula><tex-math notation="LaTeX" id="ImEquation72"><![CDATA[$m_V\geq 650$]]></tex-math></inline-formula> and 910&#x2009;GeV, respectively.</p>
<p>The vertex of <inline-formula><tex-math notation="LaTeX" id="ImEquation73"><![CDATA[$ffV$]]></tex-math></inline-formula>, which is very important in studying the creation of DCHs in <inline-formula><tex-math notation="LaTeX" id="ImEquation74"><![CDATA[$e^+e^-$]]></tex-math></inline-formula> colliders, is represented in the Lagrangian shown in Refs. [<xref ref-type="bibr" rid="PTV155C12">12</xref>, <xref ref-type="bibr" rid="PTV155C20">20</xref>, <xref ref-type="bibr" rid="PTV155C21">21</xref>, <xref ref-type="bibr" rid="PTV155C58">58</xref>], namely,
<disp-formula id="PTV155M6"><label>(6)</label><tex-math notation="LaTeX" id="DmEquation6"><![CDATA[\begin{equation} \mathcal{L}_{ffV}= g\bar{L}\bar{\sigma}^{\mu}\frac{\lambda^a}{2} L V^a_{\mu}. \end{equation}]]></tex-math>
</disp-formula>
The relations between the mass and the original states of neutral gauge bosons are given as follows:
<disp-formula id="PTV155M7"><label>(7)</label><tex-math notation="LaTeX" id="DmEquation7"><![CDATA[\begin{align} \left(\begin{matrix} W_{3\mu} \\ W_{8\mu} \\ B_{\mu} \\ \end{matrix}\right) & = \mathcal{C}_{\rm B} \left(\begin{matrix} A_{\mu} \\ Z_{\mu} \\ Z'_{\mu} \\ \end{matrix}\right) \notag \\ & = \left(\begin{matrix} \dfrac{t}{\sqrt{2\big(2t^2+3\big)}}, & \dfrac{\sqrt{3}}{2}\left(c_{\zeta}+\dfrac{s_{\zeta}}{\sqrt{2t^2+3}}\right), & \dfrac{\sqrt{3}}{2}\left(-s_{\zeta}+\dfrac{c_{\zeta}}{\sqrt{2t^2+3}}\right) \\ -\dfrac{\sqrt{3}t}{\sqrt{2\big(2t^2+3\big)}}& \dfrac{1}{2}\left(c_{\zeta}-\dfrac{3s_{\zeta}}{\sqrt{2t^2+3}}\right), & -\dfrac{1}{2}\left(s_{\zeta}+\dfrac{3c_{\zeta}}{\sqrt{2t^2+3}}\right)\\ \dfrac{\sqrt{3}}{\sqrt{2t^2+3}}&-\dfrac{\sqrt{2}s_{\zeta}t}{\sqrt{2t^2+3}} &-\dfrac{\sqrt{2}c_{\zeta}t}{\sqrt{2t^2+3}}\\ \end{matrix}\right) \left(\begin{matrix} A_{\mu} \\ Z_{\mu} \\ Z'_{\mu} \\ \end{matrix}\right). \end{align}]]></tex-math>
</disp-formula>
Here <inline-formula><tex-math notation="LaTeX" id="ImEquation75"><![CDATA[$c_{\zeta }\equiv \cos \zeta >0, s_{\zeta }\equiv \sin \zeta >0$]]></tex-math></inline-formula> with <inline-formula><tex-math notation="LaTeX" id="ImEquation76"><![CDATA[$\zeta $]]></tex-math></inline-formula> satisfying
<disp-formula id="PTV155M8"><label>(8)</label><tex-math notation="LaTeX" id="DmEquation8"><![CDATA[\begin{equation} \tan2\zeta\equiv\frac{\sqrt{\big(3 + 2 t^2\big) }\big(m_V^2 - m_W^2\big)}{\big(1+t^2\big) \big(m^2_V + m_W^2\big)}.\end{equation}]]></tex-math>
</disp-formula>
The parameter <inline-formula><tex-math notation="LaTeX" id="ImEquation77"><![CDATA[$t$]]></tex-math></inline-formula> is the ratio between <inline-formula><tex-math notation="LaTeX" id="ImEquation78"><![CDATA[$g'$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation79"><![CDATA[$g$]]></tex-math></inline-formula>, namely,
<disp-formula id="PTV155M9"><label>(9)</label><tex-math notation="LaTeX" id="DmEquation9"><![CDATA[\begin{equation} t\equiv \frac{g'}{g}=\sqrt{\frac{6\sin^2\theta_W}{1-4\sin^2\theta_W}}.\end{equation}]]></tex-math>
</disp-formula>
The masses of gauge bosons are given by
<disp-formula id="PTV155M10"><label>(10)</label><tex-math notation="LaTeX" id="DmEquation10"><![CDATA[\begin{align} m_{\gamma}&= 0,\nonumber \\ m^2_{Z}&= \frac{t^2+2}{3}\left(m^2_U-\sqrt{m_U^4-\frac{4\big(2t^2+3\big)}{\big(t^2+2\big)^2}m^2_Vm^2_W}\,\right),\nonumber \\ m^2_{Z'}&= \frac{t^2+2}{3}\left(m^2_U+\sqrt{m_U^4-\frac{4\big(2t^2+3\big)}{\big(t^2+2\big)^2}m^2_Vm^2_W}\,\right). \end{align}]]></tex-math>
</disp-formula>
The <inline-formula><tex-math notation="LaTeX" id="ImEquation80"><![CDATA[$Z$]]></tex-math></inline-formula>&#x2013;<inline-formula><tex-math notation="LaTeX" id="ImEquation81"><![CDATA[$Z'$]]></tex-math></inline-formula> mixing angle in the framework of the RM331 model is quite small, <inline-formula><tex-math notation="LaTeX" id="ImEquation82"><![CDATA[$|\phi | < 10^{-3}$]]></tex-math></inline-formula> [<xref ref-type="bibr" rid="PTV155C58">58</xref>]. It is interesting to note that, due to the generation discrimination in the 3-3-1 models, the new neutral gauge boson <inline-formula><tex-math notation="LaTeX" id="ImEquation83"><![CDATA[$Z'$]]></tex-math></inline-formula> has a flavor-changing neutral current [<xref ref-type="bibr" rid="PTV155C76">76</xref>&#x2013;<xref ref-type="bibr" rid="PTV155C78">78</xref>].</p>
<p>The above analysis is enough to calculate the vertex factors of charged leptons with neutral gauge bosons, as shown explicitly in Table <xref ref-type="table" rid="PTV155TB1">1</xref>. Here we only concentrate on the largest vertex couplings by assuming that the flavor basis of leptons and quarks is the mass basis.
<table-wrap id="PTV155TB1" position="float"><label>Table 1.</label>
<caption><p>Vertex factors between leptons, quarks, and neutral gauge bosons. Note that <inline-formula><tex-math notation="LaTeX" id="ImEquation84"><![CDATA[$e=g\sin \theta _W$]]></tex-math></inline-formula>.</p></caption>
<table frame="hsides" rules="groups">
<colgroup>
<col align="left"/>
<col align="center"/>
<col align="center"/>
<col align="center"/>
</colgroup>
<thead><tr>
<th align="left"><inline-formula><tex-math notation="LaTeX" id="ImEquation85"><![CDATA[$\bar {f}fV_{\mu }$]]></tex-math></inline-formula></th>
<th align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation86"><![CDATA[$A_{\mu }$]]></tex-math></inline-formula></th>
<th align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation87"><![CDATA[$Z_{\mu }$]]></tex-math></inline-formula></th>
<th align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation88"><![CDATA[$Z'_{\mu }$]]></tex-math></inline-formula></th>
</tr>
</thead>
<tbody><tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation89"><![CDATA[$\nu _{e}$]]></tex-math></inline-formula></td>
<td>0</td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation90"><![CDATA[$\dfrac {igc_{\zeta }}{\sqrt {3}}\bar {\sigma }^{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation91"><![CDATA[$\dfrac {-igs_{\zeta }}{\sqrt {3}}\bar {\sigma }^{\mu }$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation92"><![CDATA[$e$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation93"><![CDATA[$-ie$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation94"><![CDATA[$-\dfrac {ig}{2\sqrt {3}}\left ( c_{\zeta }+\dfrac {3s_{\zeta }}{\sqrt {2t^2+3}}\right ) \bar {\sigma }^{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation95"><![CDATA[$\dfrac {ig}{2\sqrt {3}}\left ( s_{\zeta }-\dfrac {3c_{\zeta }}{\sqrt {2t^2+3}}\right ) \bar {\sigma }^{\mu }$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation96"><![CDATA[$e^c$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation97"><![CDATA[$ie$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation98"><![CDATA[$-\dfrac {ig}{2\sqrt {3}}\left ( c_{\zeta }-\dfrac {3s_{\zeta }}{\sqrt {2t^2+3}}\right ) \bar {\sigma }^{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation99"><![CDATA[$\dfrac {ig}{2\sqrt {3}}\left ( s_{\zeta }+\dfrac {3c_{\zeta }}{\sqrt {2t^2+3}}\right ) \bar {\sigma }^{\mu }$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation100"><![CDATA[$u$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation101"><![CDATA[$\dfrac {i2e}{3}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation102"><![CDATA[$\dfrac {ig}{\sqrt {3}}\left ( c_{\zeta }-\dfrac {2t^2s_{\zeta }}{3\sqrt {2t^2+3}}\right ) \bar {\sigma }^{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation103"><![CDATA[$\dfrac {-ig}{\sqrt {3}}\left ( s_{\zeta }+\dfrac {2t^2c_{\zeta }}{3\sqrt {2t^2+3}}\right ) \bar {\sigma }^{\mu }$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation104"><![CDATA[$u^c$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation105"><![CDATA[$-\dfrac {i2e}{3}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation106"><![CDATA[$\dfrac {2igt^2s_{\zeta }}{3\sqrt {3\big (2t^2+3\big )}} \bar {\sigma }^{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation107"><![CDATA[$\dfrac {2igt^2 c_{\zeta }}{3\sqrt {3\big (2t^2+3\big )}} \bar {\sigma }^{\mu }$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation108"><![CDATA[$d$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation109"><![CDATA[$-\dfrac {ie}{3}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation110"><![CDATA[$-\dfrac {ig}{2\sqrt {3}}\left ( c_{\zeta }+\dfrac {(4t^2+9)s_{\zeta }}{3\sqrt {2t^2+3}}\right ) \bar {\sigma }^{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation111"><![CDATA[$\dfrac {ig}{2\sqrt {3}}\left ( s_{\zeta }-\dfrac {(4t^2+9)c_{\zeta }}{3\sqrt {2t^2+3}}\right ) \bar {\sigma }^{\mu }$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation112"><![CDATA[$d^c$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation113"><![CDATA[$\dfrac {ie}{3}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation114"><![CDATA[$-\dfrac {igt^2s_{\zeta }}{3\sqrt {3\big (2t^2+3\big )}} \bar {\sigma }^{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation115"><![CDATA[$-\dfrac {igt^2 c_{\zeta }}{3\sqrt {3\big (2t^2+3\big )}} \bar {\sigma }^{\mu }$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation116"><![CDATA[$J_1$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation117"><![CDATA[$\dfrac {5ie}{3}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation118"><![CDATA[$-\dfrac {ig}{2\sqrt {3}}\left ( c_{\zeta }+\dfrac {(4t^2-9)s_{\zeta }}{3\sqrt {2t^2+3}}\right ) \bar {\sigma }^{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation119"><![CDATA[$\dfrac {ig}{2\sqrt {3}}\left ( s_{\zeta }+\dfrac {(4t^2-9)c_{\zeta }}{3\sqrt {2t^2+3}}\right ) \bar {\sigma }^{\mu }$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation120"><![CDATA[$J_1^c$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation121"><![CDATA[$-\dfrac {5ie}{3}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation122"><![CDATA[$\dfrac {5igt^2s_{\zeta }}{3\sqrt {3\big (2t^2+3\big )}} \bar {\sigma }^{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation123"><![CDATA[$\dfrac {5igt^2 c_{\zeta }}{3\sqrt {3\big (2t^2+3\big )}} \bar {\sigma }^{\mu }$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation124"><![CDATA[$c, t$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation125"><![CDATA[$\dfrac {i2e}{3}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation126"><![CDATA[$\dfrac {ig}{2\sqrt {3}}\left ( c_{\zeta }+\dfrac {(2t^2+9)s_{\zeta }}{3\sqrt {2t^2+3}}\right ) \bar {\sigma }^{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation127"><![CDATA[$\dfrac {-ig}{2 \sqrt {3}}\left ( s_{\zeta }-\dfrac {(2t^2+9)c_{\zeta }}{3\sqrt {2t^2+3}}\right ) \bar {\sigma }^{\mu }$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation128"><![CDATA[$c^c, t^c$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation129"><![CDATA[$-\dfrac {i2e}{3}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation130"><![CDATA[$\dfrac {2igt^2s_{\zeta }}{3\sqrt {3\big (2t^2+3\big )}} \bar {\sigma }^{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation131"><![CDATA[$\dfrac {2igt^2 c_{\zeta }}{3\sqrt {3\big (2t^2+3\big )}} \bar {\sigma }^{\mu }$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation132"><![CDATA[$s,~b$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation133"><![CDATA[$-\dfrac {ie}{3}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation134"><![CDATA[$-\dfrac {ig}{\sqrt {3}}\left ( c_{\zeta }+\dfrac {t^2 s_{\zeta }}{3\sqrt {2t^2+3}}\right ) \bar {\sigma }^{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation135"><![CDATA[$\dfrac {ig}{\sqrt {3}}\left ( s_{\zeta }-\dfrac {4t^2c_{\zeta }}{3\sqrt {2t^2+3}}\right ) \bar {\sigma }^{\mu }$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation136"><![CDATA[$s^c,~b^c$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation137"><![CDATA[$\dfrac {ie}{3}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation138"><![CDATA[$-\dfrac {igt^2s_{\zeta }}{3\sqrt {3\big (2t^2+3\big )}} \bar {\sigma }^{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation139"><![CDATA[$-\dfrac {igt^2 c_{\zeta }}{3\sqrt {3\big (2t^2+3\big )}} \bar {\sigma }^{\mu }$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation140"><![CDATA[$j_1,~j_2$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation141"><![CDATA[$-\dfrac {4ie}{3}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation142"><![CDATA[$-\dfrac {ig}{2 \sqrt {3}}\left ( c_{\zeta }+\dfrac {(2t^2-9) s_{\zeta }}{3\sqrt {2t^2+3}}\right ) \bar {\sigma }^{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation143"><![CDATA[$-\dfrac {ig}{2\sqrt {3}}\left ( s_{\zeta }-\dfrac {(2t^2-9)c_{\zeta }}{3\sqrt {2t^2+3}}\right ) \bar {\sigma }^{\mu }$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation144"><![CDATA[$j_1^c,~j^c_2$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation145"><![CDATA[$\dfrac {4ie}{3}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation146"><![CDATA[$-\dfrac {4igt^2s_{\zeta }}{3\sqrt {3\big (2t^2+3\big )}} \bar {\sigma }^{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation147"><![CDATA[$-\dfrac {4igt^2 c_{\zeta }}{3\sqrt {3\big (2t^2+3\big )}} \bar {\sigma }^{\mu }$]]></tex-math></inline-formula></td>
</tr>
</tbody>
</table>
</table-wrap></p>
</sec>
<sec id="s2c"><label>2.3.</label><title>Constraint from the <inline-formula><tex-math notation="LaTeX" id="ImEquation148"><![CDATA[$\rho $]]></tex-math></inline-formula> parameter</title>
<p>The above analysis shows that the structure of the neutral gauge bosons is the same as that of the RM331 model when all mixing and mass parameters of these bosons are written in terms of the charged gauge boson masses. So the contributions of new heavy gauge bosons to the <inline-formula><tex-math notation="LaTeX" id="ImEquation149"><![CDATA[$\rho $]]></tex-math></inline-formula> parameter from the <inline-formula><tex-math notation="LaTeX" id="ImEquation150"><![CDATA[${\rm SU}(3)_L$]]></tex-math></inline-formula> charged gauge bosons are given in Refs. [<xref ref-type="bibr" rid="PTV155C79">79</xref>, <xref ref-type="bibr" rid="PTV155C80">80</xref>]. They also relate to the <inline-formula><tex-math notation="LaTeX" id="ImEquation151"><![CDATA[$T$]]></tex-math></inline-formula> parameter through the equality <inline-formula><tex-math notation="LaTeX" id="ImEquation152"><![CDATA[$\Delta \rho \equiv \rho -1 \simeq \widehat {\alpha }(m_Z) T$]]></tex-math></inline-formula>, where <inline-formula><tex-math notation="LaTeX" id="ImEquation153"><![CDATA[$\widehat {\alpha }(m_Z)$]]></tex-math></inline-formula> is the fine structure constant defined in the minimal scheme (<inline-formula><tex-math notation="LaTeX" id="ImEquation154"><![CDATA[$\overline {MS}$]]></tex-math></inline-formula>) at the <inline-formula><tex-math notation="LaTeX" id="ImEquation155"><![CDATA[$m_Z$]]></tex-math></inline-formula> scale [<xref ref-type="bibr" rid="PTV155C81">81</xref>]. The problem is that all of these contributions are always positive, so the total always makes the value of <inline-formula><tex-math notation="LaTeX" id="ImEquation156"><![CDATA[$\Delta \rho $]]></tex-math></inline-formula> larger than the current experimental upper bound, unless the <inline-formula><tex-math notation="LaTeX" id="ImEquation157"><![CDATA[${\rm SU}(3)_L$]]></tex-math></inline-formula> scale is larger than 9&#x2009;TeV [<xref ref-type="bibr" rid="PTV155C62">62</xref>].</p>
<p>Because the new quarks are <inline-formula><tex-math notation="LaTeX" id="ImEquation158"><![CDATA[${\rm SU}(2)_L$]]></tex-math></inline-formula> singlets, they do not contribute to the <inline-formula><tex-math notation="LaTeX" id="ImEquation159"><![CDATA[$\rho $]]></tex-math></inline-formula> parameters. The other contributions arise from Higgses and SUSY particles, including Higgsinos, gauginos, and superpartners of the fermions. Being functions of the SUSY parameters, they are completely independent of the <inline-formula><tex-math notation="LaTeX" id="ImEquation160"><![CDATA[${\rm SU}(3)_L$]]></tex-math></inline-formula> scale. The contributions of the DCHs are only from the couplings [<xref ref-type="bibr" rid="PTV155C65">65</xref>]
<disp-formula id="PTV155M11"><label>(11)</label><tex-math notation="LaTeX" id="DmEquation11"><![CDATA[\begin{equation} i c \phi^*_1\partial_{\mu}\phi_2 V^{\mu}+h.c \quad (V=W,Z)\end{equation}]]></tex-math>
</disp-formula>
of two charged Higgses <inline-formula><tex-math notation="LaTeX" id="ImEquation161"><![CDATA[$\phi _1$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation162"><![CDATA[$\phi _2$]]></tex-math></inline-formula>. According to Table <xref ref-type="table" rid="PTV155TBC4">C.4</xref>, there are only nonzero vertices of <inline-formula><tex-math notation="LaTeX" id="ImEquation163"><![CDATA[$\chi ^{++}W^-H^{-}_2$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation164"><![CDATA[$\chi ^{\prime ++}W^-H^{-}_2$]]></tex-math></inline-formula> related to DCHs. Because <inline-formula><tex-math notation="LaTeX" id="ImEquation165"><![CDATA[$\chi ^{\pm \pm }$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation166"><![CDATA[$\chi '^{\pm \pm }$]]></tex-math></inline-formula> contribute mainly to <inline-formula><tex-math notation="LaTeX" id="ImEquation167"><![CDATA[$H^{\pm \pm }_1$]]></tex-math></inline-formula> and the Goldstone <inline-formula><tex-math notation="LaTeX" id="ImEquation168"><![CDATA[$U^{\pm }$]]></tex-math></inline-formula> boson, they mix with the other two DCHs with very small factors of orders smaller than <inline-formula><tex-math notation="LaTeX" id="ImEquation169"><![CDATA[$\mathcal {O}\left (\frac {m_W^3}{m_V^3}\right )$]]></tex-math></inline-formula>. In addition, the kind of interactions given in (<xref rid="PTV155M11" ref-type="disp-formula">11</xref>) with two identical DCHs gives zero contribution to the <inline-formula><tex-math notation="LaTeX" id="ImEquation170"><![CDATA[$\rho $]]></tex-math></inline-formula> parameter [<xref ref-type="bibr" rid="PTV155C65">65</xref>]. So the total contribution of the physical DCHs to the <inline-formula><tex-math notation="LaTeX" id="ImEquation171"><![CDATA[$\rho $]]></tex-math></inline-formula> parameter is strongly suppressed.</p>
<p>Because the Higgs triplets <inline-formula><tex-math notation="LaTeX" id="ImEquation172"><![CDATA[$\rho $]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation173"><![CDATA[$\rho '$]]></tex-math></inline-formula> break <inline-formula><tex-math notation="LaTeX" id="ImEquation174"><![CDATA[${\rm SU}(2)_L$]]></tex-math></inline-formula> symmetry, they will give the main contributions to the couplings of singly charged and neutral Higgses to normal gauge bosons and therefore may significantly affect the <inline-formula><tex-math notation="LaTeX" id="ImEquation175"><![CDATA[$\rho $]]></tex-math></inline-formula> parameter. This is very similar to the case of the MSSM. In fact, the SUSYRM331 contains two CP-even neutral Higgses and two singly charged Higgses <inline-formula><tex-math notation="LaTeX" id="ImEquation176"><![CDATA[$H^{\pm }_1$]]></tex-math></inline-formula>, which behave in the same way as those in the MSSM. More explicitly, they couple with the <inline-formula><tex-math notation="LaTeX" id="ImEquation177"><![CDATA[$W$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation178"><![CDATA[$Z$]]></tex-math></inline-formula> bosons in the same way as those in the MSSM, especially in the large limit of the <inline-formula><tex-math notation="LaTeX" id="ImEquation179"><![CDATA[${\rm SU}(3)_L$]]></tex-math></inline-formula> and soft SUSY breaking scales, which is exactly the valid condition of the SUSYRM331. So the total contribution to the <inline-formula><tex-math notation="LaTeX" id="ImEquation180"><![CDATA[$\rho $]]></tex-math></inline-formula> parameter of these SUSYRM331 Higgses is nearly the same as what is found in the MSSM. In general, the contributions to the <inline-formula><tex-math notation="LaTeX" id="ImEquation181"><![CDATA[$\rho $]]></tex-math></inline-formula> parameter obtained from the investigation into the MSSM can also be used for the SUSY331 version [<xref ref-type="bibr" rid="PTV155C65">65</xref>]. The most important results are: i) all unexpected positive contributions decrease rapidly to zero when the overall sparticle mass scale is large enough, ii) the negative contribution from the Higgs scalars can reach absolute values of <inline-formula><tex-math notation="LaTeX" id="ImEquation182"><![CDATA[$10^{-4}$]]></tex-math></inline-formula>, which is the order of the recent sensitive experimental value of the <inline-formula><tex-math notation="LaTeX" id="ImEquation183"><![CDATA[$\rho $]]></tex-math></inline-formula> parameter. In the SUSYRM331 framework, the total positive SUSY contribution can be set to the order of <inline-formula><tex-math notation="LaTeX" id="ImEquation184"><![CDATA[$\mathcal {O}(10^{-4})$]]></tex-math></inline-formula>, because the soft parameters are at least of the order of the <inline-formula><tex-math notation="LaTeX" id="ImEquation185"><![CDATA[${\rm SU}(3)_L$]]></tex-math></inline-formula> scale, i.e., the TeV scale, while the total contribution from the Higgs scalar is completely different. It has a negative value when the masses of CP-odd neutral Higgses are very large and the lightest CP-even neutral Higgs reaches its largest value of <inline-formula><tex-math notation="LaTeX" id="ImEquation186"><![CDATA[$M_{Z}|\cos 2\beta |$]]></tex-math></inline-formula> at the tree level [<xref ref-type="bibr" rid="PTV155C65">65</xref>, <xref ref-type="bibr" rid="PTV155C82">82</xref>]<sup><xref ref-type="fn" rid="fn1">1</xref></sup> . Then, the contribution from the Higgs sector is
<disp-formula id="PTV155M12"><label>(12)</label><tex-math notation="LaTeX" id="DmEquation12"><![CDATA[\begin{equation} \Delta\rho^{{\rm susy}}_{{\rm H}}= \frac{3\alpha}{16\pi^2\sin^2\theta_W} f_{H}\big(\cos^22\beta,\theta_W\big), \end{equation}]]></tex-math>
</disp-formula>
where
<disp-formula id="PTV155UM1"><tex-math notation="LaTeX" id="DmEquation13"><![CDATA[\[ f_H(x,\theta_W)\equiv x\left(\frac{\ln\left(\cos^2\theta_W/x\right)}{\cos^2\theta_W-x}+ \frac{\ln x}{\cos^2\theta_W(1-x)}\right). \]]]></tex-math>
</disp-formula>
In the following, we will show that a negative <inline-formula><tex-math notation="LaTeX" id="ImEquation187"><![CDATA[$\Delta \rho ^{{\rm susy}}_{{\rm H}}$]]></tex-math></inline-formula> can cancel the new positive contributions arising from the SUSY and 3-3-1 properties. The total deviation of the <inline-formula><tex-math notation="LaTeX" id="ImEquation188"><![CDATA[$\rho $]]></tex-math></inline-formula> parameter can be divided into three parts,
<disp-formula id="PTV155M13"><label>(13)</label><tex-math notation="LaTeX" id="DmEquation14"><![CDATA[\begin{equation} \Delta\rho^{{\rm susy}}= \widehat{\alpha}(m_Z) T_{{\rm min}}+ \Delta\rho^{{\rm susy}}_{{\rm H}}+ \Delta\rho^{\prime{\rm susy}},\end{equation}]]></tex-math>
</disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation189"><![CDATA[$\Delta \rho ^{\prime {\rm susy}}$]]></tex-math></inline-formula> is the total positive contribution of the Higgsino, gaugino, and sfermion particles, and <inline-formula><tex-math notation="LaTeX" id="ImEquation190"><![CDATA[$T_{{\rm min}}$]]></tex-math></inline-formula> is the contribution from the minimal 3-3-1 framework to the oblique <inline-formula><tex-math notation="LaTeX" id="ImEquation191"><![CDATA[$T$]]></tex-math></inline-formula> parameter [<xref ref-type="bibr" rid="PTV155C79">79</xref>, <xref ref-type="bibr" rid="PTV155C80">80</xref>],
<disp-formula id="PTV155M14"><label>(14)</label><tex-math notation="LaTeX" id="DmEquation15"><![CDATA[\begin{align} T_{{\rm min}} &= \frac{3\sqrt{2}G_F}{16\pi^2 \widehat{\alpha}(m_Z)}\left[ m^2_U+m^2_V-\frac{2m^2_Um^2_V}{m^2_U-m^2_V}\ln\frac{m^2_U}{m^2_V}\right]\nonumber \\ & \quad + \frac{1}{4\pi \sin^2\theta_W}\left[ 2-\frac{m^2_Um^2_V}{m^2_U-m^2_V}\ln\frac{m^2_U}{m^2_V}+3\tan^2\theta_W\ln\frac{m^2_U}{m^2_V} \right]+\frac{m^2_{Z}-m_{Z_0}^2}{\widehat{\alpha}(m_Z)m^2_{Z}}, \end{align}]]></tex-math>
</disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation192"><![CDATA[$m_{Z}$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation193"><![CDATA[$m_{Z'}$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation194"><![CDATA[$m_U$]]></tex-math></inline-formula>, and <inline-formula><tex-math notation="LaTeX" id="ImEquation195"><![CDATA[$m_V$]]></tex-math></inline-formula> are the masses of gauge bosons predicted by the SUSYRM331. All of the experimental values are given in Ref. [<xref ref-type="bibr" rid="PTV155C81">81</xref>], namely, <inline-formula><tex-math notation="LaTeX" id="ImEquation196"><![CDATA[$m_{Z_0} = 91.1876\pm 0.0021$]]></tex-math></inline-formula>&#x2009;GeV, <inline-formula><tex-math notation="LaTeX" id="ImEquation197"><![CDATA[$m_W=80.385\pm 0.015$]]></tex-math></inline-formula>&#x2009;GeV, <inline-formula><tex-math notation="LaTeX" id="ImEquation198"><![CDATA[$\sin ^2\theta _W=0.231\,26$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation199"><![CDATA[$G_F=1.166\,3878(6)\times 10^{-5}\,{\rm GeV}^{-2}$]]></tex-math></inline-formula>, and <inline-formula><tex-math notation="LaTeX" id="ImEquation200"><![CDATA[$\widehat {\alpha }^{-1}(m_Z)=127.940\pm 0.014$]]></tex-math></inline-formula>. Also, the experimental constraint of new physics to <inline-formula><tex-math notation="LaTeX" id="ImEquation201"><![CDATA[$\Delta \rho $]]></tex-math></inline-formula> is <inline-formula><tex-math notation="LaTeX" id="ImEquation202"><![CDATA[$1.6\times 10^{-4}\leq \Delta \rho \leq 6.4\times 10^{-4}$]]></tex-math></inline-formula> [<xref ref-type="bibr" rid="PTV155C81">81</xref>]. <inline-formula><tex-math notation="LaTeX" id="ImEquation203"><![CDATA[$\Delta \rho ^{{\rm susy}}$]]></tex-math></inline-formula> is now a function of <inline-formula><tex-math notation="LaTeX" id="ImEquation204"><![CDATA[$|\cos 2\beta |$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation205"><![CDATA[$\Delta \rho ^{\prime {\rm susy}}$]]></tex-math></inline-formula>, and the <inline-formula><tex-math notation="LaTeX" id="ImEquation206"><![CDATA[${\rm SU}(3)_L$]]></tex-math></inline-formula> scale <inline-formula><tex-math notation="LaTeX" id="ImEquation207"><![CDATA[$u=\sqrt {w^2+w'^2}$]]></tex-math></inline-formula>. With the discovery of the neutral CP-even Higgs with a mass of 125 GeV, <inline-formula><tex-math notation="LaTeX" id="ImEquation208"><![CDATA[$\beta $]]></tex-math></inline-formula> should satisfy <inline-formula><tex-math notation="LaTeX" id="ImEquation209"><![CDATA[$|\cos {2\beta }|\rightarrow 1$]]></tex-math></inline-formula>. The numerical result of <inline-formula><tex-math notation="LaTeX" id="ImEquation210"><![CDATA[$\Delta \rho ^{{\rm susy}}$]]></tex-math></inline-formula> is shown in Fig. <xref ref-type="fig" rid="PTV155F1">1</xref>, where a lower bound of <inline-formula><tex-math notation="LaTeX" id="ImEquation211"><![CDATA[$u \geq 5$]]></tex-math></inline-formula>&#x2009;TeV is allowed.
<fig id="PTV155F1"><label>Fig. 1.</label>
<caption><p>Contour plot of <inline-formula><tex-math notation="LaTeX" id="ImEquation212"><![CDATA[$\Delta \rho ^{{\rm susy}}$]]></tex-math></inline-formula> as a function of <inline-formula><tex-math notation="LaTeX" id="ImEquation213"><![CDATA[$\Delta \rho ^{\prime {\rm susy}}$]]></tex-math></inline-formula> and the <inline-formula><tex-math notation="LaTeX" id="ImEquation214"><![CDATA[${\rm SU}(3)_L$]]></tex-math></inline-formula> scale <inline-formula><tex-math notation="LaTeX" id="ImEquation215"><![CDATA[$u$]]></tex-math></inline-formula>. The green region satisfies <inline-formula><tex-math notation="LaTeX" id="ImEquation216"><![CDATA[$1.6\times 10^{-4}\leq \Delta \rho ^{{\rm susy}}\leq 6.4\times 10^{-4}$]]></tex-math></inline-formula>.</p></caption>
<graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ptv15501"/>
</fig></p>
<p>Finally, what we stress here is that the sum of the respective negative and positive contributions from <inline-formula><tex-math notation="LaTeX" id="ImEquation217"><![CDATA[$\Delta \rho ^{{\rm susy}}_{H}$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation218"><![CDATA[$\Delta \rho ^{\prime {\rm susy}}$]]></tex-math></inline-formula> is enough to keep the value of the <inline-formula><tex-math notation="LaTeX" id="ImEquation219"><![CDATA[$\rho $]]></tex-math></inline-formula> parameter within the allowed constraint. Therefore, unlike the non-SUSY version, in the SUSY view, the <inline-formula><tex-math notation="LaTeX" id="ImEquation220"><![CDATA[${\rm SU}(3)_L$]]></tex-math></inline-formula> scale is free from the constraint of the <inline-formula><tex-math notation="LaTeX" id="ImEquation221"><![CDATA[$\rho $]]></tex-math></inline-formula> parameter.</p>
<p>On the other hand, the <inline-formula><tex-math notation="LaTeX" id="ImEquation222"><![CDATA[${\rm SU}(3)_L$]]></tex-math></inline-formula> scale is constrained by investigating the <inline-formula><tex-math notation="LaTeX" id="ImEquation223"><![CDATA[$Z'$]]></tex-math></inline-formula> boson. According to (<xref rid="PTV155M10" ref-type="disp-formula">10</xref>), we get
<disp-formula id="PTV155UM2"><tex-math notation="LaTeX" id="DmEquation16"><![CDATA[\[ m_{Z'}\simeq\frac{2m_V c_W }{\sqrt{3\big(1-4\sin^2\theta_W\big)}} \]]]></tex-math>
</disp-formula>
in the limit of <inline-formula><tex-math notation="LaTeX" id="ImEquation224"><![CDATA[$u\gg v,v'$]]></tex-math></inline-formula>.</p>
<p>In the framework of the minimal 3-3-1 models, the investigation of the LEP-II constraints on <inline-formula><tex-math notation="LaTeX" id="ImEquation225"><![CDATA[$m_{Z'}$]]></tex-math></inline-formula> [<xref ref-type="bibr" rid="PTV155C61">61</xref>] as well as the <inline-formula><tex-math notation="LaTeX" id="ImEquation226"><![CDATA[$B_d\rightarrow K^* \mu \mu $]]></tex-math></inline-formula> data at LHC indicates that the lower bounds of <inline-formula><tex-math notation="LaTeX" id="ImEquation227"><![CDATA[$m_{Z'}$]]></tex-math></inline-formula> must be above 7&#x2009;TeV [<xref ref-type="bibr" rid="PTV155C83">83</xref>&#x2013;<xref ref-type="bibr" rid="PTV155C85">85</xref>]. In addition, the above discussion suggests that the <inline-formula><tex-math notation="LaTeX" id="ImEquation228"><![CDATA[$Z'$]]></tex-math></inline-formula> boson in the SUSYRM331 model behaves similarly to the one in the non-SUSY version at the tree level. Combining this with the constraint of <inline-formula><tex-math notation="LaTeX" id="ImEquation229"><![CDATA[$m_{Z'}$]]></tex-math></inline-formula> in order to avoid the Landau pole, the SUSYRM331 model predicts that the most interesting range of <inline-formula><tex-math notation="LaTeX" id="ImEquation230"><![CDATA[$m_{Z'}$]]></tex-math></inline-formula> is <inline-formula><tex-math notation="LaTeX" id="ImEquation231"><![CDATA[$7\,{\rm TeV} \leq m_{Z'}\leq 9$]]></tex-math></inline-formula>&#x2009;TeV, leading to <inline-formula><tex-math notation="LaTeX" id="ImEquation232"><![CDATA[$2\,{\rm TeV}\leq m_V\leq 3\,{\rm TeV}$]]></tex-math></inline-formula>.</p>
</sec>
<sec id="s2d"><label>2.4.</label><title>Higgs sector</title>
<p>The scalar superfields, which are necessary to generate the fermion masses, are
<disp-formula id="PTV155M15"><label>(15)</label><tex-math notation="LaTeX" id="DmEquation17"><![CDATA[\begin{equation} \hat{\rho} = \left( \begin{matrix} \hat{\rho}^{+} \\ \hat{\rho}^{0} \\ \hat{\rho}^{++} \end{matrix} \right) \sim (\textbf{1},\textbf{3},+1),\quad \hat{\chi} = \left( \begin{matrix} \hat{\chi}^{-} \\ \hat{ \chi}^{--} \\ \hat{ \chi}^{0} \end{matrix} \right) \sim (\textbf{1},\textbf{3},-1). \end{equation}]]></tex-math>
</disp-formula>
To remove the chiral anomalies generated by the superpartners of the scalars, two new scalar superfields are introduced to transform as antitriplets under the <inline-formula><tex-math notation="LaTeX" id="ImEquation233"><![CDATA[${\rm SU}(3)_L$]]></tex-math></inline-formula>, namely,
<disp-formula id="PTV155M16"><label>(16)</label><tex-math notation="LaTeX" id="DmEquation18"><![CDATA[\begin{equation} \hat{\rho}^{\prime} = \left( \begin{matrix} \hat{\rho}^{\prime-} \\ \hat{\rho}^{\prime0} \\ \hat{\rho}^{\prime--} \end{matrix} \right) \sim (\textbf{1},\textbf{3}^{*},-1),\quad \hat{\chi}^{\prime} = \left( \begin{matrix} \hat{\chi}^{\prime+} \\ \hat{\chi}^{\prime++} \\ \hat{\chi}^{\prime0} \end{matrix} \right) \sim (\textbf{1},\textbf{3}^{*},+1). \end{equation}]]></tex-math>
</disp-formula>
The pattern of the symmetry breaking of the model is given by the following scheme (using the notation given in Ref. [<xref ref-type="bibr" rid="PTV155C86">86</xref>]):
<disp-formula id="PTV155M17"><label>(17)</label><tex-math notation="LaTeX" id="DmEquation19"><![CDATA[\begin{align} \hbox{SUSYRM331}&\stackrel{\mathcal{L}_{{\rm soft}}}{\longmapsto} \hbox{SU(3)}_C\ \otimes \ \hbox{SU(3)}_{L}\otimes \hbox{U(1)}_{X}\nonumber \\ &\stackrel{\langle\chi\rangle \langle \chi^{\prime}\rangle}{\longmapsto} \hbox{SU(3)}_{C} \ \otimes \ \hbox{SU(2)}_{L}\otimes \hbox{U(1)}_{Y} \nonumber \\ &\stackrel{\langle\rho\rangle \langle \rho^{\prime}\rangle}{\longmapsto} \hbox{SU(3)}_{C} \ \otimes \ \hbox{U(1)}_{Q}. \end{align}]]></tex-math>
</disp-formula>
For the sake of simplicity, all vacuum expectation values (VEVs) are supposed to be real. When the 3-3-1 symmetry is broken, i.e., <inline-formula><tex-math notation="LaTeX" id="ImEquation234"><![CDATA[${\rm SU(3)}_{C} \otimes {\rm U(1)}_{Q}$]]></tex-math></inline-formula>, the VEVs of the scalar fields are defined as follows:
<disp-formula id="PTV155M18"><label>(18)</label><tex-math notation="LaTeX" id="DmEquation20"><![CDATA[\begin{align} \langle \rho \rangle &= \left(\begin{matrix} 0, & \dfrac{v}{\sqrt{2}}, & 0 \\ \end{matrix}\right)^T,\quad \langle \chi \rangle = \left(\begin{matrix} 0, & 0, & \dfrac{w}{\sqrt{2}} \\ \end{matrix}\right)^T, \nonumber \\ \langle \rho^{\prime} \rangle &= \left(\begin{matrix} 0, & \dfrac{v'}{\sqrt{2}}, & 0 \\ \end{matrix}\right)^T,\quad \langle \chi^{\prime} \rangle = \left(\begin{matrix} 0, & 0, & \dfrac{w'}{\sqrt{2}} \\ \end{matrix}\right)^T. \end{align}]]></tex-math>
</disp-formula>
Because the symmetry breaking happens through the steps given in (<xref rid="PTV155M17" ref-type="disp-formula">17</xref>), the VEVs have to satisfy the condition <inline-formula><tex-math notation="LaTeX" id="ImEquation235"><![CDATA[$w, w^{\prime } \gg v, v{^\prime }$]]></tex-math></inline-formula>. The constraint on the <inline-formula><tex-math notation="LaTeX" id="ImEquation236"><![CDATA[$W$]]></tex-math></inline-formula> boson mass leads to the consequence that
<disp-formula id="PTV155M19"><label>(19)</label><tex-math notation="LaTeX" id="DmEquation21"><![CDATA[\begin{equation} V^{2}\equiv v^{2}+v^{\prime 2}=(246\,{\rm GeV})^2. \end{equation}]]></tex-math></disp-formula></p>
</sec>
<sec id="s2e"><label>2.5.</label><title>Higgs spectra</title>
<p>As usual, the scalar Higgs potential is written as in Ref. [<xref ref-type="bibr" rid="PTV155C20">20</xref>], except for <inline-formula><tex-math notation="LaTeX" id="ImEquation237"><![CDATA[$V_{\rm soft}$]]></tex-math></inline-formula>, which is added to the <inline-formula><tex-math notation="LaTeX" id="ImEquation238"><![CDATA[$b$]]></tex-math></inline-formula>-type terms [<xref ref-type="bibr" rid="PTV155C21">21</xref>] to guarantee the vacuum stability of the model and to avoid the appearance of many tachyon scalars [<xref ref-type="bibr" rid="PTV155C87">87</xref>, <xref ref-type="bibr" rid="PTV155C88">88</xref>]. Therefore, we have
<disp-formula id="PTV155M20"><label>(20)</label><tex-math notation="LaTeX" id="DmEquation22"><![CDATA[\begin{equation} V_{{\rm SUSYRM}331}=V_{{\rm D}}+V_{{\rm F}}+V_{{\rm soft}} \end{equation}]]></tex-math>
</disp-formula>
with
<disp-formula id="PTV155M21"><label>(21)</label><tex-math notation="LaTeX" id="DmEquation23"><![CDATA[\begin{align} V_{{\rm D}}&= -\mathcal{L}_{D}=\frac{1}{2}\left(D^{a}D^{a}+DD\right)\nonumber \\ &= \frac{g^{\prime 2}}{12}(\bar{\rho}\rho-\bar{\rho^{\prime}}\rho^{\prime} -\bar{\chi}\chi+\bar{\chi^{\prime}}\chi^{\prime})^{2} + \frac{g^{2}}{8}\sum_{i,j}\left(\bar{\rho}_{i}\lambda^{a}_{ij}\rho_{j} +\bar{\chi}_{i}\lambda^{a}_{ij}\chi_{j}- \bar{\rho^{\prime}}_{i}\lambda^{*a}_{ij}\rho^{\prime}_{j} -\bar{\chi^{\prime}}_{i}\lambda^{*a}_{ij}\chi^{\prime}_{j} \right)^{2}, \nonumber \\ V_{{\rm F}}&= -\mathcal{L}_{F}=\sum_{F}\bar{F}_{\mu}F_{\mu} = \sum_{i}\left[ \left\vert \frac{\mu_{\rho}}{2}\rho^{\prime}_{i}\right\vert^{2}+ \left\vert \frac{\mu_{\chi}}{2}\chi^{\prime}_{i}\right\vert^{2} + \left\vert \frac{\mu_{\rho}}{2}\rho_{i} \right\vert^{2}+ \left\vert \frac{\mu_{\chi}}{2}\chi_{i} \right\vert^{2} \right], \nonumber \\ V_{{\rm soft}}&= -\mathcal{L}_{{\rm SMT}}= m^{2}_{\rho}\bar{\rho}\rho+ m^{2}_{\chi}\bar{\chi}\chi+ m^{2}_{\rho^{\prime}}\bar{\rho^{\prime}}\rho^{\prime}+ m^{2}_{\chi^{\prime}}\bar{\chi^{\prime}}\chi^{\prime}- \left(b_{\rho}\rho\rho'+b_{\chi}\chi\chi'+ {\rm h.c.}\right), \end{align}]]></tex-math>
</disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation239"><![CDATA[$m_{\rho }$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation240"><![CDATA[$m_{\chi }$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation241"><![CDATA[$m_{\rho ^{\prime }}$]]></tex-math></inline-formula>, and <inline-formula><tex-math notation="LaTeX" id="ImEquation242"><![CDATA[$m_{\chi ^{\prime }}$]]></tex-math></inline-formula> have the mass dimension. Both <inline-formula><tex-math notation="LaTeX" id="ImEquation243"><![CDATA[$b_{\rho }$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation244"><![CDATA[$b_{\chi }$]]></tex-math></inline-formula> have a squared mass dimension and are assumed to be real and positive to ensure nonzero and real values for the VEVs. The expansions of the neutral scalars around their VEVs are
<disp-formula id="PTV155M22"><label>(22)</label><tex-math notation="LaTeX" id="DmEquation24"><![CDATA[\begin{align} \langle \rho \rangle&= \frac{1}{\sqrt{2}} \left( \begin{matrix} 0 \\ v+H_{\rho}+iF_{\rho} \\ 0 \end{matrix} \right), \quad \langle \rho^{\prime} \rangle=\frac{1}{\sqrt{2}} \left( \begin{matrix} 0 \\ v'+H_{\rho^{\prime}}+iF_{\rho^{\prime}}\\ 0 \end{matrix} \right), \, \nonumber \\ \langle \chi \rangle&= \frac{1}{\sqrt{2}} \left( \begin{matrix} 0 \\ 0 \\ w+H_{\chi}+iF_{\chi} \end{matrix} \right), \quad \langle \chi^{\prime} \rangle=\frac{1}{\sqrt{2}} \left( \begin{matrix} 0 \\ 0 \\ w'+H_{\chi^{\prime}}+iF_{\chi^{\prime}}\end{matrix} \right). \end{align}]]></tex-math>
</disp-formula>
The minimum of the Higgs potential corresponds to the vanishing of all linear Higgs terms in the above potential. As a result, it leads to four independent equations, shown in Ref. [<xref ref-type="bibr" rid="PTV155C21">21</xref>], which reduce to four independent parameters in the original Higgs potential. We will use the notations chosen in Ref. [<xref ref-type="bibr" rid="PTV155C20">20</xref>] for this work. In particular, two independent parameters are chosen as
<disp-formula id="PTV155M23"><label>(23)</label><tex-math notation="LaTeX" id="DmEquation25"><![CDATA[\begin{equation} t_{\gamma}=\tan\gamma=\frac{v}{v'}, \quad t_{\beta}=\tan\beta=\frac{w}{w'}. \end{equation}]]></tex-math>
</disp-formula>
These are two ratios of the VEVs of neutral Higgs scalars, and similar to the <inline-formula><tex-math notation="LaTeX" id="ImEquation245"><![CDATA[$\beta $]]></tex-math></inline-formula> parameter defined in the MSSM. The two electroweak and <inline-formula><tex-math notation="LaTeX" id="ImEquation246"><![CDATA[${\rm SU(3)}_L$]]></tex-math></inline-formula> scales relate to the masses of the <inline-formula><tex-math notation="LaTeX" id="ImEquation247"><![CDATA[$W$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation248"><![CDATA[$V$]]></tex-math></inline-formula> bosons [<xref ref-type="bibr" rid="PTV155C20">20</xref>, <xref ref-type="bibr" rid="PTV155C21">21</xref>] by two equations:
<disp-formula id="PTV155UM3"><tex-math notation="LaTeX" id="DmEquation26"><![CDATA[\[ m_W^2 = \frac{g^2}{4}\Big(v^2+v'^2\Big); \quad m_V^2=\frac{g^2}{4}\Big(w^2+w'^2\Big). \]]]></tex-math>
</disp-formula>
We can choose <inline-formula><tex-math notation="LaTeX" id="ImEquation249"><![CDATA[$m_V$]]></tex-math></inline-formula> as an independent parameter. On the other hand, there are two heavy doubly charged bosons, denoted as <inline-formula><tex-math notation="LaTeX" id="ImEquation250"><![CDATA[$U^{\pm \pm }$]]></tex-math></inline-formula>, with mass <inline-formula><tex-math notation="LaTeX" id="ImEquation251"><![CDATA[$m_U$]]></tex-math></inline-formula> satisfying <inline-formula><tex-math notation="LaTeX" id="ImEquation252"><![CDATA[$m^2_U=m^2_V+m^2_W$]]></tex-math></inline-formula>. If <inline-formula><tex-math notation="LaTeX" id="ImEquation253"><![CDATA[$m_V\gg m_W$]]></tex-math></inline-formula>, there will appear a degeneration of two heavy boson masses, <inline-formula><tex-math notation="LaTeX" id="ImEquation254"><![CDATA[$m_U= m_V+ \frac {1}{2} m_W \times \mathcal {O}\left (m_W/m_V\right ) + m_W \times \mathcal {O}\left (m_W/m_V\right )^3 \simeq m_V$]]></tex-math></inline-formula>. As mentioned above, the constraint of <inline-formula><tex-math notation="LaTeX" id="ImEquation255"><![CDATA[$m_V$]]></tex-math></inline-formula> gives a very small ratio between the two scales <inline-formula><tex-math notation="LaTeX" id="ImEquation256"><![CDATA[${\rm SU}(2)_L$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation257"><![CDATA[${\rm SU}(2)_L$]]></tex-math></inline-formula>: <inline-formula><tex-math notation="LaTeX" id="ImEquation258"><![CDATA[$m^2_W/m^2_V\leq \mathcal {O}(10^{-3})$]]></tex-math></inline-formula>. This is a rather good limit for the approximation used in this work. The minimum conditions of the superpotential result in a series of four equations:
<disp-formula id="PTV155M24"><label>(24)</label><tex-math notation="LaTeX" id="DmEquation27"><![CDATA[\begin{align} m_\rho^2+\frac{1}{4}\mu_\rho^2 &= \frac{b_\rho}{t_\gamma}-\frac{1+t^2}{3}\times m_V^2\cos{2\beta} +\frac{t^2+2} {3}\times m_W^2\cos{2\gamma}, \end{align}]]></tex-math></disp-formula>
<disp-formula id="PTV155M25"><label>(25)</label><tex-math notation="LaTeX" id="DmEquation28"><![CDATA[\begin{align} m_\chi^2+\frac{\mu_\chi^2}{4} &= \frac{b_\chi}{t_\beta}-\frac{2+t^2}{3}\times m_V^2\cos{2\beta} +\frac{1+t^2}{3}\times m_W^2\cos{2\gamma}, \end{align}]]></tex-math></disp-formula>
<disp-formula id="PTV155M26"><label>(26)</label><tex-math notation="LaTeX" id="DmEquation29"><![CDATA[\begin{align} s_{2\gamma}\equiv\sin{2\gamma}&= \frac{2b_\rho}{m_\rho^2+m_{\rho'}^2+\frac{1}{2}\mu_\rho^2},\quad s_{2\beta}\equiv\sin{2\beta}=\frac{2b_\chi}{m_\chi^2+m_{\chi'}^2+\frac{1}{2}\mu_\chi^2}. \end{align}]]></tex-math>
</disp-formula>
The two equations in (<xref rid="PTV155M26" ref-type="disp-formula">26</xref>) show the relations between the soft parameters and the ratios of the VEVs, and they are much the same as those shown in the MSSM. To estimate the scale of these soft parameters, based on the calculation in Ref. [<xref ref-type="bibr" rid="PTV155C38">38</xref>] it is useful to write Eqs. (<xref rid="PTV155M24" ref-type="disp-formula">24</xref>) and (<xref rid="PTV155M25" ref-type="disp-formula">25</xref>) in new forms, as follows:
<disp-formula id="PTV155M27"><label>(27)</label><tex-math notation="LaTeX" id="DmEquation30"><![CDATA[\begin{align} c_{2\gamma}\equiv\cos{2\gamma} & = \frac{-\left( m_\chi^2+\frac{\mu_\chi^2}{4}-\frac{b_\chi}{t_\beta}\right)\big(1+2s^2_W\big) +2\left(m_\rho^2+\frac{\mu^2_\rho}{4}-\frac{b_\rho}{t_\gamma}\right)c^2_{W}}{m^2_W}, \end{align}]]></tex-math></disp-formula>
<disp-formula id="PTV155M28"><label>(28)</label><tex-math notation="LaTeX" id="DmEquation31"><![CDATA[\begin{align} c_{2\beta}\equiv\cos{2\beta} &= \frac{\left(m_\rho^2+\frac{\mu^2_\rho}{4}-\frac{b_\rho}{t_\gamma}\right)\big(1+2s^2_W\big)- 2\left(m_\chi^2+\frac{\mu_\chi^2}{4}-\frac{b_\chi}{t_\beta}\right)c^2_W}{m^2_V}\nonumber \\ &= \frac{m_W^2}{m_V^2}\times \frac{\big(1+3t^2_W\big)c_{2\gamma}}{2} - \frac{3\big(1-4 s^2_W\big)}{2c^2_W}\times \frac{\left( m_\chi^2+\frac{\mu_\chi^2}{4}-\frac{b_\chi}{t_\beta}\right)}{m_V^2} . \end{align}]]></tex-math></disp-formula></p>
<p>Because <inline-formula><tex-math notation="LaTeX" id="ImEquation259"><![CDATA[$|c_{2\gamma }|\leq 1$]]></tex-math></inline-formula>, Eq. (<xref rid="PTV155M27" ref-type="disp-formula">27</xref>) results in a consequence: <inline-formula><tex-math notation="LaTeX" id="ImEquation260"><![CDATA[$\Big |-\Big (m_\chi ^2+\frac {\mu _\chi ^2}{4}-\frac {b_\chi }{t_\beta }\Big )\big (1+2s^2_W\big )+ 2\Big (m_\rho ^2+\frac {\mu ^2_\rho }{4}-\frac {b_\rho }{t_\gamma }\Big )c^2_{W}\Big | \leq m^2_W$]]></tex-math></inline-formula>. However, the soft-breaking parameters, such as <inline-formula><tex-math notation="LaTeX" id="ImEquation261"><![CDATA[$m^2_{\chi }$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation262"><![CDATA[$m^2_{\rho }$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation263"><![CDATA[$b_{\chi }$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation264"><![CDATA[$b_{\rho }$]]></tex-math></inline-formula>, should be much larger than <inline-formula><tex-math notation="LaTeX" id="ImEquation265"><![CDATA[$m^2_W$]]></tex-math></inline-formula>, so these parameters must be degenerate. In addition, the left-hand side of (<xref rid="PTV155M28" ref-type="disp-formula">28</xref>) also has an upper bound, <inline-formula><tex-math notation="LaTeX" id="ImEquation266"><![CDATA[$|c_{2\beta }|\leq 1$]]></tex-math></inline-formula>, as does the right-hand side. Because of the hierarchy between the two breaking scales <inline-formula><tex-math notation="LaTeX" id="ImEquation267"><![CDATA[${\rm SU(3)}_L$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation268"><![CDATA[${\rm SU(2)}_L$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation269"><![CDATA[$m_W\ll m_V$]]></tex-math></inline-formula>, the first term on the right-hand side is suppressed, and then we have <inline-formula><tex-math notation="LaTeX" id="ImEquation270"><![CDATA[$\Big |\Big (m_\chi ^2+\frac {\mu _\chi ^2}{4}-\frac {b_\chi }{t_\beta }\Big )\Big |\leq \frac {2c^2_W}{3\big (1-4 s^2_W\big )} m_V^2$]]></tex-math></inline-formula>. Hence, the two quantities <inline-formula><tex-math notation="LaTeX" id="ImEquation271"><![CDATA[$\Big (m_\chi ^2+\frac {\mu _\chi ^2}{4}-\frac {b_\chi }{t_\beta }\Big )$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation272"><![CDATA[$\Big (m_\rho ^2+\frac {\mu ^2_\rho }{4}-\frac {b_\rho }{t_\gamma }\Big )$]]></tex-math></inline-formula> are all in the <inline-formula><tex-math notation="LaTeX" id="ImEquation273"><![CDATA[${\rm SU(3)}_L$]]></tex-math></inline-formula> scale. This leads to an interesting constraint on the soft-breaking parameters of the SUSYRM331: Although the supersymmetry is spontaneously broken before the breaking of the <inline-formula><tex-math notation="LaTeX" id="ImEquation274"><![CDATA[${\rm SU}(3)_L$]]></tex-math></inline-formula> symmetry, both the soft parameters and the <inline-formula><tex-math notation="LaTeX" id="ImEquation275"><![CDATA[${\rm SU}(3)_L$]]></tex-math></inline-formula> breaking scale should be of the same order. This is a very interesting point that is not mentioned in Ref. [<xref ref-type="bibr" rid="PTV155C21">21</xref>]. This conclusion also explains why the values of parameters <inline-formula><tex-math notation="LaTeX" id="ImEquation276"><![CDATA[$b_{\rho }$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation277"><![CDATA[$b_{\chi }$]]></tex-math></inline-formula> in Ref. [<xref ref-type="bibr" rid="PTV155C21">21</xref>] are chosen in order to get consistent values of the lightest CP-even neutral Higgs mass.</p>
<p>Although the Higgs sector of the SUSYRM331 was investigated in Ref. [<xref ref-type="bibr" rid="PTV155C21">21</xref>], the two squared mass matrices of neutral Higgses and DCHs are only numerically estimated with some specific values of parameter space. However, we think that, before starting a numerical calculation, it is better to find approximate expressions of these masses in order to predict reasonable ranges of the parameters in the model, as we will show in this work. More importantly, we will show that approximate expressions are very useful in determining many interesting properties of the Higgs spectra.</p>
<p>The Higgs spectra are listed as follows:
<list list-type="order">
<list-item><p><bold>CP-odd neutral Higgses</bold>. Two massless Higgses eaten by two neutral gauge bosons are
<disp-formula id="PTV155M29"><label>(29)</label><tex-math notation="LaTeX" id="DmEquation32"><![CDATA[\begin{equation} H_{A_3}= F_{\chi'}\cos\beta-F_\chi\sin\beta, \quad H_{A_4}=F_{\rho'}\cos\gamma-F_\rho\sin\gamma. \end{equation} ]]></tex-math></disp-formula>
Two massive Higgses are expressed in terms of the original Higgses, as follows:
<disp-formula id="PTV155UM4"><tex-math notation="LaTeX" id="DmEquation33"><![CDATA[\[ H_{A_1}=F_{\rho}\cos\gamma+F_{\rho'}\sin\gamma, \quad H_{A_2}=F_{\chi}\cos\beta+F_{\chi'}\sin\beta \] ]]></tex-math></disp-formula>
and their masses are
<disp-formula id="PTV155M30"><label>(30)</label><tex-math notation="LaTeX" id="DmEquation34"><![CDATA[\begin{equation} m^2_{A_1}= \frac{2b_{\rho}}{s_{2\gamma}}=m^2_{\rho}+m^2_{\rho'}+\frac{1}{2}\mu^2_{\rho}, \quad m^2_{A_2}=\frac{2b_{\chi}}{s_{2\beta}}=m^2_{\chi}+m^2_{\chi'}+\frac{1}{2}\mu^2_{\chi}. \end{equation} ]]></tex-math></disp-formula></p></list-item>
<list-item><p><bold>Singly charged Higgses</bold>. Two massless eigenstates of these Higgses are
<disp-formula id="PTV155UM5"><tex-math notation="LaTeX" id="DmEquation35"><![CDATA[\[ H_3^{\pm} =\chi^{\pm}\sin\beta+{\chi'}^\pm\cos\beta, \quad H_4^{\pm}=\rho^{\pm}\sin\gamma+{\rho'}^\pm\cos\gamma, \] ]]></tex-math></disp-formula>
which are eaten by the singly charged gauge bosons. Two other massive states are
<disp-formula id="PTV155M31"><label>(31)</label><tex-math notation="LaTeX" id="DmEquation36"><![CDATA[\begin{align} H_1^{\pm} &= -\rho^{\pm}\cos\gamma+{\rho'}^\pm\sin\gamma, \quad m^2_{H^{\pm}_1}= m^2_{A_1}+m^2_W, \\
 H_2^{\pm} &= -\chi^{\pm}\cos\beta+{\chi'}^\pm\sin\beta, \quad m^2_{H^{\pm}_2}= m^2_{A_2} +m^2_V.\nonumber \end{align} ]]></tex-math></disp-formula></p></list-item>
<list-item><p><bold>CP-even neutral Higgses</bold>. In the basis of <inline-formula><tex-math notation="LaTeX" id="ImEquation278"><![CDATA[$(H_{\rho }$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation279"><![CDATA[$H_{\rho '}$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation280"><![CDATA[$H_{\chi }$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation281"><![CDATA[$H_{\chi '})$]]></tex-math></inline-formula>, the mass term of the neutral scalar Higgses has the form of
<disp-formula id="PTV155M32"><label>(32)</label><tex-math notation="LaTeX" id="DmEquation37"><![CDATA[\begin{equation} \mathcal{L}_{H^0} = \tfrac{1}{2}( H_{\rho}, H_{\rho'}, H_{\chi}, H_{\chi'})\times \mathcal{M}^2_{4H}\times( H_{\rho}, H_{\rho'}, H_{\chi}, H_{\chi'})^T, \end{equation} ]]></tex-math></disp-formula>
where
<disp-formula id="PTV155UM6"><tex-math notation="LaTeX" id="DmEquation38"><![CDATA[\[ M_{4H}^2=\left(\begin{matrix} m^2_{S11} & m^2_{S12} & m^2_{S13} & m^2_{S14} \\
 & m^2_{S22} & m^2_{S23} & m^2_{S24} \\
 & & m^2_{S33} & m^2_{S34} \\
 & & & m^2_{S44} \\
 \end{matrix}\right). \] ]]></tex-math></disp-formula>
Analytic formulas for the entries in the matrix were listed in Refs. [<xref ref-type="bibr" rid="PTV155C20">20</xref>, <xref ref-type="bibr" rid="PTV155C21">21</xref>]. There is a problem with finding exact analytic expressions for the eigenvalues with this matrix, which is why Ref. [<xref ref-type="bibr" rid="PTV155C21">21</xref>] had to choose the approach of numerical investigation.</p>
<p>We remind ourselves that the eigenvalues of this matrix, <inline-formula><tex-math notation="LaTeX" id="ImEquation282"><![CDATA[$\lambda =m^2_{H^0}$]]></tex-math></inline-formula>, must satisfy the equation
<disp-formula id="PTV155M33"><label>(33)</label><tex-math notation="LaTeX" id="DmEquation39"><![CDATA[\begin{equation} f(\lambda)\equiv\det\Big(M^2_{4H}-\lambda I_4\Big) = 0. \end{equation} ]]></tex-math></disp-formula>
</p>
<p>As a function of <inline-formula><tex-math notation="LaTeX" id="ImEquation283"><![CDATA[$\lambda $]]></tex-math></inline-formula>, the left-hand side of (<xref rid="PTV155M33" ref-type="disp-formula">33</xref>) is a polynomial of degree 4. Based on the very detailed discussion on Higgs spectra of the SUSYE331 in Ref. [<xref ref-type="bibr" rid="PTV155C38">38</xref>], which we will not repeat, this function can be expressed in terms of the independent parameters <inline-formula><tex-math notation="LaTeX" id="ImEquation284"><![CDATA[$m_{A_1}$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation285"><![CDATA[$m_{A_2}$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation286"><![CDATA[$c_{2\gamma }$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation287"><![CDATA[$c_{2\beta }$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation288"><![CDATA[$m_W$]]></tex-math></inline-formula>, and <inline-formula><tex-math notation="LaTeX" id="ImEquation289"><![CDATA[$m_V$]]></tex-math></inline-formula>, where <inline-formula><tex-math notation="LaTeX" id="ImEquation290"><![CDATA[$m_{A_1}$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation291"><![CDATA[$m_{A_2}$]]></tex-math></inline-formula> are soft-breaking parameters. As noted above, these soft parameters are of the same orders of the <inline-formula><tex-math notation="LaTeX" id="ImEquation292"><![CDATA[$m_V$]]></tex-math></inline-formula>&#x2013;<inline-formula><tex-math notation="LaTeX" id="ImEquation293"><![CDATA[${\rm SU}(3)_L$]]></tex-math></inline-formula> scale, i.e., <inline-formula><tex-math notation="LaTeX" id="ImEquation294"><![CDATA[$m_{A_1}/m_V$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation295"><![CDATA[$m_{A_2}/m_V\sim \mathcal {O}(1)$]]></tex-math></inline-formula>. To find approximate expressions for the Higgs masses, it is necessary to define a very small parameter: <inline-formula><tex-math notation="LaTeX" id="ImEquation296"><![CDATA[$\epsilon =\left (m^2_W/m_V^2\right )\leq \left (80.4/2000\right )^2=0.0016$]]></tex-math></inline-formula>. Then the masses of these neutral Higgses can be written as expansions of powers of <inline-formula><tex-math notation="LaTeX" id="ImEquation297"><![CDATA[$\epsilon $]]></tex-math></inline-formula>:
<disp-formula id="PTV155M34"><label>(34)</label><tex-math notation="LaTeX" id="DmEquation40"><![CDATA[\begin{align} m^2_{H^0_1}&= M^2_{Z}c^2_{2\gamma}+ \mathcal{O}\big(m_W^2\big) \times \epsilon, \nonumber \\
 m^2_{H^0_2}&= M^2_{A_1}+ \mathcal{O}\big(m_W^2\big), \nonumber \\
 m^2_{H^0_{3,4}}&= \frac{1}{6}\left[\frac{4c_W^2m_V^2}{1-4s_W^2}+3m_{A_2}^2\pm \sqrt{-\frac{48c_{2\beta}^2m_{A_2}^2m_V^2}{1-4s_W^2}+\left(3m_{A_2}^2+ \frac{4c_W^2m_V^2}{1-4s_W^2}\right)^2}\,\right] + \mathcal{O}\big(m_W^2\big). \end{align} ]]></tex-math></disp-formula>
It is necessary to note that the lightest mass has a tree-level value of <inline-formula><tex-math notation="LaTeX" id="ImEquation298"><![CDATA[$m_Z|\cos 2\gamma |\leq m_Z=92$]]></tex-math></inline-formula>&#x2009;GeV, consistent with the numerical result shown in Ref. [<xref ref-type="bibr" rid="PTV155C21">21</xref>]. Thus, the mass including loop corrections will increase to the current value of 125&#x2013;126&#x2009;GeV.</p></list-item>
</list>
</p>
<p>Although the Higgs sector was investigated in Ref. [<xref ref-type="bibr" rid="PTV155C21">21</xref>], we should emphasize a new feature in our work. To estimate the tree-level mass of the lightest CP-even Higgs, by using a reasonable approximation, we have obtained an analytic formula that is very consistent with that given in the MSSM. The interesting point is that our result depends only on the condition that all soft parameters must be in the <inline-formula><tex-math notation="LaTeX" id="ImEquation299"><![CDATA[${\rm SU}(3)_L$]]></tex-math></inline-formula> scale. The result also suggests that the <inline-formula><tex-math notation="LaTeX" id="ImEquation300"><![CDATA[$\gamma $]]></tex-math></inline-formula> parameter in the SUSYRM331 model plays a very similar role to the <inline-formula><tex-math notation="LaTeX" id="ImEquation301"><![CDATA[$\beta $]]></tex-math></inline-formula> parameter in the MSSM, defined as the ratio of two VEVs. This approximation is very useful for estimating masses as well as predicting many interesting properties of the DCHs, as we will do in this work. The authors of Ref. [<xref ref-type="bibr" rid="PTV155C21">21</xref>] also considered only the top quark and its superpartner for investigating one-loop corrections to the mass of the lightest neutral Higgs, then used this allowed value to constrain the masses of the DCHs. However, unlike the MSSM, the SUSYRM331 contains new heavy exotic quarks and their superpartners, leading to the fact that their loop corrections to the mass of the lightest neutral Higgs have to be considered. Because the masses of these new quarks are arbitrary, one cannot tell much about the constraints of charged Higgs masses from considering these loop corrections.</p>
<p>The approximate formula (<xref rid="PTV155M34" ref-type="disp-formula">34</xref>) of neutral Higgs masses is useful for finding mass eigenstates of the neutral Higgses. We will consider the two following rotations for the squared mass matrix of neutral Higgses appearing in (<xref rid="PTV155M32" ref-type="disp-formula">32</xref>):
<disp-formula id="PTV155M35"><label>(35)</label><tex-math notation="LaTeX" id="DmEquation41"><![CDATA[\begin{equation} C^{{\rm n}}_1 = \left(\begin{matrix} -c_{\gamma} &s_{\gamma} & 0 & 0 \\ s_{\gamma} & c_{\gamma} & 0 & 0 \\ 0 & 0 & 1 & 0 \\ 0 & 0 & 0 & 1 \\ \end{matrix} \right), \quad C^{{\rm n}}_2 = \left(\begin{matrix} 1& & 0 & 0 \\ 0 & c_{\alpha} & -s_{\alpha} & 0 \\ 0 & s_{\alpha} & c_{\alpha} &0 \\ 0 & 0 & 0 & 1 \\ \end{matrix}\right), \end{equation}]]></tex-math></disp-formula></p>
<p>where <inline-formula><tex-math notation="LaTeX" id="ImEquation302"><![CDATA[$s_{\alpha }\equiv \sin \alpha $]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation303"><![CDATA[$c_{\alpha }\equiv \cos \alpha $]]></tex-math></inline-formula> will be defined later. Taking the first rotation, we obtain
<disp-formula id="PTV155M36"><label>(36)</label><tex-math notation="LaTeX" id="DmEquation42"><![CDATA[\begin{align} & C^{n}_1 M^2_{4H}C^{nT}_1 \nonumber \\ & \quad = \left(\begin{matrix} m^2_{A_1}+\dfrac{2c^2_{2\gamma}\big(t^2+2\big)}{3}m^2_W&\dfrac{s_{4\gamma}\big(t^2+2\big)}{3}m^2_W & \dfrac{2s_{2\gamma}s_{\beta}\big(t^2+1\big)}{3}m_W m_V & - \dfrac{2s_{2\gamma}c_{\beta}\big(t^2+1\big)}{3}m_W m_V \\ &\dfrac{2c^2_{2\gamma}\big(t^2+2\big)}{3}m^2_W & \dfrac{2c_{2\gamma}s_{\beta}\big(t^2+1\big)}{3}m_W m_V & -\dfrac{2c_{2\gamma}c_{\beta}\big(t^2+1\big)}{3}m_W m_V \\ & & c^2_{\beta}m^2_{A_2}+ \dfrac{2s^2_{\beta}\big(t^2+2\big)}{3}m_V^2& s_{2\beta}\left[ \dfrac{m^2_{A_2}}{2}+\big(t^2+2\big)m^2_V\right] \\ & & & s^2_{\beta}m^2_{A_2}+ \dfrac{2c^2_{\beta}\big(t^2+2\big)}{3}m_V^2 \end{matrix}\right). \end{align}]]></tex-math>
</disp-formula>
The first diagonal entry of (<xref rid="PTV155M36" ref-type="disp-formula">36</xref>) is equal to the largest contribution to <inline-formula><tex-math notation="LaTeX" id="ImEquation304"><![CDATA[$m^2_{H_2^0}$]]></tex-math></inline-formula>, and the submatrix, including entries <inline-formula><tex-math notation="LaTeX" id="ImEquation305"><![CDATA[$\left ( C^{n}_1 M^2_{4H}C^{nT}_1\right )_{(i,j=4,5)}$]]></tex-math></inline-formula>, gives two other values of heavy masses <inline-formula><tex-math notation="LaTeX" id="ImEquation306"><![CDATA[$m^2_{H^0_3}$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation307"><![CDATA[$m^2_{H^0_4}$]]></tex-math></inline-formula>, while the entry <inline-formula><tex-math notation="LaTeX" id="ImEquation308"><![CDATA[$\left ( C^{n}_1 M^2_{4H}C^{nT}_1\right )_{33} = \frac {2c^2_{2\gamma } \big (t^2+2\big )}{3}m^2_W=\mathcal {O}\big (m^2_W\big )$]]></tex-math></inline-formula> relates to the lightest Higgs mass, but is different from that shown in (<xref rid="PTV155M34" ref-type="disp-formula">34</xref>). To get the right value, it must take more contributions from nondiagonal attempts containing factors <inline-formula><tex-math notation="LaTeX" id="ImEquation309"><![CDATA[$m_Wm_V$]]></tex-math></inline-formula> after taking other rotations. As mentioned above, the most interesting values of <inline-formula><tex-math notation="LaTeX" id="ImEquation310"><![CDATA[$\alpha $]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation311"><![CDATA[$\beta $]]></tex-math></inline-formula> satisfy <inline-formula><tex-math notation="LaTeX" id="ImEquation312"><![CDATA[$c_{2\gamma },c_{2\beta }\rightarrow -1$]]></tex-math></inline-formula>, i.e., <inline-formula><tex-math notation="LaTeX" id="ImEquation313"><![CDATA[$s_{\gamma ,\beta }\rightarrow 1$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation314"><![CDATA[$c_{\gamma ,\beta }\rightarrow 0$]]></tex-math></inline-formula>. This suggests that the largest correction to the lightest mass is from the entries <inline-formula><tex-math notation="LaTeX" id="ImEquation315"><![CDATA[$\left ( C^{n}_1 M^2_{4H}C^{nT}_1\right )_{23}$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation316"><![CDATA[$\left ( C^{n}_1 M^2_{4H}C^{nT}_1\right )_{32}$]]></tex-math></inline-formula>. So, taking the second rotation with <inline-formula><tex-math notation="LaTeX" id="ImEquation317"><![CDATA[$C^{{\rm n}}_2$]]></tex-math></inline-formula> given in (<xref rid="PTV155M35" ref-type="disp-formula">35</xref>) and using the limits <inline-formula><tex-math notation="LaTeX" id="ImEquation318"><![CDATA[$m_W^2\ll m^2_{V}$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation319"><![CDATA[$c_{\beta }\rightarrow 0$]]></tex-math></inline-formula>, it is easy to confirm that <inline-formula><tex-math notation="LaTeX" id="ImEquation320"><![CDATA[$\left ( C^{n}_2 C^{n}_1 M^2_{4H}(C^{n}_2C^{n}_1)^T\right )_{(22)}\simeq m^2_{Z}|c_{2\gamma }|$]]></tex-math></inline-formula> with <inline-formula><tex-math notation="LaTeX" id="ImEquation321"><![CDATA[$\alpha $]]></tex-math></inline-formula> determined by
<disp-formula id="PTV155M37"><label>(37)</label><tex-math notation="LaTeX" id="DmEquation43"><![CDATA[\begin{equation} \tan{2\alpha}\equiv \frac{ 4 c_{2\gamma}s_{\beta}\big(t^2+1\big)m_Wm_V}{3c^3_{\beta}m^2_{A_2}+2 s^2_{\beta}\big(t^2+2\big)m^2_V-2c^2_{2\gamma}\big(t^2+2\big)m^2_{W}}\sim \mathcal{O}(m_W/mV). \end{equation}]]></tex-math>
</disp-formula>
Then we can estimate that the contributions of the original Higgs states to the mass eigenstates of the CP-even neutral Higgses <inline-formula><tex-math notation="LaTeX" id="ImEquation322"><![CDATA[$H^0_1$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation323"><![CDATA[$H^0_2$]]></tex-math></inline-formula> are
<disp-formula id="PTV155M38"><label>(38)</label><tex-math notation="LaTeX" id="DmEquation44"><![CDATA[\begin{equation} H_{\rho}\rightarrow c_{\alpha} s_{\gamma} H^0_1-c_{\gamma}H^0_{2}, \quad H_{\rho'}\rightarrow c_{\alpha} c_{\gamma} H^0_1+ s_{\gamma}H^0_{2}, \quad H_{\chi}, H_{\chi'}\rightarrow \mathcal{O}(s_{\alpha}) H^0_1. \end{equation}]]></tex-math>
</disp-formula>
It is interesting that, in the decoupling regime where the SUSY and <inline-formula><tex-math notation="LaTeX" id="ImEquation324"><![CDATA[${\rm SU}(3)_L$]]></tex-math></inline-formula> scales are much larger than the <inline-formula><tex-math notation="LaTeX" id="ImEquation325"><![CDATA[${\rm SU}(2)_L$]]></tex-math></inline-formula> scale, we have <inline-formula><tex-math notation="LaTeX" id="ImEquation326"><![CDATA[$H_{\rho }\simeq s_{\gamma } H^0_1 -c_{\gamma }H^0_{2}$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation327"><![CDATA[$H_{\rho '} \simeq c_{\gamma } H^0_1+ s_{\gamma }H^0_{2}$]]></tex-math></inline-formula>, the same as those given in the MSSM [<xref ref-type="bibr" rid="PTV155C82">82</xref>]. Therefore, all couplings of these two Higgses with <inline-formula><tex-math notation="LaTeX" id="ImEquation328"><![CDATA[$W^{\pm }$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation329"><![CDATA[$Z$]]></tex-math></inline-formula> bosons are the same as those in the MSSM. More interestingly, the SUSYRM331 contains a set of Higgses including <inline-formula><tex-math notation="LaTeX" id="ImEquation330"><![CDATA[$m_{H^0_{1,2}}$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation331"><![CDATA[$m_{A_1}$]]></tex-math></inline-formula>, and <inline-formula><tex-math notation="LaTeX" id="ImEquation332"><![CDATA[$m_{H^{\pm }_1}$]]></tex-math></inline-formula> that has similar properties to the Higgs spectra of the MSSM. This property of the SUSY versions of the 3-3-1 models has also been indicated previously [<xref ref-type="bibr" rid="PTV155C38">38</xref>]. As a result, the SUSY Higgs contributions to the <inline-formula><tex-math notation="LaTeX" id="ImEquation333"><![CDATA[$\rho $]]></tex-math></inline-formula> parameter are the same in both MSSM and SUSYRM331 in the decoupling regime.</p>
<p>At the tree level, the above analysis indicates that the Higgs spectra can be determined by unknown independent parameters: <inline-formula><tex-math notation="LaTeX" id="ImEquation334"><![CDATA[$\gamma $]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation335"><![CDATA[$\beta $]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation336"><![CDATA[$m_V$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation337"><![CDATA[$m_{A_1}$]]></tex-math></inline-formula>, and <inline-formula><tex-math notation="LaTeX" id="ImEquation338"><![CDATA[$m_{A_2}$]]></tex-math></inline-formula>. Furthermore, the squared mass matrices of both CP-even neutral Higgses and DCHs depend explicitly on <inline-formula><tex-math notation="LaTeX" id="ImEquation339"><![CDATA[$c_{2\beta }$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation340"><![CDATA[$s_{2\beta }$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation341"><![CDATA[$c_{2\gamma }$]]></tex-math></inline-formula>, and <inline-formula><tex-math notation="LaTeX" id="ImEquation342"><![CDATA[$s_{2\gamma }$]]></tex-math></inline-formula> but not <inline-formula><tex-math notation="LaTeX" id="ImEquation343"><![CDATA[$t_{2\gamma }$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation344"><![CDATA[$t_{2\beta }$]]></tex-math></inline-formula>. Hence, it can be guessed that the Higgs masses will not increase to infinity when <inline-formula><tex-math notation="LaTeX" id="ImEquation345"><![CDATA[$t_{\gamma }$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation346"><![CDATA[$t_{\beta }$]]></tex-math></inline-formula> are very large. In addition, in some cases, we can take the limits <inline-formula><tex-math notation="LaTeX" id="ImEquation347"><![CDATA[$c_{2\beta ,2\gamma }\rightarrow -1$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation348"><![CDATA[$s_{2\beta ,2\gamma }\rightarrow 0$]]></tex-math></inline-formula> without any inconsistent calculations. We will use the limit <inline-formula><tex-math notation="LaTeX" id="ImEquation349"><![CDATA[$2\,{\rm TeV}\leq m_V \leq 3$]]></tex-math></inline-formula>&#x2009;TeV based on the latest update discussed above. <inline-formula><tex-math notation="LaTeX" id="ImEquation350"><![CDATA[$m_{A_1}$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation351"><![CDATA[$m_{A_2}$]]></tex-math></inline-formula> are of the same order of <inline-formula><tex-math notation="LaTeX" id="ImEquation352"><![CDATA[$m_V$]]></tex-math></inline-formula> so we set <inline-formula><tex-math notation="LaTeX" id="ImEquation353"><![CDATA[$m_{A_1}$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation354"><![CDATA[$m_{A_2}\geq 1$]]></tex-math></inline-formula>&#x2009;TeV in our calculation. Other well known values that will be used are the mass of the <inline-formula><tex-math notation="LaTeX" id="ImEquation355"><![CDATA[$W$]]></tex-math></inline-formula> boson <inline-formula><tex-math notation="LaTeX" id="ImEquation356"><![CDATA[$m_W=80.4$]]></tex-math></inline-formula>&#x2009;GeV, the sine of the Weinberg angle <inline-formula><tex-math notation="LaTeX" id="ImEquation357"><![CDATA[$s_W=0.231$]]></tex-math></inline-formula>, and the mass and total decay width of the <inline-formula><tex-math notation="LaTeX" id="ImEquation358"><![CDATA[$Z$]]></tex-math></inline-formula> boson <inline-formula><tex-math notation="LaTeX" id="ImEquation359"><![CDATA[$m_Z= 91.2$]]></tex-math></inline-formula>&#x2009;GeV, <inline-formula><tex-math notation="LaTeX" id="ImEquation360"><![CDATA[$\Gamma _Z=2.46$]]></tex-math></inline-formula>&#x2009;GeV. The discovery of the lightest CP-even Higgs mass of 125&#x2009;GeV implies that <inline-formula><tex-math notation="LaTeX" id="ImEquation361"><![CDATA[$|c_{2\gamma }| \simeq 1$]]></tex-math></inline-formula>, i.e., <inline-formula><tex-math notation="LaTeX" id="ImEquation362"><![CDATA[$t_{\gamma }$]]></tex-math></inline-formula> should be large enough, similar to the case of the MSSM. As a consequence, relation (<xref rid="PTV155M27" ref-type="disp-formula">27</xref>) shows the fine tuning among soft parameters and relation (<xref rid="PTV155M28" ref-type="disp-formula">28</xref>) predicts that <inline-formula><tex-math notation="LaTeX" id="ImEquation363"><![CDATA[$|c_{2\beta }|$]]></tex-math></inline-formula> should also be large. Therefore, we will fix <inline-formula><tex-math notation="LaTeX" id="ImEquation364"><![CDATA[$t_{\beta }=5$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation365"><![CDATA[$t_{\gamma }=10$]]></tex-math></inline-formula> in the numerical investigation that can be applied for the general case of large <inline-formula><tex-math notation="LaTeX" id="ImEquation366"><![CDATA[$t_{\beta }$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation367"><![CDATA[$t_{\gamma }$]]></tex-math></inline-formula>. This can be understood from the reason that all quantities that we consider below depend on <inline-formula><tex-math notation="LaTeX" id="ImEquation368"><![CDATA[$\gamma $]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation369"><![CDATA[$2\gamma $]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation370"><![CDATA[$\beta $]]></tex-math></inline-formula>, and <inline-formula><tex-math notation="LaTeX" id="ImEquation371"><![CDATA[$2\beta $]]></tex-math></inline-formula> only by sine or cosine factors, not tan functions.</p>
</sec>
</sec>
<sec id="s3"><label>3.</label><title>Doubly charged Higgs bosons and couplings</title>
<sec id="s3a"><label>3.1.</label><title>Mass spectra and properties of the lightest DCH</title>
<p>Consider the DCHs; the SUSYE331 model contains 8 degrees of freedom after final symmetry breaking. Therefore, the squared mass matrix is <inline-formula><tex-math notation="LaTeX" id="ImEquation372"><![CDATA[$4\times 4$]]></tex-math></inline-formula> and we cannot find the exact expressions for the physical masses. We will treat them the same as the neutral CP-even Higgses, in much more detail to discover all possible interesting properties of the DCHs, especially the lightest.</p>
<p>The mass term of the doubly charged boson is:
<disp-formula id="PTV155UM7"><tex-math notation="LaTeX" id="DmEquation45"><![CDATA[\[ \mathcal{L}_{H^{\pm\pm}}= \left(\begin{matrix} \rho^{++}, & \rho^{\prime++}, &\chi^{++}, & \chi^{\prime++} \\ \end{matrix}\right) \mathcal{M}^2_{H^{\pm\pm}} \left(\begin{matrix} \rho^{--} & \rho^{\prime--} &\chi^{--} & \chi^{\prime--} \\ \end{matrix}\right)^T, \]]]></tex-math>
</disp-formula>
where the elements of the squared mass matrix were shown precisely in Ref. [<xref ref-type="bibr" rid="PTV155C21">21</xref>]. Taking a rotation characterized by a matrix
<disp-formula id="PTV155M39"><label>(39)</label><tex-math notation="LaTeX" id="DmEquation46"><![CDATA[\begin{equation} C_1 = \left(\begin{matrix} \dfrac{-m_W s_{\gamma}}{m_U} & 0 & c_{\gamma} & \dfrac{m_V s_{\gamma}}{m_U} \\ \dfrac{-m_W c_{\gamma}}{m_U} & 0 & -s_{\gamma} & \dfrac{m_V c_{\gamma}}{m_U}\\ \dfrac{m_V s_{\beta}}{m_U} & -c_{\beta} & 0 &\dfrac{m_W s_{\beta}}{m_U} \\ \dfrac{m_Vc_{\beta}}{m_U} & s_{\beta} & 0 & \dfrac{m_W c_{\beta}}{m_U} \\ \end{matrix}\right),\end{equation}]]></tex-math>
</disp-formula>
we get new squared mass matrix:
<disp-formula id="PTV155M40"><label>(40)</label><tex-math notation="LaTeX" id="DmEquation47"><![CDATA[\begin{align} \mathcal{M}^2_{H^{\prime\pm\pm}} & \equiv C_1^T \mathcal{M}^2_{H^{\pm\pm}}C_1 \notag \\ & \quad = \left( \begin{matrix} 0 & 0 & 0 & 0 \\ 0 & m^2_{A_2}+m^2_V-c_{2\beta}c_{2\gamma}m^2_W & -s_{2\beta} s_{2\gamma}m_V m_W &c_{2\gamma}s_{2\beta} m_U m_W \\ 0 & -s_{2\beta} s_{2\gamma}m_V m_W & m_{A_1}^2 - c_{2\beta} c_{2\gamma} m_V^2 + m_W^2 & -s_{2\gamma} c_{2\beta}m_U m_V \\ 0 & c_{2\gamma}s_{2\beta} m_U m_W & -s_{2\gamma}c_{2\beta}m_U m_V & c_{2\gamma}c_{2\beta}m^2_U \\ \end{matrix}\right). \end{align}]]></tex-math>
</disp-formula>
Corresponding to the massless solution in (<xref rid="PTV155M40" ref-type="disp-formula">40</xref>), the Goldstone boson eaten by the doubly charged gauge boson is represented exactly in term of the original Higgses:
<disp-formula id="PTV155M41"><label>(41)</label><tex-math notation="LaTeX" id="DmEquation48"><![CDATA[\begin{equation} G^{\pm\pm}= -\frac{m_W s_{\gamma}}{m_U} \rho^{\pm\pm}-\frac{m_W c_{\gamma}}{m_U} \rho^{\prime\pm\pm}+\frac{m_Vs_{\beta}}{m_U} \chi^{\pm\pm}+\frac{m_V c_{\beta}}{m_U} \chi^{\prime\pm\pm}. \end{equation}]]></tex-math>
</disp-formula>
Because <inline-formula><tex-math notation="LaTeX" id="ImEquation373"><![CDATA[$m_W\ll m_U$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation374"><![CDATA[$m_V\simeq m_U$]]></tex-math></inline-formula>, and <inline-formula><tex-math notation="LaTeX" id="ImEquation375"><![CDATA[$s_{\gamma }\leq 1$]]></tex-math></inline-formula>, the doubly charged gauge boson couples weakly to light Higgses but strongly to heavy Higgses.</p>
<p>The squared mass matrix of the DCHs (<xref rid="PTV155M40" ref-type="disp-formula">40</xref>) also shows that, if there exists a light DCH (i.e., <inline-formula><tex-math notation="LaTeX" id="ImEquation376"><![CDATA[$ \sim \mathcal {O}\big (m^2_W\big )$]]></tex-math></inline-formula>), then the contributions of the off-diagonal entries to the mass of this Higgs are large. Then it is difficult to find an analytic formula for both mass eigenstates and eigenvalues. Note that, apart from the Goldstone boson (<xref rid="PTV155M41" ref-type="disp-formula">41</xref>), there are three other states denoted by <inline-formula><tex-math notation="LaTeX" id="ImEquation377"><![CDATA[$H'^{\pm \pm }_i, \, (i=1,2,3)$]]></tex-math></inline-formula>. They relate to the original DCHs by a transformation:
<disp-formula id="PTV155M42"><label>(42)</label><tex-math notation="LaTeX" id="DmEquation49"><![CDATA[\begin{equation} \left(\begin{matrix} \rho^{\pm\pm}, & \rho^{\prime\pm\pm}, & \chi^{\pm\pm}, & \chi^{\prime\pm\pm} \end{matrix}\right)^T=C_1\left(\begin{matrix} G^{\pm\pm}, & H^{\prime\pm\pm}_1,& H^{\prime\pm\pm}_2, & H^{\prime\pm\pm}_3 \end{matrix}\right)^T. \end{equation}]]></tex-math>
</disp-formula>
We assume that the three physical DCHs relate to <inline-formula><tex-math notation="LaTeX" id="ImEquation378"><![CDATA[$(H^{\prime \pm \pm }_1$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation379"><![CDATA[$H^{\prime \pm \pm }_2$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation380"><![CDATA[$H^{\prime \pm \pm }_3 )$]]></tex-math></inline-formula> by a <inline-formula><tex-math notation="LaTeX" id="ImEquation381"><![CDATA[$3\times 3$]]></tex-math></inline-formula> matrix <inline-formula><tex-math notation="LaTeX" id="ImEquation382"><![CDATA[$\Lambda $]]></tex-math></inline-formula> as follows:
<disp-formula id="PTV155M43"><label>(43)</label><tex-math notation="LaTeX" id="DmEquation50"><![CDATA[\begin{equation} \left(H^{\prime\pm\pm}_1,\,H^{\prime\pm\pm}_2,\,H^{\prime\pm\pm}_3 \right)^T= \Lambda \left(H^{\pm\pm}_1,\,H^{\pm\pm}_2,\,H^{\pm\pm}_3 \right)^T. \end{equation}]]></tex-math>
</disp-formula>
To estimate the values of the entries in the matrix <inline-formula><tex-math notation="LaTeX" id="ImEquation383"><![CDATA[$\Lambda $]]></tex-math></inline-formula>, we firstly find out some properties of the mass eigenvalues of the DCHs. The remaining three eigenvalues of this matrix <inline-formula><tex-math notation="LaTeX" id="ImEquation384"><![CDATA[$\lambda =m_{H^{\pm \pm }}^{2}$]]></tex-math></inline-formula> must satisfy the equation <inline-formula><tex-math notation="LaTeX" id="ImEquation385"><![CDATA[$\det \Big (\mathcal {M}^2_{H^{\pm \pm }} - \lambda I_4\Big ) = 0$]]></tex-math></inline-formula>, or, equivalently, <inline-formula><tex-math notation="LaTeX" id="ImEquation386"><![CDATA[$\lambda f(\lambda )=0$]]></tex-math></inline-formula> with
<disp-formula id="PTV155M44"><label>(44)</label><tex-math notation="LaTeX" id="DmEquation51"><![CDATA[\begin{equation} f(\lambda)=a\lambda^3+b\lambda^2+c\lambda+d,\end{equation}]]></tex-math>
</disp-formula>
where
<disp-formula id="PTV155M45"><label>(45)</label><tex-math notation="LaTeX" id="DmEquation52"><![CDATA[\begin{align} a&= -\Big(m^2_V + m^2_{A_1} +m^2_{A_2}+m^2_W\Big), \nonumber \\ b&= -c_{2\beta}^2 m^4_{V}+ m^2_{A_1}\left( m^2_V+c_{2\beta} c_{2\gamma}+ m^2_{A_2} \right)+\left[m^2_{A_2} + c_{2\beta} c_{2\gamma} \Big(2 m^2_V + m^2_{A_2}\Big)\right]m^2_W -c_{2\gamma}^2 m^4_W, \nonumber \\ c&= \left(m^2_V +m^2_W\right)\left[c_{2\beta} m^2_V- c_{2\gamma} \Big(m^2_W +m^2_{A_1}\Big)\right] \left[c_{2\beta}\Big(m^2_V+m^2_{A_2}\Big) - c_{2\gamma}m^2_W\right]. \end{align}]]></tex-math>
</disp-formula>
This equation gives three solutions corresponding to three masses of the physical DCHs at the tree level. We denote them as <inline-formula><tex-math notation="LaTeX" id="ImEquation387"><![CDATA[$m^2_{H^{\pm \pm }_i}$]]></tex-math></inline-formula> with <inline-formula><tex-math notation="LaTeX" id="ImEquation388"><![CDATA[$i=1,2,3$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation389"><![CDATA[$m^2_{H^{\pm \pm }_1}, m^2_{H^{\pm \pm }_2}>m^2_{H^{\pm \pm }_3}$]]></tex-math></inline-formula>. Combining the last equation of (<xref rid="PTV155M45" ref-type="disp-formula">45</xref>) with Vieta&#x0027;s formula, in order to avoid the appearance of tachyons, we deduce that
<disp-formula id="PTV155M46"><label>(46)</label><tex-math notation="LaTeX" id="DmEquation53"><![CDATA[\begin{equation} m_{H^{\pm\pm}_1}^{2}m_{H^{\pm\pm}_2}^{2}m_{H^{\pm\pm}_3}^{2} =-c>0 \Longleftrightarrow \frac{\left(m^2_{A_1}+m^2_W\right) c_{2\gamma}}{m^2_V} <c_{2\beta}<\frac{m^2_W c_{2\gamma}}{m^2_V+m_{A_2}^2}<0. \end{equation}]]></tex-math>
</disp-formula>
Furthermore, the entry <inline-formula><tex-math notation="LaTeX" id="ImEquation390"><![CDATA[$ ()_{22}$]]></tex-math></inline-formula> of (<xref rid="PTV155M40" ref-type="disp-formula">40</xref>) suggests that, if <inline-formula><tex-math notation="LaTeX" id="ImEquation391"><![CDATA[$ m^2_{A_1}$]]></tex-math></inline-formula> is enough close to <inline-formula><tex-math notation="LaTeX" id="ImEquation392"><![CDATA[$m^2_V$]]></tex-math></inline-formula>, there may appear one light DCH, while the other two values are always in the <inline-formula><tex-math notation="LaTeX" id="ImEquation393"><![CDATA[${\rm SU(3)}_L$]]></tex-math></inline-formula> scale. So, in order to find the best approximate formulas of the vertex factors <inline-formula><tex-math notation="LaTeX" id="ImEquation394"><![CDATA[$V^0H^{++}H^{--}$]]></tex-math></inline-formula>, it is better to investigate the mass values of the DCHs using the techniques shown in Ref. [<xref ref-type="bibr" rid="PTV155C38">38</xref>], and partly mentioned when discussing the neutral CP-even Higgs sector. The masses can be expanded as
<disp-formula id="PTV155M47"><label>(47)</label><tex-math notation="LaTeX" id="DmEquation54"><![CDATA[\begin{equation} m^2_{H^{\pm \pm}}= X' m^2_V + X''\times m^2_W+ \mathcal{O}(\epsilon)\times m^2_W. \end{equation}]]></tex-math>
</disp-formula>
The heavy Higgses satisfy the condition <inline-formula><tex-math notation="LaTeX" id="ImEquation395"><![CDATA[$X' \sim \mathcal {O}(1)$]]></tex-math></inline-formula>, i.e., in the soft-breaking or <inline-formula><tex-math notation="LaTeX" id="ImEquation396"><![CDATA[${\rm SU}(3)_L$]]></tex-math></inline-formula> scale. Keeping only the leading term in (<xref rid="PTV155M47" ref-type="disp-formula">47</xref>) as the largest contribution, the masses of the three DCHs are
<disp-formula id="PTV155M48"><label>(48)</label><tex-math notation="LaTeX" id="DmEquation55"><![CDATA[\begin{align} m^2_{H^{\pm \pm}_1} &\simeq m^2_V+m^2_{A_2}, \nonumber \\ m^2_{H^{\pm \pm}_{2,3}} &\simeq \frac{1}{2}\left(m^2_{A_1} \pm \sqrt{4 c_{2\beta}^2 m^4_V - 4 c_{2\beta} c_{2\gamma}m^2_V m^2_{A_1} +m^4_{A_1}} \right). \end{align}]]></tex-math>
</disp-formula>
Comparing the <inline-formula><tex-math notation="LaTeX" id="ImEquation397"><![CDATA[$\left (\mathcal {M}^2_{H^{\prime \pm \pm }}\right )_{33}$]]></tex-math></inline-formula> entry of (<xref rid="PTV155M40" ref-type="disp-formula">40</xref>) with <inline-formula><tex-math notation="LaTeX" id="ImEquation398"><![CDATA[$m^2_{H^{\pm \pm }_1}$]]></tex-math></inline-formula> in the first line of (<xref rid="PTV155M48" ref-type="disp-formula">48</xref>), it can be realized that <inline-formula><tex-math notation="LaTeX" id="ImEquation399"><![CDATA[$\left (\mathcal {M}^2_{H^{\prime \pm \pm }}\right )_{33}-m^2_{H^{\pm \pm }_1}= \mathcal {O}\big (m^2_W\big ) \ll m^2_{H^{\pm \pm }_1}$]]></tex-math></inline-formula>. As a result, the main contribution to the mass eigenstate of <inline-formula><tex-math notation="LaTeX" id="ImEquation400"><![CDATA[$m^2_{H^{\pm \pm }_1}$]]></tex-math></inline-formula> is <inline-formula><tex-math notation="LaTeX" id="ImEquation401"><![CDATA[$H^{\prime \pm \pm }_1=-c_{\beta }\chi ^{\pm \pm }+s_{\beta }\chi ^{\prime \pm \pm }$]]></tex-math></inline-formula>, i.e., <inline-formula><tex-math notation="LaTeX" id="ImEquation402"><![CDATA[$\Lambda _{1i},\Lambda _{i1}\simeq \delta _{1i}$]]></tex-math></inline-formula> with <inline-formula><tex-math notation="LaTeX" id="ImEquation403"><![CDATA[$i=1,2,3$]]></tex-math></inline-formula>. This is very useful in finding the coupling formulas between these DCHs with neutral gauge bosons.</p>
<p>The above approximative formulas of DCH masses can precisely predict the constraints of these masses. From Eq. (<xref rid="PTV155M44" ref-type="disp-formula">44</xref>), applying Vieta&#x0027;s formulas to the first line of (<xref rid="PTV155M45" ref-type="disp-formula">45</xref>), we get a relation
<disp-formula id="PTV155UM8"><tex-math notation="LaTeX" id="DmEquation56"><![CDATA[\[ m^2_{H^{\pm\pm}_1}+m^2_{H^{\pm\pm}_2}+m^2_{H^{\pm\pm}_3}= m^2_V+m^2_{A_2}+m^2_{A_1}+m^2_{W}. \]]]></tex-math>
</disp-formula>
Combining this with <inline-formula><tex-math notation="LaTeX" id="ImEquation404"><![CDATA[$m^2_{H^{\pm \pm }_1}=m^2_V+m^2_{A_2}+\mathcal {O}\big (m^2_W\big )$]]></tex-math></inline-formula>, we have a sum of two DCHs, <inline-formula><tex-math notation="LaTeX" id="ImEquation405"><![CDATA[$m^2_{H^{\pm \pm }_2}+m^2_{H^{\pm \pm }_3}=m^2_{A_{1}}+\mathcal {O}\big (m^2_W\big )$]]></tex-math></inline-formula>, which is still of the order of the <inline-formula><tex-math notation="LaTeX" id="ImEquation406"><![CDATA[${\rm SU(3)}_L$]]></tex-math></inline-formula> scale. So there must be at most one light DCH in the model. If the model contains this light Higgs, i.e., <inline-formula><tex-math notation="LaTeX" id="ImEquation407"><![CDATA[$m^2_{H^{\pm \pm }_3}\sim \mathcal {O}\big (m^2_W\big )$]]></tex-math></inline-formula>, we can prove that <inline-formula><tex-math notation="LaTeX" id="ImEquation408"><![CDATA[$m^2_{H^{\pm \pm }_2}\sim m^2_V$]]></tex-math></inline-formula>. This is the consequence deduced from the last equation of (<xref rid="PTV155M45" ref-type="disp-formula">45</xref>) and (<xref rid="PTV155M46" ref-type="disp-formula">46</xref>): the condition of the existence of this light Higgs is
<disp-formula id="PTV155M49"><label>(49)</label><tex-math notation="LaTeX" id="DmEquation57"><![CDATA[\begin{equation} 0<k_{H^{\pm\pm}}\equiv -c_{2\beta}\left[c_{2\beta} m^2_V- c_{2\gamma} \Big(m^2_W +m^2_{A_1}\Big)\right] \sim \mathcal{O}\big(m^2_W\big).\end{equation}]]></tex-math>
</disp-formula>
This leads to <inline-formula><tex-math notation="LaTeX" id="ImEquation409"><![CDATA[$m^2_{H^{\pm \pm }_2}+m^2_{H^{\pm \pm }_3}\sim \mathcal {O}\big (m^2_V\big )$]]></tex-math></inline-formula>. The mass of the lightest DCH <inline-formula><tex-math notation="LaTeX" id="ImEquation410"><![CDATA[$m^2_{H^{\pm \pm }_3}$]]></tex-math></inline-formula> depends directly on the scale of <inline-formula><tex-math notation="LaTeX" id="ImEquation411"><![CDATA[$k_{H^{\pm \pm }}$]]></tex-math></inline-formula>. It is easy to realize that two mass eigenstates <inline-formula><tex-math notation="LaTeX" id="ImEquation412"><![CDATA[$H^{\pm \pm }_{2,3}$]]></tex-math></inline-formula> get their main contributions from <inline-formula><tex-math notation="LaTeX" id="ImEquation413"><![CDATA[$\rho ^{\pm \pm }$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation414"><![CDATA[$\rho ^{\prime \pm \pm }$]]></tex-math></inline-formula>. This is consistent with the fact that the main contribution to the mass of the heavy Higgs <inline-formula><tex-math notation="LaTeX" id="ImEquation415"><![CDATA[$H^{\pm \pm }_2$]]></tex-math></inline-formula> is from the <inline-formula><tex-math notation="LaTeX" id="ImEquation416"><![CDATA[$b_{\rho }\rho \rho '$]]></tex-math></inline-formula> term. The numerical values of these masses are illustrated in Fig. <xref ref-type="fig" rid="PTV155F2">2</xref>.
<fig id="PTV155F2"><label>Fig. 2.</label>
<caption><p>Contour plots for the masses of DCHs as functions of <inline-formula><tex-math notation="LaTeX" id="ImEquation417"><![CDATA[$m_{A_1}$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation418"><![CDATA[$m_V$]]></tex-math></inline-formula>. The left (right) panel corresponds to <inline-formula><tex-math notation="LaTeX" id="ImEquation419"><![CDATA[$m_{A_2}=1$]]></tex-math></inline-formula> (2.5)&#x2009;TeV. The heaviest DCH is represented by dotted curves, the second heaviest by dashed curves, and the lightest by solid curves.</p></caption>
<graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ptv15502"/>
</fig></p>
<p>The condition (<xref rid="PTV155M49" ref-type="disp-formula">49</xref>) give a lower bound of <inline-formula><tex-math notation="LaTeX" id="ImEquation420"><![CDATA[$m_{A_1}>1.8$]]></tex-math></inline-formula>&#x2009;TeV. With <inline-formula><tex-math notation="LaTeX" id="ImEquation421"><![CDATA[$m_{A_2}<3$]]></tex-math></inline-formula>&#x2009;TeV, the heaviest DCH is always <inline-formula><tex-math notation="LaTeX" id="ImEquation422"><![CDATA[$H^{\pm \pm }_1$]]></tex-math></inline-formula>, except in the case of the very light <inline-formula><tex-math notation="LaTeX" id="ImEquation423"><![CDATA[$m_V\simeq 2$]]></tex-math></inline-formula>&#x2009;TeV. This explains why <inline-formula><tex-math notation="LaTeX" id="ImEquation424"><![CDATA[$m_{H^{\pm \pm }_1}$]]></tex-math></inline-formula> does not depend on <inline-formula><tex-math notation="LaTeX" id="ImEquation425"><![CDATA[$m_{A_1}$]]></tex-math></inline-formula>, while it is sensitive to <inline-formula><tex-math notation="LaTeX" id="ImEquation426"><![CDATA[$m_V$]]></tex-math></inline-formula>. The second heavy DCH is also independent of small values of <inline-formula><tex-math notation="LaTeX" id="ImEquation427"><![CDATA[$m_{A_1}$]]></tex-math></inline-formula>, which can be explained as follows. The condition of avoiding a tachyon DCH (<xref rid="PTV155M46" ref-type="disp-formula">46</xref>) implies that <inline-formula><tex-math notation="LaTeX" id="ImEquation428"><![CDATA[$0<c_{2\beta }/c_{2\gamma } m_V^2-m^2_W < m_{A_1}^2$]]></tex-math></inline-formula>. Therefore, a small <inline-formula><tex-math notation="LaTeX" id="ImEquation429"><![CDATA[$m_{A_1}$]]></tex-math></inline-formula> will give <inline-formula><tex-math notation="LaTeX" id="ImEquation430"><![CDATA[$c_{2\beta } m_V^2- c_{2\gamma }m_{A_1}^2 \sim \mathcal {O}(m_W^2)$]]></tex-math></inline-formula>, which is the condition for the appearance of the very light DCH. This gives
<disp-formula id="PTV155UM9"><tex-math notation="LaTeX" id="DmEquation58"><![CDATA[\[ \frac{4c_{2\beta} m_V^2\Big(c_{2\beta} m^2_V - c_{2\gamma}m^2_{A_1}\Big)}{m^4_{A_1}}\sim \frac{m_V^2}{m^2_{A_1}}\times \frac{\mathcal{O}(m_W^2)}{m^2_{A_1}}\ll 1, \]]]></tex-math>
</disp-formula>
which we can use for estimating an approximation of <inline-formula><tex-math notation="LaTeX" id="ImEquation431"><![CDATA[$m^2_{H^{\pm \pm }_2}$]]></tex-math></inline-formula>:
<disp-formula id="PTV155UM10"><tex-math notation="LaTeX" id="DmEquation59"><![CDATA[\[ m^2_{H^{\pm\pm}_2}\simeq \frac{\left(c_{2\beta}m_V^2-c_{2\gamma}m^2_{A_1}\right)^2}{m^2_{A_1}}+ s^2_{2\gamma}m^2_{A_1}+c_{2\beta}c_{2\gamma}m_V^2. \]]]></tex-math>
</disp-formula>
Here, a very small <inline-formula><tex-math notation="LaTeX" id="ImEquation432"><![CDATA[$s^2_{2\gamma }$]]></tex-math></inline-formula> is assumed in this work. This means that <inline-formula><tex-math notation="LaTeX" id="ImEquation433"><![CDATA[$m^2_{H^{\pm \pm }_2}$]]></tex-math></inline-formula> is sensitive to changes in <inline-formula><tex-math notation="LaTeX" id="ImEquation434"><![CDATA[$c_{2\beta }c_{2\gamma }m_V^2$]]></tex-math></inline-formula> but not to small changes in <inline-formula><tex-math notation="LaTeX" id="ImEquation435"><![CDATA[$m_{A_1}$]]></tex-math></inline-formula>.</p>
<p>Now we pay attention to the first interesting property relating to the SUSYRM331: it may contain the lightest DCH that does not depend on the <inline-formula><tex-math notation="LaTeX" id="ImEquation436"><![CDATA[${\rm SU}(3)_L$]]></tex-math></inline-formula> scale but on the specific correlation between <inline-formula><tex-math notation="LaTeX" id="ImEquation437"><![CDATA[$m_{A_1}$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation438"><![CDATA[$m_V$]]></tex-math></inline-formula>, as indicated in (<xref rid="PTV155M49" ref-type="disp-formula">49</xref>) and illustrated in Fig. <xref ref-type="fig" rid="PTV155F2">2</xref>. It can be seen that there always exists a region of the parameter space containing the mass of this DCH of the order of <inline-formula><tex-math notation="LaTeX" id="ImEquation439"><![CDATA[$\mathcal {O}(100)$]]></tex-math></inline-formula>&#x2009;GeV. So the ILC can create this Higgs at a collision energy of 0.5&#x2013;1.0&#x2009;TeV, while the two other DCHs are very heavy because of the large lower bound of <inline-formula><tex-math notation="LaTeX" id="ImEquation440"><![CDATA[$m_V\geq 2$]]></tex-math></inline-formula>&#x2009;TeV as well as <inline-formula><tex-math notation="LaTeX" id="ImEquation441"><![CDATA[$m_{A_1}>1.8$]]></tex-math></inline-formula>&#x2009;TeV, obtained from condition (<xref rid="PTV155M49" ref-type="disp-formula">49</xref>). The lower bound of the first DCH mass is <inline-formula><tex-math notation="LaTeX" id="ImEquation442"><![CDATA[$m_{H^{\pm \pm }_1}\simeq \sqrt {m_V^2+m^2_{A_2}}=m_{H^{\pm }_2}> 2$]]></tex-math></inline-formula>&#x2009;TeV. The additional condition of <inline-formula><tex-math notation="LaTeX" id="ImEquation443"><![CDATA[$m_{A_1}>1.8$]]></tex-math></inline-formula>&#x2009;TeV will result in a larger lower bound of <inline-formula><tex-math notation="LaTeX" id="ImEquation444"><![CDATA[$m_{H^{\pm \pm }_1}>3$]]></tex-math></inline-formula>&#x2009;TeV and be independent of <inline-formula><tex-math notation="LaTeX" id="ImEquation445"><![CDATA[$m_{A_2}$]]></tex-math></inline-formula>. The lower bound of <inline-formula><tex-math notation="LaTeX" id="ImEquation446"><![CDATA[$m^2_{H^{\pm \pm }_2}$]]></tex-math></inline-formula> directly depends on condition (<xref rid="PTV155M49" ref-type="disp-formula">49</xref>), where <inline-formula><tex-math notation="LaTeX" id="ImEquation447"><![CDATA[$m^2_{A_1}>\frac {c_{2\beta }m^2_V}{c_{2\gamma }}-m^2_W$]]></tex-math></inline-formula>, leading to <inline-formula><tex-math notation="LaTeX" id="ImEquation448"><![CDATA[$m_{H^{\pm \pm }_2}>1.9$]]></tex-math></inline-formula>&#x2009;TeV, when <inline-formula><tex-math notation="LaTeX" id="ImEquation449"><![CDATA[$c_{2\beta },c_{2\gamma }\simeq -1$]]></tex-math></inline-formula> are assumed in this work. Hence, the SUSYRM331 model predicts that the DCHs will not appear in <inline-formula><tex-math notation="LaTeX" id="ImEquation450"><![CDATA[$e^+e^-$]]></tex-math></inline-formula> colliders with colliding energies below 4&#x2009;TeV, with the exception of the lightest DCH.</p>
<p>There is a second interesting property of the lightest DCH: it is lighter than all particles including new gauge bosons and singly charged Higgses, as illustrated in Fig. <xref ref-type="fig" rid="PTV155F3">3</xref>. It is easy to see this when we compare all the masses computed above. The exotic quarks as well as their superpartners can be reasonably supposed to be heavier than the lightest DCH; thus, we do not consider them here. Then we can indicate that the lightest DCH decays into only a pair of charged leptons. Recall that all DCHs have a lepton number of two. Therefore, the total lepton number of all the final states of their decays must be the same. In particular, the final states of each decay should contain one bilepton or a pair of charged leptons. From Tables <xref ref-type="table" rid="PTV155TBC4">C.4</xref> and <xref ref-type="table" rid="PTV155TBC5">C.5</xref>, which list all three- and four-vertex couplings related to DCHs, we can see that, except for the coupling with two leptons, the lightest DCH always couples with at least one heavier particle: another DCH, a singly charged Higgs, a new gauge boson, or a CP-odd neutral Higgs. So, if it exists, the most promising signal of the lightest DCH is the decay into only a pair of leptons. This strongly suggests the possibility of detection of the lightest DCH in <inline-formula><tex-math notation="LaTeX" id="ImEquation451"><![CDATA[$e^+e^-$]]></tex-math></inline-formula> colliders such as the ILC or CLIC, even at the low energy of 0.5&#x2013;1&#x2009;TeV.
<fig id="PTV155F3"><label>Fig. 3.</label>
<caption><p>Plots of mass spectra as functions of <inline-formula><tex-math notation="LaTeX" id="ImEquation452"><![CDATA[$m_{A_1}$]]></tex-math></inline-formula> with different fixed <inline-formula><tex-math notation="LaTeX" id="ImEquation453"><![CDATA[$m_V$]]></tex-math></inline-formula>. The solid, dotted, dashed, and thick-dashed curves represent DCHs, singly charged, neutral Higgses, and <inline-formula><tex-math notation="LaTeX" id="ImEquation454"><![CDATA[$V$]]></tex-math></inline-formula> gauge bosons, respectively.</p></caption>
<graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ptv15503"/>
</fig>
<table-wrap id="PTV155TBC4" position="float"><label>Table C.4.</label>
<caption><p>Three-vertex coupling of doubly charged Higgses.</p></caption>
<table frame="hsides" rules="groups">
<colgroup>
<col align="left"/>
<col align="center"/>
<col align="center"/>
<col align="center"/>
</colgroup>
<thead><tr>
<th align="left">Vertex</th>
<th align="center">Factor</th>
<th align="center">Vertex</th>
<th align="center">Factor</th>
</tr>
</thead>
<tbody><tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation455"><![CDATA[$\rho ^{++}\rho ^{--} Z^{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation456"><![CDATA[$-\dfrac {ig}{2\sqrt {3}}\left [ \dfrac {(2t^2-3) s_{\zeta }}{\sqrt {2t^2+3}}+c_{\zeta }\right ]\big (p+p'\big )_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation457"><![CDATA[$\rho ^{\prime ++}\rho ^{\prime --} Z^{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation458"><![CDATA[$-\dfrac {i g}{2\sqrt {3}} \left [\dfrac {(2t^2-3)s_{\zeta }}{\sqrt {2t^2+3}}+c_{\zeta }\right ]\big (p+p'\big )_{\mu }$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation459"><![CDATA[$\chi ^{++}\chi ^{--} Z^{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation460"><![CDATA[$-\dfrac {i g}{2\sqrt {3}} \left [\dfrac {(2t^2-3)s_{\zeta }}{\sqrt {2t^2+3}}-c_{\zeta }\right ]\big (p+p'\big )_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation461"><![CDATA[$\chi ^{\prime ++}\chi ^{\prime --} Z^{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation462"><![CDATA[$-\dfrac {i g}{2\sqrt {3}} \left [\dfrac {(2t^2-3)s_{\zeta }}{\sqrt {2t^2+3}}-c_{\zeta }\right ]\big (p+p'\big )_{\mu }$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation463"><![CDATA[$\rho ^{++}U^{--\mu }H_{\rho }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation464"><![CDATA[$\dfrac {i g}{2}\big (p+p'\big )_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation465"><![CDATA[$\rho ^{++}U^{--\mu }H_{A_1}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation466"><![CDATA[$\dfrac {gc_{\gamma }}{2}\big (p+p'\big )_{\mu }$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation467"><![CDATA[$\rho ^{++}V^{-\mu }H^{-}_{1}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation468"><![CDATA[$-\dfrac {igc_{\gamma }}{\sqrt {2}}\big (p+p'\big )_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation469"><![CDATA[$\rho ^{\prime ++}U^{--\mu }H_{\rho '}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation470"><![CDATA[$-\dfrac {i g}{2}\big (p+p'\big )_{\mu }$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation471"><![CDATA[$\rho ^{\prime ++}U^{--\mu }H_{A_1}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation472"><![CDATA[$\dfrac {-gs_{\gamma }}{2}\big (p+p'\big )_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation473"><![CDATA[$\rho ^{\prime ++}V^{-\mu }H^{-}_{1}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation474"><![CDATA[$\dfrac {i gs_{\gamma }}{\sqrt {2}}\big (p+p'\big )_{\mu }$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation475"><![CDATA[$\chi ^{++}U^{--\mu }H_{\chi }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation476"><![CDATA[$-\dfrac {i g}{2}\big (p+p'\big )_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation477"><![CDATA[$\chi ^{++}U^{--\mu }H_{A_2}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation478"><![CDATA[$\dfrac {gc_{\beta }}{2}\big (p+p'\big )_{\mu }$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation479"><![CDATA[$\chi ^{++}W^{-\mu }H^{-}_{2}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation480"><![CDATA[$\dfrac {i gc_{\beta }}{\sqrt {2}}\big (p+p'\big )_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation481"><![CDATA[$\chi ^{\prime ++}U^{--\mu }H_{\chi '}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation482"><![CDATA[$-\dfrac {i g}{2}\big (p+p'\big )_{\mu }$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation483"><![CDATA[$\chi ^{\prime ++}U^{--\mu }H_{A_2}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation484"><![CDATA[$-\dfrac {gs_{\beta }}{2}\big (p+p'\big )_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation485"><![CDATA[$\chi ^{\prime ++}W^{-\mu }H^{-}_{2}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation486"><![CDATA[$-\dfrac {ig s_{\beta }}{\sqrt {2}}\big (p+p'\big )_{\mu }$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation487"><![CDATA[$\rho ^{\prime --}l^c_il^c_i$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation488"><![CDATA[$\dfrac {i g m_l}{\sqrt {2}m_W c_{\gamma }c_{\beta }}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation489"><![CDATA[$\chi ^{\prime ++}ll$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation490"><![CDATA[$\dfrac {ig m_l}{\sqrt {2}m_V c_{\gamma }c_{\beta }}$]]></tex-math></inline-formula></td>
</tr>
</tbody>
</table>
</table-wrap></p>
<p>As mentioned above, the state of the lightest DCH is contributed mainly from two Higgses <inline-formula><tex-math notation="LaTeX" id="ImEquation491"><![CDATA[$\rho $]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation492"><![CDATA[$\rho '$]]></tex-math></inline-formula>. Combining this with the coupling factors between DCHs and charged leptons shown in Table <xref ref-type="table" rid="PTV155TBC4">C.4</xref>, it is easy to prove that the partial decay of this DCH to a pair of same-sign leptons is <inline-formula><tex-math notation="LaTeX" id="ImEquation493"><![CDATA[$\Gamma \Big (H^{\pm \pm }\rightarrow l^{\pm }_il^{\pm }_i\Big ) \sim \left (m_{l_i}/m_W\right )^2$]]></tex-math></inline-formula> with <inline-formula><tex-math notation="LaTeX" id="ImEquation494"><![CDATA[$l_i=e,\, \mu , \, \tau $]]></tex-math></inline-formula>. As a result, we obtain <inline-formula><tex-math notation="LaTeX" id="ImEquation495"><![CDATA[${\rm Br}\Big (H^{\pm \pm }\rightarrow \tau ^{\pm }\tau ^{\pm }\Big )\simeq 1$]]></tex-math></inline-formula>, i.e., the number of events of four-tauon signals is equal to that of creating the lightest DCH at <inline-formula><tex-math notation="LaTeX" id="ImEquation496"><![CDATA[$e^+e^-$]]></tex-math></inline-formula> colliders.</p>
<p>Because the lightest DCH mainly decays to same-sign <inline-formula><tex-math notation="LaTeX" id="ImEquation497"><![CDATA[$\tau $]]></tex-math></inline-formula> pairs, the lower bound from experimental searches is 204 GeV [<xref ref-type="bibr" rid="PTV155C26">26</xref>]. This lightest DCH is very different from other DCHs predicted by other models where they can mainly decay to pairs of two same-sign <inline-formula><tex-math notation="LaTeX" id="ImEquation498"><![CDATA[$W$]]></tex-math></inline-formula> bosons or <inline-formula><tex-math notation="LaTeX" id="ImEquation499"><![CDATA[$W^-H^-$]]></tex-math></inline-formula> [<xref ref-type="bibr" rid="PTV155C35">35</xref>&#x2013;<xref ref-type="bibr" rid="PTV155C37">37</xref>]. On the other hand, the heavy DCHs predicted by the SUSYRM331 only couple to other bileptons in the model, including <inline-formula><tex-math notation="LaTeX" id="ImEquation500"><![CDATA[$H^{\pm }_2$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation501"><![CDATA[$V^{\pm }$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation502"><![CDATA[$U^{\pm \pm }$]]></tex-math></inline-formula> and their corresponding superpartners. The most interesting coupling is <inline-formula><tex-math notation="LaTeX" id="ImEquation503"><![CDATA[$H_1^{\pm \pm }W^{\mp }H^{\mp }_2$]]></tex-math></inline-formula>, which was discussed in Refs. [<xref ref-type="bibr" rid="PTV155C35">35</xref>&#x2013;<xref ref-type="bibr" rid="PTV155C37">37</xref>, <xref ref-type="bibr" rid="PTV155C89">89</xref>] for creating DCHs at LHC through virtual <inline-formula><tex-math notation="LaTeX" id="ImEquation504"><![CDATA[$W^{\pm }$]]></tex-math></inline-formula> bosons, while there are no couplings of <inline-formula><tex-math notation="LaTeX" id="ImEquation505"><![CDATA[$H^{\pm \pm }W^{\mp }W^{\mp }$]]></tex-math></inline-formula> because of the lepton number conservation. In addition, the masses of the two heavy DCHs are always larger than 1.5&#x2009;TeV; they do not appear in the <inline-formula><tex-math notation="LaTeX" id="ImEquation506"><![CDATA[$e^+e^-$]]></tex-math></inline-formula> colliders such as ILC and CLIC with their recent designs. These two Higgses may only appear at the LHC with high luminosity. In addition, both of them can be created through the channel <inline-formula><tex-math notation="LaTeX" id="ImEquation507"><![CDATA[$pp\rightarrow \gamma /Z/Z'\rightarrow H^{++}H^{--}$]]></tex-math></inline-formula>, but only <inline-formula><tex-math notation="LaTeX" id="ImEquation508"><![CDATA[$H^{\pm \pm }_1$]]></tex-math></inline-formula> may be created through the channel <inline-formula><tex-math notation="LaTeX" id="ImEquation509"><![CDATA[$pp\rightarrow W^{\pm }\rightarrow H^{\pm \pm }_1H^{\mp }_2$]]></tex-math></inline-formula>. Regarding the latter channel, discussions in Refs. [<xref ref-type="bibr" rid="PTV155C37">37</xref>, <xref ref-type="bibr" rid="PTV155C89">89</xref>] indicated that it is very hard to find signals of these very heavy DCHs, even at the very high luminosity of <inline-formula><tex-math notation="LaTeX" id="ImEquation510"><![CDATA[$3000\,{\rm fb}^{-1}$]]></tex-math></inline-formula> that LHC can reach. While the former happens for all three DCHs, the two heavy DCHs are also very hard to observe [<xref ref-type="bibr" rid="PTV155C90">90</xref>].</p>
<p>For the above reason, the SUSYRM331 predicts that only the lightest DCH may be discovered at the LHC and <inline-formula><tex-math notation="LaTeX" id="ImEquation511"><![CDATA[$e^+e^-$]]></tex-math></inline-formula> colliders and the signal can be observed through the main channel of <inline-formula><tex-math notation="LaTeX" id="ImEquation512"><![CDATA[$pp/e^+e^-\rightarrow \gamma /Z/Z'\rightarrow H^{++}_3H^{--}_3 \rightarrow $]]></tex-math></inline-formula> four tauons. With the LHC, one hopes that it will be observed up to mass of 600&#x2009;GeV with a high luminosity of <inline-formula><tex-math notation="LaTeX" id="ImEquation513"><![CDATA[$3000\,{\rm fb}^{-1}$]]></tex-math></inline-formula>. Because the cross section created is proportional to <inline-formula><tex-math notation="LaTeX" id="ImEquation514"><![CDATA[$1/s^2$]]></tex-math></inline-formula>, with <inline-formula><tex-math notation="LaTeX" id="ImEquation515"><![CDATA[$s$]]></tex-math></inline-formula> being the colliding energy, the signal of DCH at ILC and CLIC seems better than that at LHC. In addition, with the ILC or CLIC, a larger DCH mass range can be observed, so we will mainly pay attention to the lightest DCH at <inline-formula><tex-math notation="LaTeX" id="ImEquation516"><![CDATA[$e^+e^-$]]></tex-math></inline-formula> colliders.</p>
<p>Now we will estimate the allowed kinetic condition <inline-formula><tex-math notation="LaTeX" id="ImEquation517"><![CDATA[$2 m_{H^{\pm \pm }}\leq E_{\rm cm}$]]></tex-math></inline-formula> for the creation of the lightest DCH at the <inline-formula><tex-math notation="LaTeX" id="ImEquation518"><![CDATA[$e^+e^-$]]></tex-math></inline-formula> colliders with a maximal center-of-mass (CM) energy of 3&#x2009;TeV. Even in the case in which both <inline-formula><tex-math notation="LaTeX" id="ImEquation519"><![CDATA[$m_V$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation520"><![CDATA[$m_{A_1}$]]></tex-math></inline-formula> are large, there always exists a region in which the mass of the lightest DCH is of the order of <inline-formula><tex-math notation="LaTeX" id="ImEquation521"><![CDATA[$\mathcal {O}(100)$]]></tex-math></inline-formula>&#x2009;GeV. Furthermore, this light value is almost independent of <inline-formula><tex-math notation="LaTeX" id="ImEquation522"><![CDATA[$m_{A_2}$]]></tex-math></inline-formula>. Although mass values below 204&#x2009;GeV for this Higgs were almost excluded recently from its decay into only a pair of tauons [<xref ref-type="bibr" rid="PTV155C26">26</xref>, <xref ref-type="bibr" rid="PTV155C27">27</xref>], higher values can be searched for by ILC or CLIC with a CM energy of about 1&#x2009;TeV.</p>
<p>The appearance of the light DCH may give large loop corrections to the decays of well known particles. The most important is the decay channel of the SM-like Higgs <inline-formula><tex-math notation="LaTeX" id="ImEquation523"><![CDATA[$H^0_1\rightarrow \gamma \gamma $]]></tex-math></inline-formula>, which gets contributions from only pure loop corrections. The signal strength of this decay is defined as the ratio of the observed cross section and the SM prediction, <inline-formula><tex-math notation="LaTeX" id="ImEquation524"><![CDATA[$\mu _{\gamma \gamma }= \sigma ^{{\rm obs}}_{H\rightarrow \gamma \gamma }/\sigma ^{{\rm SM}}_{H\rightarrow \gamma \gamma }$]]></tex-math></inline-formula>, and was found to be slightly in excess of 1 [<xref ref-type="bibr" rid="PTV155C3">3</xref>, <xref ref-type="bibr" rid="PTV155C4">4</xref>, <xref ref-type="bibr" rid="PTV155C91">91</xref>, <xref ref-type="bibr" rid="PTV155C92">92</xref>]. The enhancement is explained by the contributions of new particles to the partial decay width of <inline-formula><tex-math notation="LaTeX" id="ImEquation525"><![CDATA[$H^0_1\rightarrow \gamma \gamma $]]></tex-math></inline-formula> [<xref ref-type="bibr" rid="PTV155C82">82</xref>]. The analytic formula of this decay width is the sum of its three particular parts: SM, <inline-formula><tex-math notation="LaTeX" id="ImEquation526"><![CDATA[${\rm SU}(3)_L$]]></tex-math></inline-formula> [<xref ref-type="bibr" rid="PTV155C93">93</xref>], and SUSY contributions. The SM and SUSYRM331 contributions can be deduced based on Refs. [<xref ref-type="bibr" rid="PTV155C82">82</xref>, <xref ref-type="bibr" rid="PTV155C94">94</xref>].</p>
<p>The SUSYRM331, with both <inline-formula><tex-math notation="LaTeX" id="ImEquation527"><![CDATA[${\rm SU}(3)_L$]]></tex-math></inline-formula> and SUSY breaking scales being larger than 7&#x2009;TeV, results in a consequence that most of the <inline-formula><tex-math notation="LaTeX" id="ImEquation528"><![CDATA[${\rm SU}(3)_L$]]></tex-math></inline-formula> and SUSY particles give suppressed contributions to this decay, except for the lightest DCH. Hence, <inline-formula><tex-math notation="LaTeX" id="ImEquation529"><![CDATA[$H^0_1\rightarrow \gamma \gamma $]]></tex-math></inline-formula> is an important channel to set a lower bound to its mass. We will follow the latest update of <inline-formula><tex-math notation="LaTeX" id="ImEquation530"><![CDATA[$\mu _{\gamma \gamma }$]]></tex-math></inline-formula> in Ref. [<xref ref-type="bibr" rid="PTV155C4">4</xref>], where <inline-formula><tex-math notation="LaTeX" id="ImEquation531"><![CDATA[$\mu _{\gamma \gamma }=1.12\pm 0.24$]]></tex-math></inline-formula> without any inconsistencies with the ATLAS results. In addition, to simplify the calculation, we consider that the largest new physics effect on the <inline-formula><tex-math notation="LaTeX" id="ImEquation532"><![CDATA[$H^0_1$]]></tex-math></inline-formula> decay is from only the lightest DCH <inline-formula><tex-math notation="LaTeX" id="ImEquation533"><![CDATA[$H^{\pm \pm }_3$]]></tex-math></inline-formula> to the partial decay <inline-formula><tex-math notation="LaTeX" id="ImEquation534"><![CDATA[$H^0_1\rightarrow \gamma \gamma $]]></tex-math></inline-formula>. As a result, we have a very simple formula, which must satisfy the experimental constraint: <inline-formula><tex-math notation="LaTeX" id="ImEquation535"><![CDATA[$0.88=1.12-0.24\leq \mu ^{{\rm SUSYRM331}}_{\gamma \gamma }\leq 1.12+0.24=1.36$]]></tex-math></inline-formula>. The partial decay of the <inline-formula><tex-math notation="LaTeX" id="ImEquation536"><![CDATA[$H^0_1\rightarrow \gamma \gamma $]]></tex-math></inline-formula> <bold>is</bold> written as
<disp-formula id="PTV155M50"><label>(50)</label><tex-math notation="LaTeX" id="DmEquation60"><![CDATA[\begin{equation} \Gamma^{{\rm SUSYRM331}}_{H^0_1\rightarrow \gamma\gamma} \simeq \frac{G_{\mu}\alpha^2 m^3_{H^0_1}}{128\sqrt{2}\pi^3}\left| A^{{\rm SM}}+ \Delta A\right|^2,\end{equation}]]></tex-math>
</disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation537"><![CDATA[$A^{{\rm SM}}$]]></tex-math></inline-formula> is the contribution from the SM particles, and <inline-formula><tex-math notation="LaTeX" id="ImEquation538"><![CDATA[$\Delta A$]]></tex-math></inline-formula> is the new contribution from the SUSYRM331 particles. The well known SM formula can be found in many textbooks or publications, e.g., in Ref. [<xref ref-type="bibr" rid="PTV155C94">94</xref>]. To find a simple analytic formula, our work considers only the case of <inline-formula><tex-math notation="LaTeX" id="ImEquation539"><![CDATA[$c_{2\gamma },c_{2\beta }\rightarrow -1$]]></tex-math></inline-formula>, where the masses of the DCHs are nearly equal to the diagonal entries of the squared mass matrix (<xref rid="PTV155M40" ref-type="disp-formula">40</xref>), being consistent with (<xref rid="PTV155M48" ref-type="disp-formula">48</xref>). The lightest DCH mass now satisfies <inline-formula><tex-math notation="LaTeX" id="ImEquation540"><![CDATA[$m^2_{H^{\pm \pm }_3} = \mathcal {O}(100)$]]></tex-math></inline-formula>&#x2009;GeV when (<xref rid="PTV155M49" ref-type="disp-formula">49</xref>) is satisfied. In addition, the main contribution to the mixing matrix of the DCHs is <inline-formula><tex-math notation="LaTeX" id="ImEquation541"><![CDATA[$C_1$]]></tex-math></inline-formula>, shown in (<xref rid="PTV155M39" ref-type="disp-formula">39</xref>). Combining this with the discussion on the neutral Higgs sector, we find that the <inline-formula><tex-math notation="LaTeX" id="ImEquation542"><![CDATA[$H^0_1H^{++}_3H^{--}_3$]]></tex-math></inline-formula> coupling is <inline-formula><tex-math notation="LaTeX" id="ImEquation543"><![CDATA[$g_{H^0HH}\simeq \frac {1}{3}g\big (t^2+2\big )c_{2\gamma }m_W\simeq -\frac {1}{3}g\big (t^2+2\big )m_W =- \frac {2c^2_W }{3(1-4s^2_W)}m_W$]]></tex-math></inline-formula>. Following this, the formula of <inline-formula><tex-math notation="LaTeX" id="ImEquation544"><![CDATA[$\Delta A$]]></tex-math></inline-formula> can be written as [<xref ref-type="bibr" rid="PTV155C82">82</xref>]
<disp-formula id="PTV155M51"><label>(51)</label><tex-math notation="LaTeX" id="DmEquation61"><![CDATA[\begin{equation} \Delta A = -\frac{8 c^2_W m^2_W}{3\Big(1-4s^2_W\Big)m^2_{H^{\pm\pm}_3}}A_0(t_H),\end{equation}]]></tex-math>
</disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation545"><![CDATA[$t_H=\frac {m^2_{H^0_1}}{4m^2_{H^{\pm \pm }_3}}$]]></tex-math></inline-formula> and
<disp-formula id="PTV155UM11"><tex-math notation="LaTeX" id="DmEquation62"><![CDATA[\begin{align*} A_0(t)&= -[t-f(t)]t^{-2},\nonumber \\ f(t)&= \begin{cases} \arcsin^2\sqrt{t} & {\rm for} \, t\leq1 \\ -\dfrac{1}{4}\left[\ln \left( \frac{1+\sqrt{1-t^{-1}}}{1-\sqrt{1-t^{-1}}}\right)- i\pi\right]^2 & {\rm for} \, t>1. \\ \end{cases} \end{align*}]]></tex-math>
</disp-formula>
The signal strength of the decay <inline-formula><tex-math notation="LaTeX" id="ImEquation546"><![CDATA[$H^0_1\rightarrow \gamma \gamma $]]></tex-math></inline-formula> predicted by the SUSYRM331 is shown in Fig. <xref ref-type="fig" rid="PTV155F4">4</xref>, where <inline-formula><tex-math notation="LaTeX" id="ImEquation547"><![CDATA[$m_{H^{\pm \pm }_3}\geq 200$]]></tex-math></inline-formula>&#x2009;GeV is allowed, being equal to the lower bound of 200&#x2009;GeV from the current experiments.
<fig id="PTV155F4"><label>Fig. 4.</label>
<caption><p>Signal strength of the decay <inline-formula><tex-math notation="LaTeX" id="ImEquation548"><![CDATA[$H^0_1\rightarrow \gamma \gamma $]]></tex-math></inline-formula> as a function of the lightest DCH mass.</p></caption>
<graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ptv15504"/>
</fig></p>
<p>Finally, in order to calculate the cross sections of the DCHs in the <inline-formula><tex-math notation="LaTeX" id="ImEquation549"><![CDATA[$e^+e^-$]]></tex-math></inline-formula> colliders, the next subsection will calculate the coupling of <inline-formula><tex-math notation="LaTeX" id="ImEquation550"><![CDATA[$H^{++}H^{--}V^0$]]></tex-math></inline-formula>.</p>
</sec>
<sec id="s3b"><label>3.2.</label><title>Couplings between DCHs with neutral scalars and gauge bosons</title>
<p>It is noted that the process <inline-formula><tex-math notation="LaTeX" id="ImEquation551"><![CDATA[$e^{+}e^{-}\rightarrow H^{++}H^{--}$]]></tex-math></inline-formula> through virtual neutral Higgses is involved with the coupling <inline-formula><tex-math notation="LaTeX" id="ImEquation552"><![CDATA[$e^{+}e^{-}H^0$]]></tex-math></inline-formula>. In the SUSY version [<xref ref-type="bibr" rid="PTV155C12">12</xref>], this kind of coupling is <inline-formula><tex-math notation="LaTeX" id="ImEquation553"><![CDATA[$2 g m_e/(m_Wc_{\gamma })$]]></tex-math></inline-formula>, while the SUSY version [<xref ref-type="bibr" rid="PTV155C20">20</xref>] does not have this kind of coupling at the tree level. In this work, we will use the case in Ref. [<xref ref-type="bibr" rid="PTV155C12">12</xref>]. Corresponding with this, we consider the coupling <inline-formula><tex-math notation="LaTeX" id="ImEquation554"><![CDATA[$H^{++}H^{--}\rho ^{\prime 0}$]]></tex-math></inline-formula>. Couplings <inline-formula><tex-math notation="LaTeX" id="ImEquation555"><![CDATA[$H^{++}H^{--}H^0$]]></tex-math></inline-formula> come from the <inline-formula><tex-math notation="LaTeX" id="ImEquation556"><![CDATA[$D$]]></tex-math></inline-formula>-term of the scalar potential (<xref rid="PTV155M20" ref-type="disp-formula">20</xref>), namely,
<disp-formula id="PTV155M52"><label>(52)</label><tex-math notation="LaTeX" id="DmEquation63"><![CDATA[\begin{align} \mathcal{L}_{H^{++}H^{--}H^0}&= \frac{gm_W}{6} \rho^{\prime0} \left(\begin{matrix} \rho^{--}, & \rho^{\prime--}, &\chi^{--}, & \chi^{\prime--} \\ \end{matrix} \right)\nonumber \\ & \quad \times \left(\begin{matrix} 2s_{\gamma}\big(t^2-1\big) & -3s_{\gamma} & 0 & 0 \\ -3c_{\gamma}& 2 c_{\gamma}\big(t^2+2\big)& 0 & 0 \\ 0 & 2 c_{\gamma}\big(t^2-2\big) & 0 \\ 0 & 0 & 0 & -2 c_{\gamma}\big(t^2-2\big) \end{matrix} \right) \left(\begin{matrix} \rho^{++}\\ \rho^{\prime++} \\ \chi^{++}\\ \chi^{\prime++} \end{matrix} \right). \end{align}]]></tex-math>
</disp-formula>
Because the contributions from neutral Higgs mediations only relate to <inline-formula><tex-math notation="LaTeX" id="ImEquation557"><![CDATA[$\rho ^{\prime 0}$]]></tex-math></inline-formula>, the contribution to the <inline-formula><tex-math notation="LaTeX" id="ImEquation558"><![CDATA[$e^{+}e^{-}\rightarrow H^{++}H^{--}$]]></tex-math></inline-formula> amplitude is proportional to
<disp-formula id="PTV155UM12"><tex-math notation="LaTeX" id="DmEquation64"><![CDATA[\[ \frac{gm_e}{m_Wc_{\gamma}}\times m_W c_{\gamma}=\frac{m_e e^2}{s^2_{\theta_W}}. \]]]></tex-math>
</disp-formula>
This contribution is smaller than that from neutral gauge boson mediation by a factor of <inline-formula><tex-math notation="LaTeX" id="ImEquation559"><![CDATA[$m_e/\sqrt {s}$]]></tex-math></inline-formula>, so we can neglect it.</p>
<p>The Higgs&#x2013;Higgs&#x2013;gauge boson vertices come from the covariant kinetic terms of the Higgses:
<disp-formula id="PTV155UM13"><tex-math notation="LaTeX" id="DmEquation65"><![CDATA[\begin{align*} \mathcal{L}^{{\rm kinetic}}_{{\rm H}}&= \sum_{H} \left(\mathcal{D}_{\mu}H\right)^{\dagger}\mathcal{D}^{\mu}H, \nonumber \\ & \rightarrow \frac{ig}{2}\left(-\frac{2}{\sqrt{3}}V^{8\mu}+\frac{\sqrt{2}t}{\sqrt{3}}B^{\mu} \right) \left(\rho^{--}\partial_{\mu}\rho^{++}+\rho^{\prime--}\partial_{\mu}\rho^{\prime++}\right)\nonumber \\ & \quad - \frac{ig}{2}\left(-V^{3\mu}+\frac{1}{\sqrt{3}}V^{8\mu}-\frac{\sqrt{2}t}{\sqrt{3}}B^{\mu} \right) \left(\chi^{--}\partial_{\mu}\chi^{++}+\chi^{\prime--}\partial_{\mu}\chi^{\prime++}\right)+{\rm H.c}. \end{align*}]]></tex-math>
</disp-formula>
The interactions among neutral gauge bosons and DCHs can be written as
<disp-formula id="PTV155M53"><label>(53)</label><tex-math notation="LaTeX" id="DmEquation66"><![CDATA[\begin{align} \mathcal{L}_{HHV^0}&= i 2e A^{\mu}\left(\rho^{--}\partial_{\mu}\rho^{++}+\rho^{\prime--}\partial_{\mu}\rho^{\prime++}+ \chi^{--}\partial_{\mu}\chi^{++}+\chi^{\prime--}\partial_{\mu}\chi^{\prime++}\right)\nonumber \\ & \quad + \frac{ig}{2\sqrt{3}}\left[-\left(c_{\zeta}+\frac{(2t^2-3)s_{\zeta}}{\sqrt{2t^2+3}}\right)Z^{\mu} + \left(s_{\zeta}-\frac{(2t^2-3)c_{\zeta}}{\sqrt{2t^2+3}}\right)Z'^{\mu}\right] \nonumber \\ & \quad \times \left(\rho^{--}\partial_{\mu}\rho^{++}+\rho^{\prime--}\partial_{\mu}\rho^{\prime++}\right)\nonumber \\ & \quad + \frac{ig}{2\sqrt{3}}\left[\left(c_{\zeta}-\frac{(2t^2-3)s_{\zeta}}{\sqrt{2t^2+3}}\right)Z^{\mu} -\left(s_{\zeta}+\frac{(2t^2-3)c_{\zeta}}{\sqrt{2t^2+3}}\right)Z^{\prime\mu}\right] \nonumber \\ & \quad \times \left(\chi^{--}\partial_{\mu}\chi^{++}+\chi^{\prime--}\partial_{\mu}\chi^{\prime++}\right)+{\rm H.c.}, \end{align}]]></tex-math>
</disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation560"><![CDATA[$\mathcal {D}_{\mu }=\partial _{\mu }-i g V^a_{\mu }T^a -ig' X T^9B_{\mu }$]]></tex-math></inline-formula>; <inline-formula><tex-math notation="LaTeX" id="ImEquation561"><![CDATA[$T^a=\frac {1}{2} \lambda ^a$]]></tex-math></inline-formula> or <inline-formula><tex-math notation="LaTeX" id="ImEquation562"><![CDATA[$-\frac {1}{2} \lambda ^{a*}$]]></tex-math></inline-formula>, corresponding to triplet or antitriplet representations of Higgses; and <inline-formula><tex-math notation="LaTeX" id="ImEquation563"><![CDATA[$T^9=\frac {1}{\sqrt {6}} {\rm diag}(1,1,1)$]]></tex-math></inline-formula>. In order to find the couplings of <inline-formula><tex-math notation="LaTeX" id="ImEquation564"><![CDATA[$Z, Z^\prime $]]></tex-math></inline-formula> bosons with the DCHs, we have to change the basis <inline-formula><tex-math notation="LaTeX" id="ImEquation565"><![CDATA[$\big (\rho ^{--}, \rho ^{\prime --}, \chi ^{--}, \chi ^{\prime --}\big )$]]></tex-math></inline-formula> into the physical mass states <inline-formula><tex-math notation="LaTeX" id="ImEquation566"><![CDATA[$\big (G^{--}, H^{--}_1, H^{--}_2, H^{--}_3\big )$]]></tex-math></inline-formula>. Based on (<xref rid="PTV155M40" ref-type="disp-formula">40</xref>), if we ignore the suppressed terms containing a factor of <inline-formula><tex-math notation="LaTeX" id="ImEquation567"><![CDATA[$m^2_W/m^2_V$]]></tex-math></inline-formula>, we can estimate the <inline-formula><tex-math notation="LaTeX" id="ImEquation568"><![CDATA[$H^{--}H^{++}V^0$]]></tex-math></inline-formula> couplings. In the limit <inline-formula><tex-math notation="LaTeX" id="ImEquation569"><![CDATA[$\Lambda _{11}\simeq 1$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation570"><![CDATA[$\Lambda _{12}=\Lambda _{13}\rightarrow 0$]]></tex-math></inline-formula>, the couplings of two different DCHs with gauge bosons are very suppressed. So we only investigate the couplings of <inline-formula><tex-math notation="LaTeX" id="ImEquation571"><![CDATA[$H^{++}_iH^{--}_i V$]]></tex-math></inline-formula>. These couplings are almost independent of <inline-formula><tex-math notation="LaTeX" id="ImEquation572"><![CDATA[$\Lambda _{ij}$]]></tex-math></inline-formula> or the masses of DCHs, as given in Table <xref ref-type="table" rid="PTV155TB2">2</xref>.
<table-wrap id="PTV155TB2" position="float"><label>Table 2.</label>
<caption><p>Couplings of DCHs with neutral gauge bosons.</p></caption>
<table frame="hsides" rules="groups">
<colgroup>
<col align="left"/>
<col align="center"/>
<col align="center"/>
<col align="center"/>
</colgroup>
<thead><tr>
<th align="left"><inline-formula><tex-math notation="LaTeX" id="ImEquation573"><![CDATA[$V^{\mu }H^{--}_iH^{++}_i\big (p+p'\big )_{\mu }$]]></tex-math></inline-formula></th>
<th align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation574"><![CDATA[$A^{\mu }$]]></tex-math></inline-formula></th>
<th align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation575"><![CDATA[$Z^{\mu }$]]></tex-math></inline-formula></th>
<th align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation576"><![CDATA[$Z^{\prime \mu }$]]></tex-math></inline-formula></th>
</tr>
</thead>
<tbody><tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation577"><![CDATA[$H^{\pm \pm }_1$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation578"><![CDATA[$2\textit {ie}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation579"><![CDATA[$\dfrac {ig}{2\sqrt {3}} \left (\dfrac {2t^2-3}{\sqrt {2t^2+3}}s_{\zeta }-c_{\zeta }\right )$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation580"><![CDATA[$\dfrac {ig}{2\sqrt {3}} \left (\dfrac {2t^2-3}{\sqrt {2t^2+3}}c_{\zeta }+s_{\zeta }\right )$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation581"><![CDATA[$H^{\pm \pm }_{2,3}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation582"><![CDATA[$2\textit {ie}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation583"><![CDATA[$\dfrac {ig}{2\sqrt {3}} \left (\dfrac {2t^2-3}{\sqrt {2t^2+3}}s_{\zeta }+c_{\zeta }\right )$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation584"><![CDATA[$\dfrac {ig}{2\sqrt {3}} \left (\dfrac {2t^2-3}{\sqrt {2t^2+3}}c_{\zeta }-s_{\zeta }\right )$]]></tex-math></inline-formula></td>
</tr>
</tbody>
</table>
</table-wrap>
</p>
</sec>
</sec>
<sec id="s4"><label>4.</label><title>Signal of doubly charged Higgses in <inline-formula><tex-math notation="LaTeX" id="ImEquation585"><![CDATA[$e^+e^-$]]></tex-math></inline-formula> colliders</title>
<p>In an <inline-formula><tex-math notation="LaTeX" id="ImEquation586"><![CDATA[$e^{+}e^{-}$]]></tex-math></inline-formula> collider, the reaction <inline-formula><tex-math notation="LaTeX" id="ImEquation587"><![CDATA[$e^{+}e^{-}\rightarrow H^{++}H^{--}$]]></tex-math></inline-formula> may involve the mediations of virtual neutral particles such as Higgses and gauge bosons. However, the main contributions relate only to neutral gauge bosons, as shown in the Feynman diagrams in Fig. <xref ref-type="fig" rid="PTV155F5">5</xref>.
<fig id="PTV155F5"><label>Fig. 5.</label>
<caption><p>Feynman diagrams for production of <inline-formula><tex-math notation="LaTeX" id="ImEquation588"><![CDATA[$H^{++}$]]></tex-math></inline-formula> and its decays in <inline-formula><tex-math notation="LaTeX" id="ImEquation589"><![CDATA[$e^+e^-$]]></tex-math></inline-formula> colliders.</p></caption>
<graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ptv15505"/>
</fig></p>
<p>In the center-of-mass (CM) frame, the differential cross section for each DCH is given by
<disp-formula id="PTV155M54"><label>(54)</label><tex-math notation="LaTeX" id="DmEquation67"><![CDATA[\begin{equation} \frac{d\sigma}{d(\cos\theta)}= \frac{1}{32\pi s} \sqrt{1- \frac{4m^2_{H^{\pm\pm}}}{s}}\left|\overline{\mathcal{M}} \right|^2, \end{equation}]]></tex-math>
</disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation590"><![CDATA[$s=(p_{1}+p_{2})^2=E^2_{{\rm cm}}$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation591"><![CDATA[$\mathcal {M}$]]></tex-math></inline-formula> is the scattering amplitude; <inline-formula><tex-math notation="LaTeX" id="ImEquation592"><![CDATA[$\theta $]]></tex-math></inline-formula> is the angle between <inline-formula><tex-math notation="LaTeX" id="ImEquation593"><![CDATA[$\vec {k}_1$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation594"><![CDATA[$\vec {p}_1$]]></tex-math></inline-formula>. The detailed calculation is shown in Appendix A. The final result is
<disp-formula id="PTV155M55"><label>(55)</label><tex-math notation="LaTeX" id="DmEquation68"><![CDATA[\begin{equation} \frac{d\sigma}{d(\cos\theta)} = -\frac{s}{32\pi} \sqrt{1- \frac{4m^2_{H^{\pm\pm}}}{s}} \times \left(|\lambda_L|^2+|\lambda_R|^2\right) \left(1+\cos^2\theta\right), \end{equation}]]></tex-math>
</disp-formula>
where
<disp-formula id="PTV155M56"><label>(56)</label><tex-math notation="LaTeX" id="DmEquation69"><![CDATA[\begin{align} \lambda^{H_1}_{L} &= \sum_{a} \frac{G^a_LG^a_H}{s-m^{a2}_V+ i m^a_V \Gamma_a} \nonumber \\ &= e^2\times \left[\frac{2}{s}+ \frac{\left(c_{\zeta}+\frac{3s_{\zeta}}{\sqrt{2t^2+3}}\right)\left(\frac{2t^2-3}{\sqrt{2t^2+3}}s_{\zeta}-c_{\zeta}\right)}{12 s^2_{\theta_W}\left(s-m^2_Z+im_Z\Gamma_Z\right)}+ \frac{\left(-s_{\zeta}+\frac{3c_{\zeta}}{\sqrt{2t^2+3}}\right) \left(\frac{2t^2-3}{\sqrt{2t^2+3}}c_{\zeta}+s_{\zeta}\right)}{12 s^2_{\theta_W}\left(s-m^2_{Z'}+im_{Z'}\Gamma_{Z'}\right)}\right], \end{align}]]></tex-math></disp-formula></p>
<p>where <inline-formula><tex-math notation="LaTeX" id="ImEquation595"><![CDATA[$a=\gamma ,Z,Z'$]]></tex-math></inline-formula>, the total width of <inline-formula><tex-math notation="LaTeX" id="ImEquation596"><![CDATA[$Z'$]]></tex-math></inline-formula> is given in Appendix B, and
<disp-formula id="PTV155M57"><label>(57)</label><tex-math notation="LaTeX" id="DmEquation70"><![CDATA[\begin{align} \lambda^{H_1}_{R} &= \sum_{a} \frac{G^a_RG^a_H}{s-m^{a2}_V+i m^a_V \Gamma_a} \nonumber \\ &= e^2 \left[\frac{2}{s}- \frac{\left(\frac{2t^2-3}{\sqrt{2t^2+3}}s_{\zeta}-c_{\zeta}\right) \left(-\frac{3s_{\zeta}}{\sqrt{2t^2+3}}+c_{\zeta}\right)}{12 s^2_{\theta_W}\left(s-m^2_Z+im_Z\Gamma_Z\right)}- \frac{\left(\frac{2t^2-3}{\sqrt{2t^2+3}}c_{\zeta}+s_{\zeta}\right) \left(\frac{3c_{\zeta}}{\sqrt{2t^2+3}}+s_{\zeta}\right)}{12 s^2_{\theta_W}\left(s-m^2_{Z'}+im_{Z'}\Gamma_{Z'}\right)}\right]. \end{align}]]></tex-math>
</disp-formula>
Here <inline-formula><tex-math notation="LaTeX" id="ImEquation597"><![CDATA[$G^a_L, G^a_H$]]></tex-math></inline-formula> are the couplings of the neutral gauge bosons with two leptons and two DCHs, respectively.</p>
<p>Similarly, in the case of <inline-formula><tex-math notation="LaTeX" id="ImEquation598"><![CDATA[$H^{\pm \pm }_{2,3}$]]></tex-math></inline-formula>, we have
<disp-formula id="PTV155M58"><label>(58)</label><tex-math notation="LaTeX" id="DmEquation71"><![CDATA[\begin{equation} \lambda^{H_{2,3}}_{L} =e^2\times \left[\frac{2}{s}+ \frac{\left(c_{\zeta}+\frac{3s_{\zeta}}{\sqrt{2t^2+3}}\right) \left(\frac{2t^2-3}{\sqrt{2t^2+3}}s_{\zeta}+c_{\zeta}\right)}{12 s^2_{\theta_W}\left(s-m^2_Z+im_Z\Gamma_Z\right)}+ \frac{\left(\frac{3c_{\zeta}}{\sqrt{2t^2+3}}-s_{\zeta}\right) \left(\frac{2t^2-3}{\sqrt{2t^2+3}}c_{\zeta}-s_{\zeta}\right)}{12 s^2_{\theta_W}\left(s-m^2_{Z'}+im_{Z'}\Gamma_{Z'}\right)}\right]\end{equation}]]></tex-math>
</disp-formula>
and
<disp-formula id="PTV155M59"><label>(59)</label><tex-math notation="LaTeX" id="DmEquation72"><![CDATA[\begin{equation} \lambda^{H_{2,3}}_{R} =e^2 \left[\frac{2}{s}- \frac{\left(\frac{2t^2-3}{\sqrt{2t^2+3}}s_{\zeta}+c_{\zeta}\right) \left(c_{\zeta}-\frac{3s_{\zeta}}{\sqrt{2t^2+3}}\right)}{12 s^2_{\theta_W}\left(s-m^2_Z+im_Z\Gamma_Z\right)}- \frac{\left(\frac{2t^2-3}{\sqrt{2t^2+3}}c_{\zeta}-s_{\zeta}\right) \left(\frac{3c_{\zeta}}{\sqrt{2t^2+3}}+s_{\zeta}\right)}{12 s^2_{\theta_W}\left(s-m^2_{Z'}+im_{Z'}\Gamma_{Z'}\right)}\right].\end{equation}]]></tex-math>
</disp-formula>
The total cross section is
<disp-formula id="PTV155M60"><label>(60)</label><tex-math notation="LaTeX" id="DmEquation73"><![CDATA[\begin{align} \sigma &= \frac{s}{12\pi} \sqrt{1- \frac{4m^2_{H^{\pm\pm}}}{s}} \times \left(|\lambda_L|^2+|\lambda_R|^2\right). \end{align}]]></tex-math>
</disp-formula>
The above process happens only when <inline-formula><tex-math notation="LaTeX" id="ImEquation599"><![CDATA[$\sqrt {s}> 2 m_{H^{\pm \pm }}>400$]]></tex-math></inline-formula>&#x2009;GeV from the prediction of the SUSYRM331.</p>
<p>To determine the signals of the lightest DCH, we firstly investigate the dependence of the cross section of the process <inline-formula><tex-math notation="LaTeX" id="ImEquation600"><![CDATA[$e^+e^-\rightarrow H^{++}_3H^{--}_3$]]></tex-math></inline-formula> on the fixed collision energies of 0.5, 1, 2, and 3 TeV, as shown in Fig. <xref ref-type="fig" rid="PTV155F6">6</xref>. For <inline-formula><tex-math notation="LaTeX" id="ImEquation601"><![CDATA[$\sqrt {s}=0.5$]]></tex-math></inline-formula>&#x2009;TeV, with each fixed value of <inline-formula><tex-math notation="LaTeX" id="ImEquation602"><![CDATA[$m_V$]]></tex-math></inline-formula> there exists a very small range of <inline-formula><tex-math notation="LaTeX" id="ImEquation603"><![CDATA[$m_{A_1}$]]></tex-math></inline-formula> corresponding to the creation of <inline-formula><tex-math notation="LaTeX" id="ImEquation604"><![CDATA[$H^{\pm \pm }_3$]]></tex-math></inline-formula>. This is because a small <inline-formula><tex-math notation="LaTeX" id="ImEquation605"><![CDATA[$m_{A_1}$]]></tex-math></inline-formula> will create a tachyon DCH while large values will make the masses of the DCHs larger than the allowed kinetic condition. The cross section in this case can reach few pb. For larger <inline-formula><tex-math notation="LaTeX" id="ImEquation606"><![CDATA[$\sqrt {s}$]]></tex-math></inline-formula>, the cross sections decrease but still reach <inline-formula><tex-math notation="LaTeX" id="ImEquation607"><![CDATA[$\mathcal {O}$]]></tex-math></inline-formula>(0.1) pb. One of the most important properties of the lightest SUSYRM331 DCH is that its mass characterizes the difference between two parameters <inline-formula><tex-math notation="LaTeX" id="ImEquation608"><![CDATA[$m_{A_1}$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation609"><![CDATA[$m_V$]]></tex-math></inline-formula>. Hence, the signal of DCH requires near-degeneration between these two masses, <inline-formula><tex-math notation="LaTeX" id="ImEquation610"><![CDATA[$|m_{A_1}-m_V|<100$]]></tex-math></inline-formula>&#x2009;GeV when <inline-formula><tex-math notation="LaTeX" id="ImEquation611"><![CDATA[$\sqrt {s}\leq 1$]]></tex-math></inline-formula>&#x2009;TeV. We can also see that the low colliding energies give a rather large cross section for creating the lightest DCH.
<fig id="PTV155F6"><label>Fig. 6.</label>
<caption><p>Plots of the production cross sections of the lightest DCH <inline-formula><tex-math notation="LaTeX" id="ImEquation612"><![CDATA[$H^{\pm \pm }_{3}$]]></tex-math></inline-formula> as a function of <inline-formula><tex-math notation="LaTeX" id="ImEquation613"><![CDATA[$m_{A_1}$]]></tex-math></inline-formula> with different colliding energies. The values of <inline-formula><tex-math notation="LaTeX" id="ImEquation614"><![CDATA[$m_V$]]></tex-math></inline-formula> are <inline-formula><tex-math notation="LaTeX" id="ImEquation615"><![CDATA[$m_V =2$]]></tex-math></inline-formula>, 2.2, 2.5, and 2.8&#x2009;TeV, represented by dotted, dot-dashed, dashed, and solid curves, respectively.</p></caption>
<graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ptv15506"/>
</fig></p>
<p>The heavier DCHs may be created with very high collision energies, i.e., higher than 4&#x2009;TeV. For illustration, Fig. <xref ref-type="fig" rid="PTV155F7">7</xref> represents the total cross sections <inline-formula><tex-math notation="LaTeX" id="ImEquation616"><![CDATA[$\sigma (e^{+}e^{-}\rightarrow H^{++}H^{--})$]]></tex-math></inline-formula> of three DCHs in a CM energy of <inline-formula><tex-math notation="LaTeX" id="ImEquation617"><![CDATA[$\sqrt {s}=5$]]></tex-math></inline-formula>&#x2009;TeV, although this goes beyond the maximal energy that both ILC and CLIC can reach. Because all <inline-formula><tex-math notation="LaTeX" id="ImEquation618"><![CDATA[$m_{A_1},m_{A_2},m_V \gg m_{W}$]]></tex-math></inline-formula>, the cross sections of the DCHs depend weakly on the change of <inline-formula><tex-math notation="LaTeX" id="ImEquation619"><![CDATA[$m_{A_1}$]]></tex-math></inline-formula>. Apart from <inline-formula><tex-math notation="LaTeX" id="ImEquation620"><![CDATA[$m_{H^{\pm \pm }_{2,3}}$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation621"><![CDATA[$m_{A_1}$]]></tex-math></inline-formula> only affects the decay width of <inline-formula><tex-math notation="LaTeX" id="ImEquation622"><![CDATA[$m_{Z'}$]]></tex-math></inline-formula>, which makes a small contribution to the cross section in the limit of very large SUSY and <inline-formula><tex-math notation="LaTeX" id="ImEquation623"><![CDATA[${\rm SU}(3)_L$]]></tex-math></inline-formula> scales. A value of <inline-formula><tex-math notation="LaTeX" id="ImEquation624"><![CDATA[$m_V=2$]]></tex-math></inline-formula>&#x2009;TeV gives <inline-formula><tex-math notation="LaTeX" id="ImEquation625"><![CDATA[$m_{H^{\pm \pm }_1}\simeq \sqrt {m^2_{A_2}+m^2_{V}}=\sqrt {s}$]]></tex-math></inline-formula>, leading to a rather small cross section of <inline-formula><tex-math notation="LaTeX" id="ImEquation626"><![CDATA[$\mathcal {O}(10^{-2})$]]></tex-math></inline-formula>&#x2009;pb (the dotted curve in the left-hand panel), and does not depend on <inline-formula><tex-math notation="LaTeX" id="ImEquation627"><![CDATA[$m_{A_1}$]]></tex-math></inline-formula>, while the value of <inline-formula><tex-math notation="LaTeX" id="ImEquation628"><![CDATA[$m_V=2.5$]]></tex-math></inline-formula>&#x2009;TeV gives <inline-formula><tex-math notation="LaTeX" id="ImEquation629"><![CDATA[$m_{H^{\pm \pm }_1}>\sqrt {s}$]]></tex-math></inline-formula>, and <inline-formula><tex-math notation="LaTeX" id="ImEquation630"><![CDATA[$H^{\pm \pm }_1$]]></tex-math></inline-formula> cannot appear. For <inline-formula><tex-math notation="LaTeX" id="ImEquation631"><![CDATA[$H^{\pm \pm }_2$]]></tex-math></inline-formula>, as explained above, its mass is also independent of small <inline-formula><tex-math notation="LaTeX" id="ImEquation632"><![CDATA[$m_{A_1}$]]></tex-math></inline-formula>. Furthermore, all couplings and gauge boson masses related to the cross sections are independent of the mentioned range of <inline-formula><tex-math notation="LaTeX" id="ImEquation633"><![CDATA[$m_{A_1}$]]></tex-math></inline-formula>. So the <inline-formula><tex-math notation="LaTeX" id="ImEquation634"><![CDATA[$\lambda ^{H}_{L,R}$]]></tex-math></inline-formula> shown in (<xref rid="PTV155M56" ref-type="disp-formula">56</xref>)&#x2013;(<xref rid="PTV155M59" ref-type="disp-formula">59</xref>) will become constant too, giving the same property of the cross section for this DCH. However, it is very sensitive to <inline-formula><tex-math notation="LaTeX" id="ImEquation635"><![CDATA[$m_V$]]></tex-math></inline-formula>. In particular, it can get a value of 0.1&#x2009;pb with <inline-formula><tex-math notation="LaTeX" id="ImEquation636"><![CDATA[$m_V=2$]]></tex-math></inline-formula>&#x2009;TeV but this reduces to <inline-formula><tex-math notation="LaTeX" id="ImEquation637"><![CDATA[$0.03$]]></tex-math></inline-formula>&#x2009;pb for <inline-formula><tex-math notation="LaTeX" id="ImEquation638"><![CDATA[$m_V=2.5$]]></tex-math></inline-formula>&#x2009;TeV. When <inline-formula><tex-math notation="LaTeX" id="ImEquation639"><![CDATA[$\sqrt {s}=5$]]></tex-math></inline-formula>&#x2009;TeV, the cross section of the lightest DCH is 0.1&#x2009;pb for all masses satisfying the kinetic condition, rather smaller than the other cases with <inline-formula><tex-math notation="LaTeX" id="ImEquation640"><![CDATA[$\sqrt {s}<3$]]></tex-math></inline-formula>&#x2009;TeV.
<fig id="PTV155F7"><label>Fig. 7.</label>
<caption><p>Total cross sections of creating three DCHs in <inline-formula><tex-math notation="LaTeX" id="ImEquation641"><![CDATA[$e^{+}e^{-}$]]></tex-math></inline-formula> colliders as a function of <inline-formula><tex-math notation="LaTeX" id="ImEquation642"><![CDATA[$m_{A_1}$]]></tex-math></inline-formula> at a very high colliding energy of 5&#x2009;TeV and <inline-formula><tex-math notation="LaTeX" id="ImEquation643"><![CDATA[$m_{V}= 2$]]></tex-math></inline-formula> (2.5)&#x2009;TeV. The heaviest DCH is represented by dotted curves, the second heaviest by dashed curves, and the lightest by solid curves.</p></caption>
<graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ptv15507"/>
</fig></p>
<p>Figures <xref ref-type="fig" rid="PTV155F6">6</xref> and <xref ref-type="fig" rid="PTV155F7">7</xref> only help us see the maximal values of the cross sections for creation of the DCHs. The above discussion does not include the lower bound on the lightest DCH mass. Figure <xref ref-type="fig" rid="PTV155F8">8</xref> is used to estimate the values of the cross sections for <inline-formula><tex-math notation="LaTeX" id="ImEquation644"><![CDATA[$\sqrt {s}=1$]]></tex-math></inline-formula>&#x2013;3&#x2009;TeV, including both the condition of the lower DCH mass bound and the allowed kinetic condition for creating heavy physical DCHs. Each panel in the figures has the same interesting properties. When a DCH mass approaches the limit of the kinetic-allowed value, the corresponding cross section will decrease to zero. This explains why the contours of these two quantities almost overlap each other in the limits of <inline-formula><tex-math notation="LaTeX" id="ImEquation645"><![CDATA[$m_{H^{\pm \pm }}\rightarrow \sqrt {s}/2$]]></tex-math></inline-formula> and cross section <inline-formula><tex-math notation="LaTeX" id="ImEquation646"><![CDATA[$\sigma \rightarrow 0$]]></tex-math></inline-formula>.
<fig id="PTV155F8"><label>Fig. 8.</label>
<caption><p>Contour plots of the mass and the production cross section of the lightest DCH in <inline-formula><tex-math notation="LaTeX" id="ImEquation647"><![CDATA[$e^{+}e^{-}$]]></tex-math></inline-formula> colliders as functions of <inline-formula><tex-math notation="LaTeX" id="ImEquation648"><![CDATA[$m_{V}$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation649"><![CDATA[$m_{A_1}$]]></tex-math></inline-formula> with different colliding energies of 1, 1.5, 2, and 3&#x2009;TeV. The mass and the cross section are represented by solid and dotted curves, respectively.</p></caption>
<graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ptv15508"/>
</fig></p>
<p>In Fig. <xref ref-type="fig" rid="PTV155F8">8</xref>, the cross section can reach a value of a few pb with <inline-formula><tex-math notation="LaTeX" id="ImEquation650"><![CDATA[$\sqrt {s}=1$]]></tex-math></inline-formula>&#x2009;TeV if a lower bound of the DHC mass of 200&#x2009;GeV is considered. In general, a value of a few pb can be reached by searching for a very light DCH with a mass below 250&#x2009;GeV in colliding energies in the range of 0.5&#x2013;1&#x2009;TeV. These values of the cross section are much smaller than the maximal value for <inline-formula><tex-math notation="LaTeX" id="ImEquation651"><![CDATA[$\sqrt {s}=0.5$]]></tex-math></inline-formula>&#x2009;TeV shown in Fig. <xref ref-type="fig" rid="PTV155F6">6</xref>. In addition, the region of the parameter space allowed for the DCH appearance is very narrow, implying the degeneration of <inline-formula><tex-math notation="LaTeX" id="ImEquation652"><![CDATA[$m_{A_1}$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation653"><![CDATA[$m_V$]]></tex-math></inline-formula>. With <inline-formula><tex-math notation="LaTeX" id="ImEquation654"><![CDATA[$\sqrt {s}=1.5$]]></tex-math></inline-formula>&#x2013;2&#x2009;TeV, the lightest DCH with mass 500&#x2009;GeV <inline-formula><tex-math notation="LaTeX" id="ImEquation655"><![CDATA[$<m_{H^{\pm \pm }_3}<750$]]></tex-math></inline-formula>&#x2009;GeV may be detected with the corresponding <inline-formula><tex-math notation="LaTeX" id="ImEquation656"><![CDATA[$ \sigma > 0.4$]]></tex-math></inline-formula>&#x2009;pb. More interestingly, it can reach 1&#x2009;pb, twice as large as in the case of <inline-formula><tex-math notation="LaTeX" id="ImEquation657"><![CDATA[$\sqrt {s}=1$]]></tex-math></inline-formula>&#x2009;Tev, if the mass is around 500&#x2009;GeV. For <inline-formula><tex-math notation="LaTeX" id="ImEquation658"><![CDATA[$\sqrt {s}=3.0$]]></tex-math></inline-formula>, the cross sections for <inline-formula><tex-math notation="LaTeX" id="ImEquation659"><![CDATA[$m_{H^{\pm \pm }_3} > 0.5$]]></tex-math></inline-formula>&#x2009;TeV are not larger than 0.3&#x2009;pb. This value is close to the maximal value shown in Fig. <xref ref-type="fig" rid="PTV155F6">6</xref>. From this, we can conclude that the largest cross section for searching for the lightest DCH with a mass from <inline-formula><tex-math notation="LaTeX" id="ImEquation660"><![CDATA[$0.5$]]></tex-math></inline-formula>&#x2013;0.75&#x2009;TeV corresponds to intermediate values of <inline-formula><tex-math notation="LaTeX" id="ImEquation661"><![CDATA[$\sqrt {s}$]]></tex-math></inline-formula> from 1.5&#x2013;2&#x2009;TeV.</p>
<p>Figure <xref ref-type="fig" rid="PTV155F9">9</xref> shows the rather small cross sections of creating all DCHs when <inline-formula><tex-math notation="LaTeX" id="ImEquation662"><![CDATA[$\sqrt {s}=5$]]></tex-math></inline-formula>&#x2009;TeV. For the lightest, the maximal is below 0.1&#x2009;pb, while for the two others the value is of the order of <inline-formula><tex-math notation="LaTeX" id="ImEquation663"><![CDATA[$10^{-2}$]]></tex-math></inline-formula>&#x2009;pb.
<fig id="PTV155F9"><label>Fig. 9.</label>
<caption><p>Contour plots of production cross sections of DCHs in <inline-formula><tex-math notation="LaTeX" id="ImEquation664"><![CDATA[$e^{+}e^{-}$]]></tex-math></inline-formula> colliders as a function of <inline-formula><tex-math notation="LaTeX" id="ImEquation665"><![CDATA[$m_{V}$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation666"><![CDATA[$m_{A_1}$]]></tex-math></inline-formula> at a colliding energy of 5&#x2009;TeV. The left panel focuses on the lightest DCH, where the dotted and solid curves describe the cross section and mass, respectively. The right panel represents the cross sections of the remaining two DCHs; the second heaviest and the heaviest are described by dashed and dotted curves, respectively. In addition, the dashed and solid thick curves represent the maximal mass values of the DCHs allowed by the kinetic condition.</p></caption>
<graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ptv15509"/>
</fig></p>
<p>All the above numerical investigations show that the production cross sections of the lightest DCHs in <inline-formula><tex-math notation="LaTeX" id="ImEquation667"><![CDATA[$e^+e^-$]]></tex-math></inline-formula> colliders can be reach values of <inline-formula><tex-math notation="LaTeX" id="ImEquation668"><![CDATA[$10^{-1}$]]></tex-math></inline-formula> to a few pb, depending on the DCH mass and the collision energy. This will be a good signal for the detection of the lightest DCH in near-future colliders [<xref ref-type="bibr" rid="PTV155C22">22</xref>&#x2013;<xref ref-type="bibr" rid="PTV155C25">25</xref>]. In particular, for the ILC, with a collision energy of 0.5&#x2013;1&#x2009;TeV, corresponding to an integrated luminosity of 500&#x2013;1000&#x2009;fb<inline-formula><tex-math notation="LaTeX" id="ImEquation669"><![CDATA[$^{-1}$]]></tex-math></inline-formula> [<xref ref-type="bibr" rid="PTV155C22">22</xref>, <xref ref-type="bibr" rid="PTV155C23">23</xref>], the number of events for creation of the lightest DCH will be around <inline-formula><tex-math notation="LaTeX" id="ImEquation670"><![CDATA[$5\times 10^5$]]></tex-math></inline-formula>&#x2013;<inline-formula><tex-math notation="LaTeX" id="ImEquation671"><![CDATA[$10^6$]]></tex-math></inline-formula>, corresponding to a DCH mass range of 200&#x2013;500&#x2009;GeV. With the CLIC [<xref ref-type="bibr" rid="PTV155C24">24</xref>, <xref ref-type="bibr" rid="PTV155C25">25</xref>], where the collision energy will increase to 3&#x2009;TeV or more, the lightest DCH may be observed with a larger mass range. Furthermore, the estimated integrated luminosity targets will be 1.5&#x2009;<inline-formula><tex-math notation="LaTeX" id="ImEquation672"><![CDATA[${\rm ab}^{-1}$]]></tex-math></inline-formula> at 1.4 (1.5)&#x2009;TeV and 2 <inline-formula><tex-math notation="LaTeX" id="ImEquation673"><![CDATA[${\rm ab}^{-1}$]]></tex-math></inline-formula> at 3&#x2009;TeV collision energy. The DCH with a mass below 750&#x2009;GeV gives the best signal with <inline-formula><tex-math notation="LaTeX" id="ImEquation674"><![CDATA[$\sqrt {s}=1.5$]]></tex-math></inline-formula>&#x2013;2&#x2009;TeV, where the observed number of events can reach <inline-formula><tex-math notation="LaTeX" id="ImEquation675"><![CDATA[$6\times 10^5$]]></tex-math></inline-formula>&#x2013;<inline-formula><tex-math notation="LaTeX" id="ImEquation676"><![CDATA[$1.5\times 10^6$]]></tex-math></inline-formula>. With <inline-formula><tex-math notation="LaTeX" id="ImEquation677"><![CDATA[$s=3$]]></tex-math></inline-formula>&#x2009;TeV, the maximal number of events reduces to <inline-formula><tex-math notation="LaTeX" id="ImEquation678"><![CDATA[$6\times 10^5$]]></tex-math></inline-formula>. When the collision energy is high enough to create heavy DCHs, the number of events reduces to <inline-formula><tex-math notation="LaTeX" id="ImEquation679"><![CDATA[$10^4$]]></tex-math></inline-formula>, corresponding to a luminosity of 1&#x2009;<inline-formula><tex-math notation="LaTeX" id="ImEquation680"><![CDATA[${\rm ab}^{-1}$]]></tex-math></inline-formula>.</p>
</sec>
<sec id="s5"><label>5.</label><title>Conclusions</title>
<p>We have investigated the Higgs sector of the SUSYRM331 model, where the DCHs are particularly concentrated on as one of the signals indicating new physics at <inline-formula><tex-math notation="LaTeX" id="ImEquation681"><![CDATA[$e^+e^-$]]></tex-math></inline-formula> colliders. Here, the masses of neutral CP-even Higgses, DCHs, and the cross sections of the creation of DCHs at <inline-formula><tex-math notation="LaTeX" id="ImEquation682"><![CDATA[$e^+e^-$]]></tex-math></inline-formula> colliders can be represented according to five unknown parameters: two masses <inline-formula><tex-math notation="LaTeX" id="ImEquation683"><![CDATA[$m_{A_1,A_2}$]]></tex-math></inline-formula> of neutral CP-odd Higgses characterizing the soft scale; the mass of the singly charged heavy gauge boson <inline-formula><tex-math notation="LaTeX" id="ImEquation684"><![CDATA[$m_V$]]></tex-math></inline-formula>&#x2013;<inline-formula><tex-math notation="LaTeX" id="ImEquation685"><![CDATA[${\rm SU}(3)_L$]]></tex-math></inline-formula> breaking scale; and both <inline-formula><tex-math notation="LaTeX" id="ImEquation686"><![CDATA[${\gamma }$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation687"><![CDATA[${\beta }$]]></tex-math></inline-formula>, relating to the ratios of the VEVs. This choice of parameters helps us to discuss the relations among not only particle masses but also the breaking scales of the model more easily. We have found the exact condition <inline-formula><tex-math notation="LaTeX" id="ImEquation688"><![CDATA[$\frac {\left (m^2_{A_1}+m^2_W\right ) c_{2\gamma }}{m^2_V} <c_{2\beta }<\frac {m^2_W c_{2\gamma }}{m^2_V+m^2_{A_2}}<0$]]></tex-math></inline-formula> that must be satisfied to avoid tachyons of the DCHs at the tree level. The numerical investigation of the DCHs as a function of <inline-formula><tex-math notation="LaTeX" id="ImEquation689"><![CDATA[$m_{A_1}$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation690"><![CDATA[$m_V$]]></tex-math></inline-formula> shows that, even with very large values of <inline-formula><tex-math notation="LaTeX" id="ImEquation691"><![CDATA[$m_{A_1}$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation692"><![CDATA[$m_{A_2}$]]></tex-math></inline-formula>, and <inline-formula><tex-math notation="LaTeX" id="ImEquation693"><![CDATA[$m_V$]]></tex-math></inline-formula>, there may still exist a light DCH if the value of <inline-formula><tex-math notation="LaTeX" id="ImEquation694"><![CDATA[$m_{A_1}$]]></tex-math></inline-formula> is close enough to that of <inline-formula><tex-math notation="LaTeX" id="ImEquation695"><![CDATA[$m_V$]]></tex-math></inline-formula>, being consistent with the relation <inline-formula><tex-math notation="LaTeX" id="ImEquation696"><![CDATA[$ 0<-c_{2\beta }\left [c_{2\beta } m^2_V- c_{2\gamma } \left (m^2_W +m^2_{A_1}\right )\right ] \sim \mathcal {O}\big (m^2_W\big )$]]></tex-math></inline-formula> found by our analysis. The constraint on the decay <inline-formula><tex-math notation="LaTeX" id="ImEquation697"><![CDATA[$H^0_1\rightarrow \gamma \gamma $]]></tex-math></inline-formula> gives a lower bound on the mass of the DCH of about 200&#x2009;GeV, the same as the experimental value given by CMS. Finally, we have investigated the possibility of creating DCHs in <inline-formula><tex-math notation="LaTeX" id="ImEquation698"><![CDATA[$e^+e^-$]]></tex-math></inline-formula> colliders with collision energies from 1 to 3&#x2009;TeV, and indicated that only the lightest DCH may be created. The production cross sections range from 0.1 to a few pb, depending on the mass range and the collision energy. Because the SUSYRM331 is valid in the limit of the very large <inline-formula><tex-math notation="LaTeX" id="ImEquation699"><![CDATA[${\rm SU}(3)_L$]]></tex-math></inline-formula> scale, the two other DCHs always have masses above 2&#x2009;TeV; therefore, they do not appear unless the collision energies are higher than 4&#x2009;TeV. In any case, they will give small cross sections for all three DCHs, of the order of <inline-formula><tex-math notation="LaTeX" id="ImEquation700"><![CDATA[$\mathcal {O}(10^{-2})$]]></tex-math></inline-formula> pb for the two heavier DCHs and 0.1&#x2009;pb for the lightest. The two heavier DCHs are difficult to observe in the LHC, ILC, and CLIC. On the other hand, the lightest DCH, which only decays to a same-sign pair of charged tauons, gives the most promising signal for searching for it in <inline-formula><tex-math notation="LaTeX" id="ImEquation701"><![CDATA[$e^+e^-$]]></tex-math></inline-formula> colliders such as the ILC and CLIC. If it is detected, the numerical investigation in this work will give interesting information on parameters such as <inline-formula><tex-math notation="LaTeX" id="ImEquation702"><![CDATA[$m_{A_1}$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation703"><![CDATA[$m_V$]]></tex-math></inline-formula>.</p>
</sec>
<sec id="s6"><title>Funding</title>
<p>Open Access funding: <funding-source>SCOAP<sup>3</sup></funding-source>.</p>
</sec>
</body>
<back>
<ack><title>Acknowledgments</title>
<p>This research is funded by the Vietnam National Foundation for Science and Technology Development (NAFOSTED) under grant number 103.01-2014.69.</p>
</ack>
<app-group>
<app><title>Appendix A. Cross section of <inline-formula><tex-math notation="LaTeX" id="ImEquation704"><![CDATA[$e^{+}e^{-}\rightarrow H^{++}H^{--}$]]></tex-math></inline-formula></title>
<sec id="s7"><title/>
<p>The Lagrangian for the process <inline-formula><tex-math notation="LaTeX" id="ImEquation705"><![CDATA[$e^{+}e^{-} \rightarrow H^{++}H^{--}$]]></tex-math></inline-formula> can be written in terms of a two-component spinor:
<disp-formula id="PTV155M61"><label>(A1)</label><tex-math notation="LaTeX" id="DmEquation74"><![CDATA[\begin{equation} \mathcal{L}_{eeV^0}= -A^{a}_{\mu}\left(G^a_L e^{\dagger}\bar{\sigma}^{\mu}e-G^a_R e^{c\dagger}\bar{\sigma}^{\mu}e^c\right)+ \sum_{H=H^{\pm\pm}_{1,2,3}}G^a_H A^a_{\mu} \left( H^{++}\partial_{\mu}H^{--}-{\rm H.c.}\right),\end{equation}]]></tex-math>
</disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation706"><![CDATA[$A^a_{\mu }=A_{\mu }$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation707"><![CDATA[$Z_{\mu }$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation708"><![CDATA[$Z'_{\mu }$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation709"><![CDATA[$G^{a}_L$]]></tex-math></inline-formula>, and <inline-formula><tex-math notation="LaTeX" id="ImEquation710"><![CDATA[$G^a_R$]]></tex-math></inline-formula> are given in Table <xref ref-type="table" rid="PTV155TB1">1</xref>, and <inline-formula><tex-math notation="LaTeX" id="ImEquation711"><![CDATA[$G^a_H$]]></tex-math></inline-formula> is given in Table <xref ref-type="table" rid="PTV155TB2">2</xref>. The Feynman rules can be found in, e.g., Ref. [<xref ref-type="bibr" rid="PTV155C96">96</xref>]; the details are shown in Fig. <xref ref-type="fig" rid="PTV155FA1">A.1</xref>.
<fig id="PTV155FA1"><label>Fig. A.1.</label>
<caption><p>Feynman rules for interacting vertices of <inline-formula><tex-math notation="LaTeX" id="ImEquation712"><![CDATA[$llA^a$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation713"><![CDATA[$H^{++}H^{--}A^a$]]></tex-math></inline-formula>, where <inline-formula><tex-math notation="LaTeX" id="ImEquation714"><![CDATA[$A^a$]]></tex-math></inline-formula> is a physical neutral gauge boson.</p></caption>
<graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ptv15510"/>
</fig></p>
<p>Denoting <inline-formula><tex-math notation="LaTeX" id="ImEquation715"><![CDATA[$k=k_2-k_1$]]></tex-math></inline-formula>, the total amplitude for each DCH is written as
<disp-formula id="PTV155M62"><label>(A2)</label><tex-math notation="LaTeX" id="DmEquation75"><![CDATA[\begin{align} i\mathcal{M}_H&= -i\left(x^{\dagger}_2[\bar{\sigma}.k]x_1\right)\sum_{a} \frac{G^a_LG^a_H}{(p_1+p_2)^2-m^{a2}_V}-i \left(y_2[\sigma.k]y^{\dagger}_1\right)\sum_{a} \frac{G^a_LG^a_H}{(p_1+p_2)^2-m^{a2}_V} \nonumber \\ &\equiv -i \left(x^{\dagger}_2[\bar{\sigma}.k]x_1\right)\lambda_L-i \left(y_2[\sigma.k]y^{\dagger}_1\right)\lambda_R, \end{align}]]></tex-math>
</disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation716"><![CDATA[$m^a_V=0$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation717"><![CDATA[$m_Z$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation718"><![CDATA[$m_{Z'}$]]></tex-math></inline-formula> correspond to photons and <inline-formula><tex-math notation="LaTeX" id="ImEquation719"><![CDATA[$Z$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation720"><![CDATA[$Z'$]]></tex-math></inline-formula> bosons. Squaring the amplitude and summing over the electron and positron spins, we have
<disp-formula id="PTV155M63"><label>(A3)</label><tex-math notation="LaTeX" id="DmEquation76"><![CDATA[\begin{align} \left|\overline{\mathcal{M}} \right|^2&= \sum_{s_1,s_2}\mathcal{M}_H^{\dagger}\mathcal{M}_H \nonumber \\ &= 2\left(|\lambda_L|^2+|\lambda_R|^2\right)\left[ 2(p_1.k)(p_2.k)-(p_1.p_2) k^2\right]+ 2 \Re(\lambda_L^* \lambda_R) m_e^2 k^2. \end{align}]]></tex-math>
</disp-formula>
Now we use the fact that <inline-formula><tex-math notation="LaTeX" id="ImEquation721"><![CDATA[$p_1^2=p_2^2=m^2_e\simeq 0$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation722"><![CDATA[$k^2_1=k^2_2=m^2_{H^{\pm \pm }}$]]></tex-math></inline-formula>. Furthermore, all terms in (<xref rid="PTV155M63" ref-type="disp-formula">A3</xref>) are invariant under the Lorentz transformation, so the result is unchanged when we use any particular frame. Here we use the center-of-mass frame where the momenta of the two initial particles are
<disp-formula id="PTV155M64"><label>(A4)</label><tex-math notation="LaTeX" id="DmEquation77"><![CDATA[\begin{equation} p_{1\mu}=\left( E,0,0,E\right), \quad p_{2\mu}=\left(E,0,0,-E\right)\end{equation}]]></tex-math>
</disp-formula>
with <inline-formula><tex-math notation="LaTeX" id="ImEquation723"><![CDATA[$E=E_{\rm cm}/2=\sqrt {s}/2$]]></tex-math></inline-formula>. We define the two four-momenta of the final particles as <inline-formula><tex-math notation="LaTeX" id="ImEquation724"><![CDATA[$k_{1\mu }=(E_1,\vec {k}_1)$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation725"><![CDATA[$k_{2\mu }=(E_2,\vec {k}_2)$]]></tex-math></inline-formula>. Using the condition of four-momentum conservation, it is easy to prove the following results:
<disp-formula id="PTV155M65"><label>(A5)</label><tex-math notation="LaTeX" id="DmEquation78"><![CDATA[\begin{align} k^2&= (k_1-k_2)^2=4m^2_{H^{\pm\pm}}-s,\quad p_1.k=-p_2.k=\frac{s\cos\theta}{2}\sqrt{1-\frac{4m^2_{H^{\pm\pm}}}{s}} \nonumber \\ p_1.p_2&= \frac{s}{2}-m^2_e\simeq \frac{s}{2}. \end{align}]]></tex-math>
</disp-formula>
Inserting all results (<xref rid="PTV155M65" ref-type="disp-formula">A5</xref>) into (<xref rid="PTV155M63" ref-type="disp-formula">A3</xref>), we obtain
<disp-formula id="PTV155M66"><label>(A6)</label><tex-math notation="LaTeX" id="DmEquation79"><![CDATA[\begin{align} \left|\overline{\mathcal{M}} \right|^2&= -\left(|\lambda_L|^2+|\lambda_R|^2\right) s^2 \left(1+\cos^2\theta\right)+ 2 \Re(\lambda_L^* \lambda_R) m_e^2 \left(s-4m^2_{H^{\pm\pm}}\right)\nonumber \\ &\simeq -\left(|\lambda_L|^2+|\lambda_R|^2\right) s^2 \left(1+\cos^2\theta\right). \end{align}]]></tex-math></disp-formula></p>
</sec>
</app>
<app><title>Appendix B. Total width of the <inline-formula><tex-math notation="LaTeX" id="ImEquation726"><![CDATA[$Z'$]]></tex-math></inline-formula> gauge boson</title>
<sec id="s8"><title/>
<p>For any particles <inline-formula><tex-math notation="LaTeX" id="ImEquation727"><![CDATA[$\phi $]]></tex-math></inline-formula> (fermion, gauge boson, scalar) in the model, we define the corresponding covariant derivative related to neutral gauge bosons as <inline-formula><tex-math notation="LaTeX" id="ImEquation728"><![CDATA[$D_{\mu } \phi \equiv \left ( \partial _{\mu }-i q_{\phi } A_{\mu } -i g^{\phi }_{Z} Z_{\mu }-ig^{\phi }_{Z'} Z'_{\mu }\right )\phi $]]></tex-math></inline-formula>. The analytic forms of <inline-formula><tex-math notation="LaTeX" id="ImEquation729"><![CDATA[$g^{\phi }_{Z'}$]]></tex-math></inline-formula> depend on the particular representation of <inline-formula><tex-math notation="LaTeX" id="ImEquation730"><![CDATA[$\phi $]]></tex-math></inline-formula>. In particular, we have
<list list-type="bullet">
<list-item><p><inline-formula><tex-math notation="LaTeX" id="ImEquation731"><![CDATA[${\rm SU(3)}_L$]]></tex-math></inline-formula> singlet
<disp-formula id="PTV155UM14"><tex-math notation="LaTeX" id="DmEquation80"><![CDATA[\[ g^{\phi}_{Z'}=\frac{-gY_{\phi}c_{\zeta}t^2}{\sqrt{3\big(2t^2+3\big)}} \] ]]></tex-math></disp-formula>
</p></list-item>
<list-item><p><inline-formula><tex-math notation="LaTeX" id="ImEquation732"><![CDATA[${\rm SU(3)}_L$]]></tex-math></inline-formula> triplet
<disp-formula id="PTV155UM15"><tex-math notation="LaTeX" id="DmEquation81"><![CDATA[\[ g^{\phi}_{Z'} =\frac{g}{2\sqrt{3}}\left(\begin{matrix} - 2\left( s_{\zeta}+\dfrac{Y_{\phi}t^2c_{\zeta}}{\sqrt{2t^2+3}}\right) &0 & 0 \\
 0 &s_{\zeta}-\dfrac{c_{\zeta}\left(2Y_{\phi}t^2+3\right)}{\sqrt{2t^2+3}} & 0 \\
 0 & 0 &s_{\zeta}+\dfrac{c_{\zeta}\left(-2Y_{\phi}t^2+3\right)}{\sqrt{2t^2+3}} \\
 \end{matrix}\right) \] ]]></tex-math></disp-formula>
</p></list-item>
<list-item><p><inline-formula><tex-math notation="LaTeX" id="ImEquation733"><![CDATA[${\rm SU(3)}_L$]]></tex-math></inline-formula> antitriplet
<disp-formula id="PTV155UM16"><tex-math notation="LaTeX" id="DmEquation82"><![CDATA[\[ g^{\phi}_{Z'}=\frac{g}{2\sqrt{3}}\left(\begin{matrix} 2\left( s_{\zeta}-\dfrac{Y_{\phi}t^2c_{\zeta}}{\sqrt{2t^2+3}}\right) &0 & 0 \\
 0 &-s_{\zeta}-\dfrac{c_{\zeta}\left(2Y_{\phi}t^2-3\right)}{\sqrt{2t^2+3}} & 0 \\
 0 & 0 &-s_{\zeta}-\dfrac{c_{\zeta}\left(2Y_{\phi}t^2+3\right)}{\sqrt{2t^2+3}} \\
 \end{matrix}\right) \] ]]></tex-math></disp-formula>
</p></list-item>
<list-item><p>The <inline-formula><tex-math notation="LaTeX" id="ImEquation734"><![CDATA[${\rm SU(3)}_L$]]></tex-math></inline-formula> adjoint representation relates to gauge bosons and their superpartners only. The standard couplings of three gauge bosons can be written as <inline-formula><tex-math notation="LaTeX" id="ImEquation735"><![CDATA[$i g^{V}_{Z'} \left [g^{\mu \nu }(p-k_1)^{\sigma }\right .$]]></tex-math></inline-formula> <inline-formula><tex-math notation="LaTeX" id="ImEquation736"><![CDATA[$\left .+g^{\sigma \nu }(k_1-k_2)^{\mu }+g^{\mu \sigma }(k_2-p)^{\nu }\right ]$]]></tex-math></inline-formula>, where <inline-formula><tex-math notation="LaTeX" id="ImEquation737"><![CDATA[$g^{VV'}_{Z'}$]]></tex-math></inline-formula> is shown in Table <xref ref-type="table" rid="PTV155TBB1">B.1</xref>. With gauginos, the vertices can also be written in the form of <inline-formula><tex-math notation="LaTeX" id="ImEquation738"><![CDATA[$ig^{\tilde {V}}_{Z'}Z'_{\mu }\tilde {V}^{\dagger }\bar {\sigma }^{\mu }\tilde {V}$]]></tex-math></inline-formula>, where <inline-formula><tex-math notation="LaTeX" id="ImEquation739"><![CDATA[$g^{\tilde {V}}_{Z'}=g^{V}_{Z'}$]]></tex-math></inline-formula>.</p></list-item>
</list>
<table-wrap id="PTV155TBB1" position="float"><label>Table B.1.</label>
<caption><p>Couplings of the <inline-formula><tex-math notation="LaTeX" id="ImEquation740"><![CDATA[$Z'$]]></tex-math></inline-formula> gauge boson with two gauge bosons (two gauginos).</p></caption>
<table frame="hsides" rules="groups">
<colgroup>
<col align="left"/>
<col align="center"/>
<col align="center"/>
<col align="center"/>
</colgroup>
<thead><tr>
<th align="left">Gauge boson</th>
<th align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation741"><![CDATA[$Z'W^+W^-$]]></tex-math></inline-formula></th>
<th align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation742"><![CDATA[$Z'U^{++}U^{--}$]]></tex-math></inline-formula></th>
<th align="center"><inline-formula><tex-math notation="LaTeX" id="ImEquation743"><![CDATA[$Z'V^+V^-$]]></tex-math></inline-formula></th>
</tr>
</thead>
<tbody><tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation744"><![CDATA[$g^{V}_{Z'}$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation745"><![CDATA[$(g^{\widetilde {V}}_{Z'})$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation746"><![CDATA[$\dfrac {g\sqrt {3}}{2}\left (-s_{\zeta }+ \dfrac {c_{\zeta }}{\sqrt {2t^2+3}}\right )$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation747"><![CDATA[$ -\dfrac {g\sqrt {3}c_{\zeta }}{\sqrt {2t^2+3}}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation748"><![CDATA[$-\dfrac {g\sqrt {3}}{2} \left (s_{\zeta }+\dfrac {c_{\zeta }}{\sqrt {2t^2+3}}\right )$]]></tex-math></inline-formula></td>
</tr>
</tbody>
</table>
</table-wrap></p>
<p>Below, we will calculate the partial decay width of <inline-formula><tex-math notation="LaTeX" id="ImEquation749"><![CDATA[$Z'$]]></tex-math></inline-formula> into three different classes of particles. Analytic formulas can be found in Ref. [<xref ref-type="bibr" rid="PTV155C95">95</xref>]. For the purpose of estimating the total width decays of <inline-formula><tex-math notation="LaTeX" id="ImEquation750"><![CDATA[$Z'$]]></tex-math></inline-formula> as simply as possible, we only consider the largest contribution to each class of particles. In addition, all particles such as gauginos, sleptons, squarks receiving masses from the soft terms are very heavy, so that <inline-formula><tex-math notation="LaTeX" id="ImEquation751"><![CDATA[$Z'$]]></tex-math></inline-formula> cannot decay into them. We assume similar situations for cases of exotic quarks. The decay of the <inline-formula><tex-math notation="LaTeX" id="ImEquation752"><![CDATA[$Z'$]]></tex-math></inline-formula> related to these particles deserves further detailed study. Here the following numerical values are used: <inline-formula><tex-math notation="LaTeX" id="ImEquation753"><![CDATA[$s_{\zeta }= 0.155$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation754"><![CDATA[$c_{\zeta }=0.988$]]></tex-math></inline-formula>, corresponding to the definition (<xref rid="PTV155M8" ref-type="disp-formula">8</xref>) in the case <inline-formula><tex-math notation="LaTeX" id="ImEquation755"><![CDATA[$m_V\gg m_{W}$]]></tex-math></inline-formula>. The value of <inline-formula><tex-math notation="LaTeX" id="ImEquation756"><![CDATA[$t$]]></tex-math></inline-formula> follows the definition (<xref rid="PTV155M9" ref-type="disp-formula">9</xref>) with <inline-formula><tex-math notation="LaTeX" id="ImEquation757"><![CDATA[$s^2_{W}=0.231$]]></tex-math></inline-formula>.</p>
<sec id="s8a"><label>B.1.</label><title>Decay of <inline-formula><tex-math notation="LaTeX" id="ImEquation758"><![CDATA[$Z'$]]></tex-math></inline-formula> to fermions pairs</title>
<p>This kind of decay is involved with the Lagrangian below:
<disp-formula id="PTV155M67"><label>(B1)</label><tex-math notation="LaTeX" id="DmEquation83"><![CDATA[\begin{equation} \mathcal{L}_{Z'ff}= \sum_{f}Z^{\prime\mu}\left(g^{f}_{Z'} f^{\dagger}\overline{\sigma}_{\mu}f+ g^{f^c}_{Z'} f^{c\dagger}\overline{\sigma}_{\mu}f ^c\right)= \sum_{f}Z^{\prime\mu}\left( g^{f}_{Z'} f^{\dagger}\overline{\sigma}_{\mu}f- g^{f^c}_{Z'} f^{c}\sigma_{\mu}f ^{c\dagger}\right),\end{equation}]]></tex-math></disp-formula></p>
<p>where the sum is over all fermions in the model that couple with <inline-formula><tex-math notation="LaTeX" id="ImEquation759"><![CDATA[$Z'$]]></tex-math></inline-formula> and satisfy the kinetic condition <inline-formula><tex-math notation="LaTeX" id="ImEquation760"><![CDATA[$m_{Z'}> 2 m_{f}$]]></tex-math></inline-formula>. Formulas of <inline-formula><tex-math notation="LaTeX" id="ImEquation761"><![CDATA[$g^{f}_{Z'}$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation762"><![CDATA[$g^{f^c}_{Z'}$]]></tex-math></inline-formula> were shown in Table <xref ref-type="table" rid="PTV155TB1">1</xref>. The partial decay width corresponding to each fermion is [<xref ref-type="bibr" rid="PTV155C96">96</xref>]
<disp-formula id="PTV155M68"><label>(B2)</label><tex-math notation="LaTeX" id="DmEquation84"><![CDATA[\begin{align} \Gamma\Big(Z'\rightarrow ff^+\Big) & = \frac{N^f_c m_{Z'}}{24\pi}\left( 1-\frac{4m^2_f}{m^2_{Z'}}\right)^{1/2} \left[ \left( \Big|g^f_{Z'}\Big|^2+ \Big|g^{f^c}_{Z'}\Big|^2\right)\left(1-\frac{m^2_f}{m^2_{Z'}}\right)-6g^{f}_{Z'}g^{f^c}_{Z'} \frac{m^2_f}{m^2_{Z'}}\right] , \end{align}]]></tex-math>
</disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation763"><![CDATA[$N^f_c$]]></tex-math></inline-formula> is the color factor, being equal to 3 for quarks and 1 for all other fermions (leptons, quarks, Higgsinos, and gauginos).</p>
</sec>
<sec id="s8b"><label>B.2.</label><title>Decay of <inline-formula><tex-math notation="LaTeX" id="ImEquation764"><![CDATA[$Z'$]]></tex-math></inline-formula> to scalar pairs</title>
<p>The Lagrangian related to these decays is
<disp-formula id="PTV155M69"><label>(B3)</label><tex-math notation="LaTeX" id="DmEquation85"><![CDATA[\begin{equation} \mathcal{L}_{Z'S_iS_i}=\sum_{S_i,S_j}ig^{S_{ij}}_{Z'} Z'_{\mu}\left[ S_i^{\dagger} \partial^{\mu}S_j- (\partial^{\mu}S_i^{\dagger})S_i\right],\end{equation}]]></tex-math>
</disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation765"><![CDATA[$S_i$]]></tex-math></inline-formula> stands for any scalars in the model. The Feynman rule is the same as that for the DCH shown in Fig. <xref ref-type="fig" rid="PTV155FA1">A.1</xref>, where <inline-formula><tex-math notation="LaTeX" id="ImEquation766"><![CDATA[$G^a_H\rightarrow i g^{S_{ij}}_{Z'}$]]></tex-math></inline-formula>. Nonzero values of <inline-formula><tex-math notation="LaTeX" id="ImEquation767"><![CDATA[$ g^{S_{ij}}_{Z'}$]]></tex-math></inline-formula> for Higgses in the model are shown in Table <xref ref-type="table" rid="PTV155TBB2">B.2</xref>.
<table-wrap id="PTV155TBB2" position="float"><label>Table B.2.</label>
<caption><p><inline-formula><tex-math notation="LaTeX" id="ImEquation768"><![CDATA[$ZHH$]]></tex-math></inline-formula> couplings.</p></caption>
<table frame="hsides" rules="groups">
<colgroup>
<col align="left"/>
<col align="center"/>
<col align="center"/>
<col align="center"/>
</colgroup>
<thead><tr>
<th align="left">Vertex</th>
<th align="center">Factor</th>
<th align="center">Vertex</th>
<th align="center">Factor</th>
</tr>
</thead>
<tbody><tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation769"><![CDATA[$Z'H_1^{+}H_1^{-}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation770"><![CDATA[$\dfrac {-ig}{\sqrt {3}}\left (s_{\zeta }+\dfrac {t^2c_{\zeta }}{\sqrt {2t^2+3}}\right )$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation771"><![CDATA[$Z'H_2^{+}H_2^{-}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation772"><![CDATA[$\dfrac {-ig}{\sqrt {3}}\left (s_{\zeta }-\dfrac {t^2c_{\zeta }}{\sqrt {2t^2+3}}\right )$]]></tex-math></inline-formula></td>
</tr>
</tbody>
</table>
</table-wrap></p>
<p>If the momentum of the <inline-formula><tex-math notation="LaTeX" id="ImEquation773"><![CDATA[$Z'$]]></tex-math></inline-formula> boson is <inline-formula><tex-math notation="LaTeX" id="ImEquation774"><![CDATA[$p_{\mu }$]]></tex-math></inline-formula>, then we have <inline-formula><tex-math notation="LaTeX" id="ImEquation775"><![CDATA[$p^2=m^2_{Z'}$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation776"><![CDATA[$p=k_1+k_2$]]></tex-math></inline-formula>. The amplitude of the decay is
<disp-formula id="PTV155UM17"><tex-math notation="LaTeX" id="DmEquation86"><![CDATA[\[ i\mathcal{M}\big(Z'\rightarrow S_iS_j\big)=-g^{S_{ij}}_{Z'} \left( k_2-k_1\right)\cdot\varepsilon \]]]></tex-math>
</disp-formula>
with <inline-formula><tex-math notation="LaTeX" id="ImEquation777"><![CDATA[$\varepsilon _{\mu }=\varepsilon _{\mu }(p,\lambda _{Z'})$]]></tex-math></inline-formula> being the polarization vector of <inline-formula><tex-math notation="LaTeX" id="ImEquation778"><![CDATA[$Z'$]]></tex-math></inline-formula>.</p>
<p>Averaging over the <inline-formula><tex-math notation="LaTeX" id="ImEquation779"><![CDATA[$Z'$]]></tex-math></inline-formula> polarization using
<disp-formula id="PTV155M70"><label>(B4)</label><tex-math notation="LaTeX" id="DmEquation87"><![CDATA[\begin{equation} \frac{1}{3}\sum_{\lambda_{Z'}} \varepsilon_{\mu}\varepsilon^*_{\nu}=\frac{1}{3} \left( -g_{\mu\nu}+\frac{p_{\mu}p_{\mu}}{m^2_{Z'}}\right),\end{equation}]]></tex-math>
</disp-formula>
we obtain the squared amplitude
<disp-formula id="PTV155M71"><label>(B5)</label><tex-math notation="LaTeX" id="DmEquation88"><![CDATA[\begin{equation} \frac{1}{3}\Big|\mathcal{M}\Big(Z'\rightarrow S_iS_j\Big)\Big|^2=\frac{1}{3}\left| g^{S_{ij}}_{Z'} \right|^2\left[-(k_1-k_2)^2+\frac{\left(k_1^2-k^2_2\right)^2}{m^2_{Z'}}\right]. \end{equation}]]></tex-math>
</disp-formula>
Noting that <inline-formula><tex-math notation="LaTeX" id="ImEquation780"><![CDATA[$ k_1^2=m^2_{S_i}$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation781"><![CDATA[$k_2^2=m^2_{S_j}$]]></tex-math></inline-formula>, and <inline-formula><tex-math notation="LaTeX" id="ImEquation782"><![CDATA[$(k_1-k_2)^2=2\left ( m^2_{S_i}+m^2_{S_j}\right )-m^2_{Z'}$]]></tex-math></inline-formula> we have the formula of <inline-formula><tex-math notation="LaTeX" id="ImEquation783"><![CDATA[$\Gamma \big (Z'\rightarrow SS\big )$]]></tex-math></inline-formula>, namely,
<disp-formula id="PTV155M72"><label>(B6)</label><tex-math notation="LaTeX" id="DmEquation89"><![CDATA[\begin{align} \Gamma(Z'\rightarrow S_iS_j)&= \frac{1}{16 \pi m_{Z'}} \sqrt{\left(1-\frac{m^2_{S_i}+m^2_{S_j}}{m^2_{Z'}}\right)^2- \frac{4m^2_{S_i}m^2_{S_j}}{m^4_{Z'}}}\times \frac{1}{3}\Big|\mathcal{M}\Big(Z'\rightarrow S_iS_j\Big)\Big|^2 \nonumber \\ &= \frac{\left| g^{S_{ij}}_{Z'}\right|^2 m_{Z'} }{48\pi} \times \sqrt{\left(1-\frac{m^2_{S_i}+m^2_{S_j}}{m^2_{Z'}}\right)^2- \frac{4m^2_{S_i}m^2_{S_j}}{m^4_{Z'}}} \nonumber \\ & \quad \times \left[1-\frac{2(m^2_{S_i}+m^2_{S_j})}{m^2_{Z'}}+ \frac{\left(m^2_{S_i}-m^2_{S_j}\right)^2}{m^4_{Z'}}\right] \end{align}]]></tex-math>
</disp-formula>
for two distinguishable final states. For identical final states, there needs to be an extra factor <inline-formula><tex-math notation="LaTeX" id="ImEquation784"><![CDATA[$1/2$]]></tex-math></inline-formula> to avoid counting each final state twice [<xref ref-type="bibr" rid="PTV155C97">97</xref>]. Therefore, if <inline-formula><tex-math notation="LaTeX" id="ImEquation785"><![CDATA[$S_i\equiv S_j\rightarrow S$]]></tex-math></inline-formula>, then <inline-formula><tex-math notation="LaTeX" id="ImEquation786"><![CDATA[$m_{S_i} =m_{S_j}=m_S$]]></tex-math></inline-formula> and, denoting <inline-formula><tex-math notation="LaTeX" id="ImEquation787"><![CDATA[$g^{S_{ij}}_{Z'}=g^{S}_{Z'}$]]></tex-math></inline-formula>, we have a more simple formula:
<disp-formula id="PTV155M73"><label>(B7)</label><tex-math notation="LaTeX" id="DmEquation90"><![CDATA[\begin{equation} \Gamma\big(Z'\rightarrow SS\big)= \frac{| g^{S}_{Z'}|^2m_{Z'}}{96\pi }\left[ 1- \frac{4m^2_{S}}{m^2_{Z'}}\right]^{5/2} .\end{equation}]]></tex-math>
</disp-formula>
It is noted that <inline-formula><tex-math notation="LaTeX" id="ImEquation788"><![CDATA[$ | g^{S}_{Z'}|^2\sim g^2/12\times \mathcal {O}(1)$]]></tex-math></inline-formula>, as shown in Table <xref ref-type="table" rid="PTV155TB2">2</xref> for DCHs. This means that
<disp-formula id="PTV155M74"><label>(B8)</label><tex-math notation="LaTeX" id="DmEquation91"><![CDATA[\begin{equation} \Gamma\big(Z'\rightarrow SS\big) \sim \frac{g^2m_{Z'}}{576\pi}\times \mathcal{O}(1)\ll \Gamma\big(Z'\rightarrow ff\big). \end{equation}]]></tex-math></disp-formula>
<table-wrap id="PTV155TBB3" position="float"><label>Table B.3.</label>
<caption><p>Coupling of <inline-formula><tex-math notation="LaTeX" id="ImEquation789"><![CDATA[$Z'HV$]]></tex-math></inline-formula>.</p></caption>
<table frame="hsides" rules="groups">
<colgroup>
<col align="left"/>
<col align="center"/>
<col align="center"/>
<col align="center"/>
</colgroup>
<thead><tr>
<th align="left">Vertex</th>
<th align="center">Factor</th>
<th align="center">Vertex</th>
<th align="center">Factor</th>
</tr>
</thead>
<tbody><tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation790"><![CDATA[$Z'U^{\pm \pm }\rho ^{\mp \mp }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation791"><![CDATA[$\dfrac {igs_{\gamma }m_W}{\sqrt {3}}\left (s_{\zeta }-\dfrac {2c_{\zeta }t^2}{\sqrt {2t^2+3}}\right )$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation792"><![CDATA[$Z'U^{\pm \pm }\rho ^{\prime \mp \mp }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation793"><![CDATA[$\dfrac {igc_{\gamma }m_W}{\sqrt {3}} \left (s_{\zeta }-\dfrac {2c_{\zeta }t^2}{\sqrt {2t^2+3}}\right )$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation794"><![CDATA[$Z'U^{\pm \pm }\chi ^{\mp \mp }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation795"><![CDATA[$\dfrac {igs_{\beta }m_V}{\sqrt {3}}\left (s_{\zeta }+\dfrac {2c_{\zeta }t^2} {\sqrt {2t^2+3}}\right )$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation796"><![CDATA[$Z'U^{\pm \pm }\chi ^{\prime \mp \mp }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation797"><![CDATA[$\dfrac {igm_{V}c_{\beta }}{\sqrt {3}}\left (s_{\zeta }+\dfrac {2c_{\zeta }t^2} {\sqrt {2t^2+3}}\right )$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation798"><![CDATA[$Z'ZH_{\rho }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation799"><![CDATA[$\dfrac {2igc_{2\zeta }s_{\gamma }\sqrt {2t^2+3}m_V^2m_W}{3(m^2_V+m^2_W)}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation800"><![CDATA[$Z'ZH_{\rho '}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation801"><![CDATA[$\dfrac {2igc_{2\zeta }c_{\gamma }\sqrt {2t^2+3}m_V^2 m_W}{3(m^2_V+m^2_W)}$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation802"><![CDATA[$Z'ZH_{\chi }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation803"><![CDATA[$-\dfrac {2igc_{2\zeta }s_{\beta }\sqrt {2t^2+3}m_V m^2_W}{3(m^2_V+m^2_W)}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation804"><![CDATA[$Z'ZH_{\chi '}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation805"><![CDATA[$-\dfrac {2igc_{2\zeta }c_{\beta }\sqrt {2t^2+3}m_Vm^2_W}{3(m^2_V+m^2_W)}$]]></tex-math></inline-formula></td>
</tr>
</tbody>
</table>
</table-wrap></p>
</sec>
<sec id="s8c"><label>B.3.</label><title>Decay of <inline-formula><tex-math notation="LaTeX" id="ImEquation806"><![CDATA[$Z'$]]></tex-math></inline-formula> to one gauge boson and one scalar</title>
<p>This case happens only with scalars that inherit nonzero VEVs, i.e., neutral Higgses in the model. Detailed investigation shows that possible vertices are <inline-formula><tex-math notation="LaTeX" id="ImEquation807"><![CDATA[$Z'H^{++}U^{--}$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation808"><![CDATA[$Z'H^{--}U^{++}$]]></tex-math></inline-formula>, and <inline-formula><tex-math notation="LaTeX" id="ImEquation809"><![CDATA[$Z'ZH^{0}$]]></tex-math></inline-formula>. This part of the Lagrangian has the form <inline-formula><tex-math notation="LaTeX" id="ImEquation810"><![CDATA[$g^{SV}_{Z'}Z'_{\mu }V^{\mu }S$]]></tex-math></inline-formula>. Vertex factors are shown in Table <xref ref-type="table" rid="PTV155TBB3">B.3</xref>. The partial decay width for this case is
<disp-formula id="PTV155M75"><label>(B9)</label><tex-math notation="LaTeX" id="DmEquation92"><![CDATA[\begin{align} \Gamma(Z'\rightarrow SV)&= \frac{\left| g^{SV}_{Z'}\right|^2}{48\pi m_{Z'}}\times \sqrt{\left(1-\frac{m^2_V+m^2_S}{m^2_{Z'}}\right)^2-\frac{4m^2_Vm^2_S}{m^4_{Z'}}} \times \left[ 2+ \frac{\left(m^2_{Z'}+m^2_V-m^2_S\right)^2}{4m^2_Vm^2_{Z'}}\right]. \end{align}]]></tex-math>
</disp-formula>
We can estimate that the largest contributions to <inline-formula><tex-math notation="LaTeX" id="ImEquation811"><![CDATA[$ \Gamma (Z'\rightarrow SV)$]]></tex-math></inline-formula> are from <inline-formula><tex-math notation="LaTeX" id="ImEquation812"><![CDATA[$\chi $]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation813"><![CDATA[$\chi '$]]></tex-math></inline-formula>, namely, <inline-formula><tex-math notation="LaTeX" id="ImEquation814"><![CDATA[$\Gamma (Z'\rightarrow SV)= 0.06 g^2 m_{Z'}\times \mathcal {O}(1)$]]></tex-math></inline-formula>.</p>
</sec>
<sec id="s8d"><label>B.4.</label><title>Decay of <inline-formula><tex-math notation="LaTeX" id="ImEquation815"><![CDATA[$Z'$]]></tex-math></inline-formula> to gauge boson pairs</title>
<p>The possible decays are <inline-formula><tex-math notation="LaTeX" id="ImEquation816"><![CDATA[$Z'\rightarrow WW,VV,UU$]]></tex-math></inline-formula> with the respective couplings shown in Table <xref ref-type="table" rid="PTV155TBB1">B.1</xref>. The general vertex factor is <inline-formula><tex-math notation="LaTeX" id="ImEquation817"><![CDATA[$i g^{X}_{Z'}\left [g^{\mu \nu }(p-k_1)^{\sigma }+g^{\sigma \nu }(k_1-k_2)^{\mu } +g^{\mu \sigma }(k_2-p)^{\nu }\right ]$]]></tex-math></inline-formula>, where <inline-formula><tex-math notation="LaTeX" id="ImEquation818"><![CDATA[$X=W$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation819"><![CDATA[$U$]]></tex-math></inline-formula>, or <inline-formula><tex-math notation="LaTeX" id="ImEquation820"><![CDATA[$V$]]></tex-math></inline-formula> gauge bosons. The partial decay for each particle can be written by
<disp-formula id="PTV155M76"><label>(B10)</label><tex-math notation="LaTeX" id="DmEquation93"><![CDATA[\begin{equation} \Gamma(Z'\rightarrow XX)= \frac{\left| g^{X}_{Z'}\right|^2m_{Z'}}{192\pi } \left[1- \frac{4m^2_X} {m_{Z'}^2}\right]^{3/2} \frac{m^4_{Z'}+12m^4_{X}+20m^2_{X}m^2_{Z'}}{m^4_X}.\end{equation}]]></tex-math>
</disp-formula>
From the mass spectra of gauge bosons given in Appendix 2.2, we can see that, in the case of <inline-formula><tex-math notation="LaTeX" id="ImEquation821"><![CDATA[$m_W \ll m_V$]]></tex-math></inline-formula>, we have <inline-formula><tex-math notation="LaTeX" id="ImEquation822"><![CDATA[$ m^2_{Z'}\simeq \frac {2\big (t^2+2\big )}{3} m^2_U$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation823"><![CDATA[$m^2_U\simeq m^2_V$]]></tex-math></inline-formula>. Furthermore, from the definition of <inline-formula><tex-math notation="LaTeX" id="ImEquation824"><![CDATA[$\zeta $]]></tex-math></inline-formula> in (<xref rid="PTV155M8" ref-type="disp-formula">8</xref>), we can see that, in the limit of <inline-formula><tex-math notation="LaTeX" id="ImEquation825"><![CDATA[$m_W/m_V\rightarrow 0$]]></tex-math></inline-formula>, we get <inline-formula><tex-math notation="LaTeX" id="ImEquation826"><![CDATA[$g^W_{Z'}\rightarrow 0$]]></tex-math></inline-formula>. More exactly, if <inline-formula><tex-math notation="LaTeX" id="ImEquation827"><![CDATA[$m_W^2/m_V=\epsilon \ll 1$]]></tex-math></inline-formula>, then <inline-formula><tex-math notation="LaTeX" id="ImEquation828"><![CDATA[$g^W_{Z'} \simeq \frac {\sqrt {3}g \big (t^2+1\big )^2}{\sqrt {2}\big (t^2+2\big )^{3/2}} \times \frac {m_W^2}{m^2_V}$]]></tex-math></inline-formula>, leading to the result that <inline-formula><tex-math notation="LaTeX" id="ImEquation829"><![CDATA[$\Gamma (Z'\rightarrow W^+W^-)\simeq \frac {g^2 m_{Z'}(1+t^2)^2}{648\pi \big (t^2+2\big )}$]]></tex-math></inline-formula>. It is noted that, in this case, <inline-formula><tex-math notation="LaTeX" id="ImEquation830"><![CDATA[$c_{\zeta }\simeq 0.988$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation831"><![CDATA[$s_{\zeta } \simeq 0.155$]]></tex-math></inline-formula>.</p>
</sec>
</sec>
</app>
<app><title>Appendix C. Coupling of doubly charged Higgs</title>
<sec id="s9"><title/>
<p>Three-vertex coupling is shown in Table <xref ref-type="table" rid="PTV155TBC4">C.4</xref>, four-vertex coupling in Table <xref ref-type="table" rid="PTV155TBC5">C.5</xref>.
<table-wrap id="PTV155TBC5" position="float"><label>Table C.5.</label>
<caption><p>Four-vertex coupling of DCHs.</p></caption>
<table frame="hsides" rules="groups">
<colgroup>
<col align="left"/>
<col align="center"/>
<col align="center"/>
<col align="center"/>
</colgroup>
<thead><tr>
<th align="left">Vertex</th>
<th align="center">Factor</th>
<th align="center">Vertex</th>
<th align="center">Factor</th>
</tr>
</thead>
<tbody><tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation832"><![CDATA[$\rho ^{++}\rho ^{--} A^{\mu }A_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation833"><![CDATA[$4ie^2$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation834"><![CDATA[$\rho ^{\prime ++}\rho ^{\prime --} A^{\mu }A_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation835"><![CDATA[$4ie^2$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation836"><![CDATA[$\chi ^{++}\chi ^{--} A^{\mu }A_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation837"><![CDATA[$4ie^2$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation838"><![CDATA[$\chi ^{\prime ++}\chi ^{\prime --} A^{\mu }A_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation839"><![CDATA[$4ie^2$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation840"><![CDATA[$\rho ^{++}\rho ^{--} A^{\mu }Z_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation841"><![CDATA[$\dfrac {-i\sqrt {2}g^2 t}{\sqrt {3\big (2t^2+3\big )}}\left [ \dfrac {(2t^2-3)s_{\zeta }}{\sqrt {2t^2+3}}+c_{\zeta }\right ]$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation842"><![CDATA[$\rho ^{\prime ++}\rho ^{\prime --} A^{\mu }Z_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation843"><![CDATA[$\dfrac {-i\sqrt {2}g^2 t}{\sqrt {3\big (2t^2+3\big )}}\left [ \dfrac {(2t^2-3)s_{\zeta }}{\sqrt {2t^2+3}}+c_{\zeta }\right ]$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation844"><![CDATA[$\chi ^{++}\chi ^{--} A^{\mu }Z_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation845"><![CDATA[$\dfrac {-i\sqrt {2}g^2 t}{\sqrt {3\big (2t^2+3\big )}}\left [ \dfrac {(2t^2-3)s_{\zeta }}{\sqrt {2t^2+3}}-c_{\zeta }\right ]$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation846"><![CDATA[$\chi ^{\prime ++}\chi ^{\prime --} A^{\mu }Z_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation847"><![CDATA[$\dfrac {-i\sqrt {2}g^2 t}{\sqrt {3\big (2t^2+3\big )}}\left [ \dfrac {(2t^2-3)s_{\zeta }}{\sqrt {2t^2+3}}-c_{\zeta }\right ]$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation848"><![CDATA[$ \rho ^{++}H_{\rho } U^{--\mu }A_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation849"><![CDATA[$\dfrac {ie^2}{s_W}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation850"><![CDATA[$ \rho ^{\prime ++}H_{\rho '} U^{--\mu }A_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation851"><![CDATA[$\dfrac {ie^2}{s_W}$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation852"><![CDATA[$ \chi ^{++}H_{\chi } U^{--\mu }A_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation853"><![CDATA[$\dfrac {ie^2}{s_W}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation854"><![CDATA[$ \chi ^{\prime ++}H_{\chi '} U^{--\mu }A_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation855"><![CDATA[$\dfrac {ie^2}{s_W}$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation856"><![CDATA[$ \rho ^{++}H_{\rho } U^{--\mu }Z_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation857"><![CDATA[$-\dfrac {ig^2}{2\sqrt {3}} \left [\dfrac {2 t^2 s_{\zeta }}{\sqrt {2t^2+3}}+c_{\zeta }\right ]$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation858"><![CDATA[$ \rho ^{\prime ++}H_{\rho '} U^{--\mu }Z_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation859"><![CDATA[$-\dfrac {ig^2}{2\sqrt {3}} \left [\dfrac {2 t^2 s_{\zeta }}{\sqrt {2t^2+3}}+c_{\zeta }\right ]$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation860"><![CDATA[$ \chi ^{++}H_{\chi } U^{--\mu }Z_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation861"><![CDATA[$\dfrac {ig^2}{2\sqrt {3}} \left [\dfrac {2 t^2 s_{\zeta }}{\sqrt {2t^2+3}}-c_{\zeta }\right ]$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation862"><![CDATA[$ \chi ^{\prime ++}H_{\chi '} U^{--\mu }Z_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation863"><![CDATA[$\dfrac {ig^2}{2\sqrt {3}} \left [\dfrac {2 t^2 s_{\zeta }}{\sqrt {2t^2+3}}-c_{\zeta }\right ]$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation864"><![CDATA[$ \rho ^{++}H_{\rho } V^{-\mu }W^{-}_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation865"><![CDATA[$\dfrac {ig^2}{2\sqrt {2}}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation866"><![CDATA[$ \rho ^{\prime ++}H_{\rho '} V^{-\mu }W^{-}_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation867"><![CDATA[$\dfrac {ig^2}{2\sqrt {2}}$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation868"><![CDATA[$ \chi ^{++}H_{\chi } V^{-\mu }W^{-}_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation869"><![CDATA[$\dfrac {ig^2}{2\sqrt {2}}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation870"><![CDATA[$ \chi ^{\prime ++}H_{\chi '} V^{-\mu }W^{-}_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation871"><![CDATA[$\dfrac {ig^2}{2\sqrt {2}}$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation872"><![CDATA[$ \rho ^{++}H_{A_1} U^{--\mu }A_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation873"><![CDATA[$\dfrac {e^2c_{\gamma }}{s_W}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation874"><![CDATA[$ \rho ^{\prime ++}H_{A_1} U^{--\mu }A_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation875"><![CDATA[$\dfrac {-e^2s_{\gamma }}{s_W}$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation876"><![CDATA[$ \chi ^{++}H_{A_2} U^{--\mu }A_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation877"><![CDATA[$\dfrac {e^2c_{\beta }}{s_W}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation878"><![CDATA[$ \chi ^{\prime ++}H_{A_2} U^{--\mu }A_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation879"><![CDATA[$-\dfrac {e^2s_{\beta }}{s_W}$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation880"><![CDATA[$ \rho ^{++}H_{A_1} U^{--\mu }Z_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation881"><![CDATA[$-\dfrac {g^2c_{\gamma }}{2\sqrt {3}} \left [\dfrac {2 t^2 s_{\zeta }}{\sqrt {2t^2+3}}+c_{\zeta }\right ]$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation882"><![CDATA[$ \rho ^{\prime ++}H_{A_1} U^{--\mu }Z_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation883"><![CDATA[$\dfrac {g^2s_{\gamma }}{2\sqrt {3}} \left [\dfrac {2 t^2 s_{\zeta }}{\sqrt {2t^2+3}}+c_{\zeta }\right ]$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation884"><![CDATA[$ \chi ^{++}H_{A_2} U^{--\mu }Z_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation885"><![CDATA[$-\dfrac {g^2c_{\beta }}{2\sqrt {3}} \left [\dfrac {2 t^2 s_{\zeta }}{\sqrt {2t^2+3}}-c_{\zeta }\right ]$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation886"><![CDATA[$ \chi ^{\prime ++}H_{A_2} U^{--\mu }Z_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation887"><![CDATA[$\dfrac {g^2s_{\beta }}{2\sqrt {3}} \left [\dfrac {2 t^2 s_{\zeta }}{\sqrt {2t^2+3}}-c_{\zeta }\right ]$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation888"><![CDATA[$ \rho ^{++}H_{A_1} V^{-\mu }W^{-}_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation889"><![CDATA[$\dfrac {g^2c_{\gamma }}{2\sqrt {2}}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation890"><![CDATA[$ \rho ^{\prime ++}H_{A_1} V^{-\mu }W^{-}_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation891"><![CDATA[$\dfrac {-g^2s_{\gamma }}{2\sqrt {2}}$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation892"><![CDATA[$ \chi ^{++}H_{A_2} V^{-\mu }W^{-}_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation893"><![CDATA[$\dfrac {-g^2c_{\beta }}{2\sqrt {2}}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation894"><![CDATA[$ \chi ^{\prime ++}H_{A_2} V^{-\mu }W^{-}_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation895"><![CDATA[$\dfrac {g^2s_{\beta }}{2\sqrt {2}}$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation896"><![CDATA[$ \rho ^{++}H^-_{1} V^{-\mu }A_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation897"><![CDATA[$\dfrac {-3ie^2c_{\gamma }}{\sqrt {2}s_W}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation898"><![CDATA[$ \rho ^{\prime ++}H^-_{1} V^{-\mu }A_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation899"><![CDATA[$\dfrac {3ie^2s_{\gamma }}{\sqrt {2}s_W}$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation900"><![CDATA[$ \chi ^{++}H^-_{2} W^{-\mu }A_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation901"><![CDATA[$\dfrac {3ie^2c_{\beta }}{\sqrt {2}s_W}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation902"><![CDATA[$ \chi ^{\prime ++}H^-_{2} W^{-\mu }A_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation903"><![CDATA[$\dfrac {-3ie^2s_{\beta }}{\sqrt {2}s_W}$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation904"><![CDATA[$ \rho ^{++}H^-_{1} U^{--\mu }W^{+}_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation905"><![CDATA[$\dfrac {-ig^2c_{\gamma }}{2}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation906"><![CDATA[$ \rho ^{\prime ++}H^-_{1} U^{--\mu }W^{+}_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation907"><![CDATA[$\dfrac {ig^2s_{\gamma }}{2}$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation908"><![CDATA[$ \chi ^{++}H^-_{2} U^{--\mu }V^{+}_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation909"><![CDATA[$\dfrac {-ig^2c_{\beta }}{2}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation910"><![CDATA[$ \chi ^{\prime ++}H^-_{2} U^{--\mu }V^{+}_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation911"><![CDATA[$\dfrac {ig^2s_{\beta }}{2}$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation912"><![CDATA[$ \rho ^{++}H^-_{1} V^{-\mu }Z_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation913"><![CDATA[$\dfrac {ig^2c_{\gamma }}{2\sqrt {6}} \left [\dfrac {(4 t^2-3) s_{\zeta }}{\sqrt {2t^2+3}}-c_{\zeta }\right ]$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation914"><![CDATA[$ \rho ^{\prime ++}H^-_{1} V^{-\mu }Z_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation915"><![CDATA[$-\dfrac {ig^2 s_{\gamma }}{2\sqrt {6}} \left [\dfrac {(4 t^2-3) s_{\zeta }}{\sqrt {2t^2+3}}-c_{\zeta }\right ]$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation916"><![CDATA[$ \chi ^{++}H^-_{1}W^{-\mu }Z_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation917"><![CDATA[$\dfrac {ig^2c_{\beta }}{2\sqrt {6}} \left [\dfrac {(4 t^2-3) s_{\zeta }}{\sqrt {2t^2+3}}+c_{\zeta }\right ]$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation918"><![CDATA[$ \chi ^{\prime ++}H^-_{1} W^{-\mu }Z_{\mu }$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation919"><![CDATA[$-\dfrac {ig^2 s_{\beta }}{2\sqrt {6}} \left [\dfrac {(4 t^2-3) s_{\zeta }}{\sqrt {2t^2+3}}+c_{\zeta }\right ]$]]></tex-math></inline-formula></td>
</tr>
</tbody>
</table>
</table-wrap></p>
</sec>
</app>
</app-group>
<fn-group>
<fn id="fn1"><label>1</label><p>Note that the well known <inline-formula><tex-math notation="LaTeX" id="ImEquation920"><![CDATA[$\beta $]]></tex-math></inline-formula> in the MSSM is different from our definition of <inline-formula><tex-math notation="LaTeX" id="ImEquation921"><![CDATA[$\beta $]]></tex-math></inline-formula> in (<xref rid="PTV155M23" ref-type="disp-formula">23</xref>). In fact, the <inline-formula><tex-math notation="LaTeX" id="ImEquation922"><![CDATA[$\gamma $]]></tex-math></inline-formula> parameter in
(<xref rid="PTV155M23" ref-type="disp-formula">23</xref>) plays the same role as <inline-formula><tex-math notation="LaTeX" id="ImEquation923"><![CDATA[$\beta $]]></tex-math></inline-formula> in the MSSM.</p></fn>
</fn-group>
<ref-list><title>References</title>
<ref id="PTV155C1"><label>1</label><mixed-citation publication-type="journal"><collab>ATLAS Collaboration</collab>, <source>Phys. Lett. B</source> <volume>716</volume>, <fpage>1</fpage> (<year>2012</year>) [<elocation-id content-type="arxiv">arXiv:1207.7214</elocation-id>] [<comment><ext-link ext-link-type="uri" xlink:href="http://inspirehep.net/search?p=find+EPRINT+arXiv:1207.7214">Search inSPIRE</ext-link></comment>]hep-ex. <comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1016/j.physletb.2012.08.020">doi:10.1016/j.physletb.2012.08.020</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C2"><label>2</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Aad</surname> <given-names>G.</given-names></string-name></person-group> et al. [<collab>CMS Collaboration</collab>], <source>Phys. Lett. B</source> <volume>716</volume>, <fpage>30</fpage> (<year>2012</year>) [<elocation-id content-type="arxiv">arXiv:1207.7235</elocation-id>] [<comment><ext-link ext-link-type="uri" xlink:href="http://inspirehep.net/search?p=find+EPRINT+arXiv:1207.7235">Search inSPIRE</ext-link></comment>]hep-ex. <comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1016/j.physletb.2012.08.021">doi:10.1016/j.physletb.2012.08.021</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C3"><label>3</label><mixed-citation publication-type="journal"><collab>CMS Collaboration</collab>, <source>Eur. Phys. J. C</source> <volume>74</volume>, <fpage>3076</fpage> (<year>2014</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1140/epjc/s10052-014-3076-z">doi:10.1140/epjc/s10052-014-3076-z</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C4"><label>4</label><mixed-citation publication-type="journal"><collab>CMS Collaboration</collab>, <source>Eur. Phys. J. C</source> <volume>75</volume>, <fpage>212</fpage> (<year>2015</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1140/epjc/s10052-015-3351-7">doi:10.1140/epjc/s10052-015-3351-7</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C5"><label>5</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Mohopatra</surname> <given-names>R. N.</given-names></string-name> and <string-name><surname>Pati</surname> <given-names>J. C.</given-names></string-name></person-group>, <source>Phys. Rev. D</source> <volume>11</volume>, <fpage>2558</fpage> (<year>1975</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.11.2558">doi:10.1103/PhysRevD.11.2558</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C6"><label>6</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Senjanovic</surname> <given-names>G.</given-names></string-name> and <string-name><surname>Mohopatra</surname> <given-names>R. N.</given-names></string-name></person-group>, <source>Phys. Rev. D</source> <volume>12</volume>, <fpage>1502</fpage> (<year>1975</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.12.1502">doi:10.1103/PhysRevD.12.1502</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C7"><label>7</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Senjanovic</surname> <given-names>G.</given-names></string-name></person-group>, <source>Nucl. Phys. B</source> <volume>153</volume>, <fpage>334</fpage> (<year>1979</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1016/0550-3213(79)90604-7">doi:10.1016/0550-3213(79)90604-7</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C8"><label>8</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Zee</surname> <given-names>A.</given-names></string-name></person-group>, <source>Nucl. Phys. B</source> <volume>264</volume>, <fpage>99</fpage> (<year>1986</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1016/0550-3213(86)90475-X">doi:10.1016/0550-3213(86)90475-X</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C9"><label>9</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Babu</surname> <given-names>K. S.</given-names></string-name></person-group>, <source>Phys. Lett. B</source> <volume>203</volume>, <fpage>132</fpage> (<year>1988</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1016/0370-2693(88)91584-5">doi:10.1016/0370-2693(88)91584-5</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C10"><label>10</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Pisano</surname> <given-names>F.</given-names></string-name> and <string-name><surname>Pleitez</surname> <given-names>V.</given-names></string-name></person-group>, <source>Phys. Rev. D</source> <volume>46</volume>, <fpage>410</fpage> (<year>1992</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.46.410">doi:10.1103/PhysRevD.46.410</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C11"><label>11</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Foot</surname> <given-names>R.</given-names></string-name>, <string-name><surname>Hernandez</surname> <given-names>O. F.</given-names></string-name>, <string-name><surname>Pisano</surname> <given-names>F.</given-names></string-name>, and <string-name><surname>Pleitez</surname> <given-names>V.</given-names></string-name></person-group>, <source>Phys. Rev. D</source> <volume>47</volume>, <fpage>4158</fpage> (<year>1993</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.47.4158">doi:10.1103/PhysRevD.47.4158</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C12"><label>12</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Ferreira</surname> <given-names>J. G.</given-names> <suffix>Jr</suffix></string-name>, <string-name><surname>Pinheiro</surname> <given-names>P. R. D.</given-names></string-name>, <string-name><surname>de S. Pires</surname> <given-names>C. A.</given-names></string-name>, and <string-name><surname>Rodrigues da Silva</surname> <given-names>P. S.</given-names></string-name></person-group>, <source>Phys. Rev. D</source> <volume>84</volume>, <fpage>095019</fpage> (<year>2011</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.84.095019">doi:10.1103/PhysRevD.84.095019</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C13"><label>13</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Frampton</surname> <given-names>P. H.</given-names></string-name></person-group>, <source>Phys. Rev. Lett.</source> <volume>69</volume>, <fpage>2889</fpage> (<year>1992</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevLett.69.2889">doi:10.1103/PhysRevLett.69.2889</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C14"><label>14</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Kuchimanchi</surname> <given-names>R.</given-names></string-name> and <string-name><surname>Mohapatra</surname> <given-names>R. N.</given-names></string-name></person-group>, <source>Phys. Rev. D</source> <volume>48</volume>, <fpage>4352</fpage> (<year>1993</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.48.4352">doi:10.1103/PhysRevD.48.4352</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C15"><label>15</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Aulakh</surname> <given-names>C. S.</given-names></string-name>, <string-name><surname>Melfo</surname> <given-names>A.</given-names></string-name>, and <string-name><surname>Senjanovic</surname> <given-names>G.</given-names></string-name></person-group>, <source>Phys. Rev. D</source> <volume>57</volume>, <fpage>4174</fpage> (<year>1998</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.57.4174">doi:10.1103/PhysRevD.57.4174</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C16"><label>16</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Aulakh</surname> <given-names>C. S.</given-names></string-name>, <string-name><surname>Melfo</surname> <given-names>A.</given-names></string-name>, <string-name><surname>Rasin</surname> <given-names>A.</given-names></string-name>, and <string-name><surname>Senjanovic</surname> <given-names>G.</given-names></string-name></person-group>, <source>Phys. Rev. D</source> <volume>58</volume>, <fpage>115007</fpage> (<year>1998</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.58.115007">doi:10.1103/PhysRevD.58.115007</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C17"><label>17</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Chacko</surname> <given-names>Z.</given-names></string-name> and <string-name><surname>Mohapatra</surname> <given-names>R. N.</given-names></string-name></person-group>, <source>Phys. Rev. D</source> <volume>58</volume>, <fpage>015003</fpage> (<year>1998</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.58.015003">doi:10.1103/PhysRevD.58.015003</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C18"><label>18</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Babu</surname> <given-names>K. S.</given-names></string-name> and <string-name><surname>Mohapatra</surname> <given-names>R. N.</given-names></string-name></person-group>, <source>Phys. Lett. B</source> <volume>668</volume>, <fpage>404</fpage> (<year>2008</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1016/j.physletb.2008.09.018">doi:10.1016/j.physletb.2008.09.018</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C19"><label>19</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Montero</surname> <given-names>J. C.</given-names></string-name>, <string-name><surname>Pleitez</surname> <given-names>V.</given-names></string-name>, and <string-name><surname>Rodriguez</surname> <given-names>M. C.</given-names></string-name></person-group>, <source>Phys. Rev. D</source> <volume>65</volume>, <fpage>035006</fpage> (<year>2002</year>) [<elocation-id content-type="arxiv">arXiv:hep-ph/0012178</elocation-id>]. <comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.65.035006">doi:10.1103/PhysRevD.65.035006</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C20"><label>20</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Huong</surname> <given-names>D. T.</given-names></string-name>, <string-name><surname>Hue</surname> <given-names>L. T.</given-names></string-name>, <string-name><surname>Rodriguez</surname> <given-names>M. C.</given-names></string-name>, and <string-name><surname>Long</surname> <given-names>H. N.</given-names></string-name></person-group>, <source>Nucl. Phys. B</source> <volume>870</volume>, <fpage>293</fpage> (<year>2013</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1016/j.nuclphysb.2013.01.016">doi:10.1016/j.nuclphysb.2013.01.016</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C21"><label>21</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Ferreira</surname> <given-names>J. G.</given-names></string-name>, <string-name><surname>de S. Pires</surname> <given-names>C. A.</given-names></string-name>, <string-name><surname>Rodrigues da Silva</surname> <given-names>P. S.</given-names></string-name>, and <string-name><surname>Sampieri</surname> <given-names>A.</given-names></string-name></person-group>, <source>Phys. Rev. D</source> <volume>88</volume>, <fpage>105013</fpage> (<year>2013</year>) [<elocation-id content-type="arxiv">arXiv:1308.0575</elocation-id>] [<comment><ext-link ext-link-type="uri" xlink:href="http://inspirehep.net/search?p=find+EPRINT+arXiv:1308.0575">Search inSPIRE</ext-link></comment>]hep-ph. <comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.88.105013">doi:10.1103/PhysRevD.88.105013</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C22"><label>22</label><mixed-citation publication-type="other"><person-group person-group-type="author"><string-name><surname>Behnke</surname> <given-names>T.</given-names></string-name></person-group> et al., [<elocation-id content-type="arxiv">arXiv:1306.6327</elocation-id>] [<comment><ext-link ext-link-type="uri" xlink:href="http://inspirehep.net/search?p=find+EPRINT+arXiv:1306.6327">Search inSPIRE</ext-link></comment>]physics.acc-ph.</mixed-citation></ref>
<ref id="PTV155C23"><label>23</label><mixed-citation publication-type="other"><person-group person-group-type="author"><string-name><surname>Baer</surname> <given-names>H.</given-names></string-name></person-group> et al., [<elocation-id content-type="arxiv">arXiv:1306.6352</elocation-id>] [<comment><ext-link ext-link-type="uri" xlink:href="http://inspirehep.net/search?p=find+EPRINT+arXiv:1306.6352">Search inSPIRE</ext-link></comment>]hep-ph.</mixed-citation></ref>
<ref id="PTV155C24"><label>24</label><mixed-citation publication-type="other"><person-group person-group-type="author"><string-name><surname>Accomando</surname> <given-names>E.</given-names></string-name></person-group> et al. [<collab>CLIC Physics Working Group Collaboration</collab>], [<elocation-id content-type="arxiv">arXiv:hep-ph/0412251</elocation-id>[<comment><ext-link ext-link-type="uri" xlink:href="http://inspirehep.net/search?p=find+EPRINT+arXiv:hep-ph/0412251">Search inSPIRE</ext-link></comment>].</mixed-citation></ref>
<ref id="PTV155C25"><label>25</label><mixed-citation publication-type="other"><person-group person-group-type="author"><string-name><surname>Linssen</surname> <given-names>L.</given-names></string-name>, <string-name><surname>Miyamoto</surname> <given-names>A.</given-names></string-name>, <string-name><surname>Stanitzki</surname> <given-names>M.</given-names></string-name>, and <string-name><surname>Weerts</surname> <given-names>H.</given-names></string-name></person-group>, <comment><italic>Physics and Detectors at CLIC: CLIC Conceptual Design Report</italic>, CERN-2012-003</comment>, [<elocation-id content-type="arxiv">arXiv:1202.5940</elocation-id>] [<comment><ext-link ext-link-type="uri" xlink:href="http://inspirehep.net/search?p=find+EPRINT+arXiv:1202.5940">Search inSPIRE</ext-link></comment>]physics.ins-det.</mixed-citation></ref>
<ref id="PTV155C26"><label>26</label><mixed-citation publication-type="journal"><collab>CMS Collaboration</collab>, <source>Eur. Phys. J. C</source> <volume>72</volume>, <fpage>2189</fpage> (<year>2012</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1140/epjc/s10052-012-2189-5">doi:10.1140/epjc/s10052-012-2189-5</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C27"><label>27</label><mixed-citation publication-type="journal"><collab>ATLAS Collaboration</collab>, <source>Eur. Phys. J. C</source> <volume>72</volume>, <fpage>2244</fpage> (<year>2012</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1140/epjc/s10052-012-2244-2">doi:10.1140/epjc/s10052-012-2244-2</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C28"><label>28</label><mixed-citation publication-type="journal"><collab>ATLAS Collaboration</collab>, <source>J. High Energy Phys.</source> <volume>1503</volume>, <fpage>041</fpage> (<year>2015</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1007/JHEP03(2015)041">doi:10.1007/JHEP03(2015)041</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C29"><label>29</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Beringer</surname> <given-names>J.</given-names></string-name></person-group> et al. <source>[Particle Data Group], Phys. Rev. D</source> <volume>86</volume>, <fpage>010001</fpage> (<year>2012</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.86.010001">doi:10.1103/PhysRevD.86.010001</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C30"><label>30</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Huitu</surname> <given-names>K.</given-names></string-name>, <string-name><surname>Maalampi</surname> <given-names>J.</given-names></string-name>, <string-name><surname>Pietila</surname> <given-names>A.</given-names></string-name>, and <string-name><surname>Raidal</surname> <given-names>M.</given-names></string-name></person-group>, <source>Nucl. Phys. B</source> <volume>487</volume>, <fpage>27</fpage> (<year>1997</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1016/S0550-3213(97)87466-4">doi:10.1016/S0550-3213(97)87466-4</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C31"><label>31</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Gunion</surname> <given-names>J. F.</given-names></string-name></person-group>, <source>Int. J. Mod. Phys. A</source> <volume>11</volume>, <fpage>1551</fpage> (<year>1996</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1142/S0217751X96000730">doi:10.1142/S0217751X96000730</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C32"><label>32</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Babu</surname> <given-names>K. S.</given-names></string-name>, <string-name><surname>Patra</surname> <given-names>A.</given-names></string-name>, and <string-name><surname>Rai</surname> <given-names>S. K.</given-names></string-name></person-group>, <source>Phys. Rev. D</source> <volume>88</volume>, <fpage>055006</fpage> (<year>2013</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.88.055006">doi:10.1103/PhysRevD.88.055006</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C33"><label>33</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Montalvo</surname> <given-names>J. E. C.</given-names></string-name>, <string-name><surname>Cortez</surname> <given-names>N. V.</given-names></string-name>, and <string-name><surname>Tonasse</surname> <given-names>M. D.</given-names></string-name></person-group>, <source>Phys. Rev. D</source> <volume>78</volume>, <fpage>116003</fpage> (<year>2008</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.78.116003">doi:10.1103/PhysRevD.78.116003</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C34"><label>34</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Montalvo</surname> <given-names>J. E. C.</given-names></string-name>, <string-name><surname>Ulloa</surname> <given-names>G. H. R</given-names></string-name>, and <string-name><surname>Tonasse</surname> <given-names>M. D.</given-names></string-name></person-group>, <source>Eur. Phys. J. C</source> <volume>72</volume>, <fpage>2210</fpage> (<year>2012</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1140/epjc/s10052-012-2210-z">doi:10.1140/epjc/s10052-012-2210-z</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C35"><label>35</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Kanemura</surname> <given-names>S.</given-names></string-name>, <string-name><surname>Kikuchi</surname> <given-names>M.</given-names></string-name>, <string-name><surname>Yokoya</surname> <given-names>H.</given-names></string-name>, and <string-name><surname>Yagyu</surname> <given-names>K.</given-names></string-name></person-group>, <source>Prog. Theor. Exp. Phys.</source> <volume>2015</volume>, <fpage>051B02</fpage> (<year>2015</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1093/ptep/ptv071">doi:10.1093/ptep/ptv071</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C36"><label>36</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Kanemura</surname> <given-names>S.</given-names></string-name>, <string-name><surname>Kikuchi</surname> <given-names>M.</given-names></string-name>, <string-name><surname>Yagyu</surname> <given-names>K.</given-names></string-name>, and <string-name><surname>Yokoya</surname> <given-names>H.</given-names></string-name></person-group>, <source>Phys. Rev. D</source> <volume>90</volume>, <fpage>115018</fpage> (<year>2014</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.90.115018">doi:10.1103/PhysRevD.90.115018</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C37"><label>37</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Chen</surname> <given-names>C. H.</given-names></string-name> and <string-name><surname>Nomura</surname> <given-names>T.</given-names></string-name></person-group>, <source>Phys. Rev. D</source> <volume>91</volume>, <fpage>035023</fpage> (<year>2015</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.91.035023">doi:10.1103/PhysRevD.91.035023</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C38"><label>38</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Binh</surname> <given-names>D. T.</given-names></string-name>, <string-name><surname>Hue</surname> <given-names>L. T.</given-names></string-name>, <string-name><surname>Huong</surname> <given-names>D. T.</given-names></string-name>, and <string-name><surname>Long</surname> <given-names>H. N.</given-names></string-name></person-group>, <source>Eur. Phys. J. C</source> <volume>74</volume>, <fpage>2851</fpage> (<year>2014</year>) [<elocation-id content-type="arxiv">arXiv:1308.3085</elocation-id>] [<comment><ext-link ext-link-type="uri" xlink:href="http://inspirehep.net/search?p=find+EPRINT+arXiv:1308.3085">Search inSPIRE</ext-link></comment>]hep-ph. <comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1140/epjc/s10052-014-2851-1">doi:10.1140/epjc/s10052-014-2851-1</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C39"><label>39</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Dong</surname> <given-names>P. V.</given-names></string-name>, <string-name><surname>Tham</surname> <given-names>T. D.</given-names></string-name>, and <string-name><surname>Hung</surname> <given-names>H. T.</given-names></string-name></person-group>, <source>Phys. Rev. D</source> <volume>87</volume>, <fpage>115003</fpage> (<year>2013</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.87.115003">doi:10.1103/PhysRevD.87.115003</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C40"><label>40</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Dong</surname> <given-names>P. V.</given-names></string-name>, <string-name><surname>Huong</surname> <given-names>D. T.</given-names></string-name>, <string-name><surname>Queiroz</surname> <given-names>F. S.</given-names></string-name>, and <string-name><surname>Thuy</surname> <given-names>N. T.</given-names></string-name></person-group>, <source>Phys. Rev. D</source> <volume>90</volume>, <fpage>075021</fpage> (<year>2014</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.90.075021">doi:10.1103/PhysRevD.90.075021</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C41"><label>41</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Huong</surname> <given-names>D. T.</given-names></string-name>, <string-name><surname>Dong</surname> <given-names>P. V.</given-names></string-name>, <string-name><surname>Kim</surname> <given-names>C. S.</given-names></string-name>, and <string-name><surname>Thuy</surname> <given-names>N. T.</given-names></string-name></person-group>, <source>Phys. Rev. D</source> <volume>91</volume>, <fpage>055023</fpage> (<year>2015</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.91.055023">doi:10.1103/PhysRevD.91.055023</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C42"><label>42</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Huong</surname> <given-names>D. T.</given-names></string-name> and <string-name><surname>Long</surname> <given-names>H. N.</given-names></string-name></person-group>, <source>J. Phys. G</source> <volume>38</volume>, <fpage>015202</fpage> (<year>2011</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1088/0954-3899/38/1/015202">doi:10.1088/0954-3899/38/1/015202</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C43"><label>43</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Huong</surname> <given-names>D. T.</given-names></string-name> and <string-name><surname>Long</surname> <given-names>H. N.</given-names></string-name></person-group>, <source>Phys. Atom. Nucl.</source> <volume>73</volume>, <fpage>791</fpage> (<year>2010</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1134/S1063778810050078">doi:10.1134/S1063778810050078</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C44"><label>44</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Singer</surname> <given-names>M.</given-names></string-name>, <string-name><surname>Valle</surname> <given-names>J. W. F.</given-names></string-name>, and <string-name><surname>Schechter</surname> <given-names>J.</given-names></string-name></person-group>, <source>Phys. Rev. D</source> <volume>22</volume>, <fpage>738</fpage> (<year>1980</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.22.738">doi:10.1103/PhysRevD.22.738</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C45"><label>45</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Foot</surname> <given-names>R.</given-names></string-name>, <string-name><surname>Long</surname> <given-names>H. N.</given-names></string-name>, and <string-name><surname>Tran</surname> <given-names>T. A.</given-names></string-name></person-group>, <source>Phys. Rev. D</source> <volume>50</volume>, <fpage>R34</fpage> (<year>1994</year>) [<elocation-id content-type="arxiv">arXiv:hep-ph/9402243</elocation-id>[<comment><ext-link ext-link-type="uri" xlink:href="http://inspirehep.net/search?p=find+EPRINT+arXiv:hep-ph/9402243">Search inSPIRE</ext-link></comment>]. <comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.50.R34">doi:10.1103/PhysRevD.50.R34</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C46"><label>46</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Montero</surname> <given-names>J. C.</given-names></string-name>, <string-name><surname>Pisano</surname> <given-names>F.</given-names></string-name>, and <string-name><surname>Pleitez</surname> <given-names>V.</given-names></string-name></person-group>, <source>Phys. Rev. D</source> <volume>47</volume>, <fpage>2918</fpage> (<year>1993</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.47.2918">doi:10.1103/PhysRevD.47.2918</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C47"><label>47</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Long</surname> <given-names>H. N.</given-names></string-name></person-group>, <source>Phys. Rev. D</source> <volume>54</volume>, <fpage>4691</fpage> (<year>1996</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.54.4691">doi:10.1103/PhysRevD.54.4691</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C48"><label>48</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Long</surname> <given-names>H. N.</given-names></string-name></person-group>, <source>Phys. Rev. D</source> <volume>53</volume>, <fpage>437</fpage> (<year>1996</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.53.437">doi:10.1103/PhysRevD.53.437</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C49"><label>49</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Long</surname> <given-names>H. N.</given-names></string-name></person-group>, <source>Mod. Phys. Lett. A</source> <volume>13</volume>, <fpage>1865</fpage> (<year>1998</year>) [<elocation-id content-type="arxiv">arXiv:hep-ph/9711204</elocation-id>[<comment><ext-link ext-link-type="uri" xlink:href="http://inspirehep.net/search?p=find+EPRINT+arXiv:hep-ph/9711204">Search inSPIRE</ext-link></comment>]. <comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1142/S0217732398001959">doi:10.1142/S0217732398001959</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C50"><label>50</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Pisano</surname> <given-names>F.</given-names></string-name></person-group>, <source>Mod. Phys. Lett. A</source> <volume>11</volume>, <fpage>2639</fpage> (<year>1996</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1142/S0217732396002630">doi:10.1142/S0217732396002630</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C51"><label>51</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Doff</surname> <given-names>A.</given-names></string-name> and <string-name><surname>Pisano</surname> <given-names>F.</given-names></string-name></person-group>, <source>Mod. Phys. Lett. A</source> <volume>14</volume>, <fpage>1133</fpage> (<year>1999</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1142/S0217732399001218">doi:10.1142/S0217732399001218</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C52"><label>52</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>de S. Pires</surname> <given-names>C. A.</given-names></string-name> and <string-name><surname>Ravinez</surname> <given-names>O. P.</given-names></string-name></person-group>, <source>Phys. Rev. D</source> <volume>58</volume>, <fpage>035008</fpage> (<year>1998</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.58.035008">doi:10.1103/PhysRevD.58.035008</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C53"><label>53</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>de S. Pires</surname> <given-names>C. A.</given-names></string-name></person-group>, <source>Phys. Rev. D</source> <volume>60</volume>, <fpage>075013</fpage> (<year>1999</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.60.075013">doi:10.1103/PhysRevD.60.075013</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C54"><label>54</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Dong</surname> <given-names>P. V.</given-names></string-name> and <string-name><surname>Long</surname> <given-names>H. N.</given-names></string-name></person-group>, <source>Int. J. Mod. Phys. A</source> <volume>21</volume>, <fpage>6677</fpage> (<year>2006</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1142/S0217751X06035191">doi:10.1142/S0217751X06035191</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C55"><label>55</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Dong</surname> <given-names>P. V.</given-names></string-name>, <string-name><surname>Long</surname> <given-names>H. N.</given-names></string-name>, <string-name><surname>Nhung</surname> <given-names>D. T.</given-names></string-name>, and <string-name><surname>Soa</surname> <given-names>D. V.</given-names></string-name></person-group>, <source>Phys. Rev. D</source> <volume>73</volume>, <fpage>035004</fpage> (<year>2006</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.73.035004">doi:10.1103/PhysRevD.73.035004</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C56"><label>56</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Dong</surname> <given-names>P. V.</given-names></string-name> and <string-name><surname>Long</surname> <given-names>H. N.</given-names></string-name></person-group>, <source>Adv. High Energy Phys.</source> <volume>2008</volume>, <fpage>739492</fpage> (<year>2008</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1155/2008/739492">doi:10.1155/2008/739492</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C57"><label>57</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Ponce</surname> <given-names>W.</given-names></string-name>, <string-name><surname>Giraldo</surname> <given-names>Y.</given-names></string-name>, and <string-name><surname>Sanchez</surname> <given-names>L. A.</given-names></string-name></person-group>, <source>Phys. Rev. D</source> <volume>67</volume>, <fpage>075001</fpage> (<year>2003</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.67.075001">doi:10.1103/PhysRevD.67.075001</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C58"><label>58</label><mixed-citation publication-type="other"><person-group person-group-type="author"><string-name><surname>Huyen</surname> <given-names>V. T. N.</given-names></string-name>, <string-name><surname>Lam</surname> <given-names>T. T.</given-names></string-name>, <string-name><surname>Long</surname> <given-names>H. N.</given-names></string-name>, and <string-name><surname>Phong</surname> <given-names>V. Q.</given-names></string-name></person-group>, [<elocation-id content-type="arxiv">arXiv:1210.5833</elocation-id>] [<comment><ext-link ext-link-type="uri" xlink:href="http://inspirehep.net/search?p=find+EPRINT+arXiv:1210.5833">Search inSPIRE</ext-link></comment>]hep-ph.</mixed-citation></ref>
<ref id="PTV155C59"><label>59</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Dias</surname> <given-names>A. G.</given-names></string-name>, <string-name><surname>Martinez</surname> <given-names>R.</given-names></string-name>, and <string-name><surname>Pleitez</surname> <given-names>V.</given-names></string-name></person-group>, <source>Eur. Phys. J. C</source> <volume>39</volume>, <fpage>101</fpage> (<year>2005</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1140/epjc/s2004-02083-0">doi:10.1140/epjc/s2004-02083-0</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C60"><label>60</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Dias</surname> <given-names>A. G.</given-names></string-name> and <string-name><surname>Pleitez</surname> <given-names>V.</given-names></string-name></person-group>, <source>Phys. Rev. D</source> <volume>80</volume>, <fpage>056007</fpage> (<year>2009</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.80.056007">doi:10.1103/PhysRevD.80.056007</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C61"><label>61</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Buras</surname> <given-names>A. J.</given-names></string-name>, <string-name><surname>Fazio</surname> <given-names>F. D.</given-names></string-name>, <string-name><surname>Girrbach-Noe</surname> <given-names>J.</given-names></string-name>, and <string-name><surname>Carlucci</surname> <given-names>M. V.</given-names></string-name></person-group>, <source>J. High Energy Phys.</source> <volume>1402</volume>, <fpage>112</fpage> (<year>2014</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1007/JHEP02(2014)112">doi:10.1007/JHEP02(2014)112</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C62"><label>62</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Dong</surname> <given-names>P. V.</given-names></string-name> and <string-name><surname>Si</surname> <given-names>D. T.</given-names></string-name></person-group>, <source>Phys. Rev. D</source> <volume>90</volume>, <fpage>117703</fpage> (<year>2014</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.90.117703">doi:10.1103/PhysRevD.90.117703</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C63"><label>63</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Peskin</surname> <given-names>M. E.</given-names></string-name> and <string-name><surname>Takeuchi</surname> <given-names>T.</given-names></string-name></person-group>, <source>Phys. Rev. Lett.</source> <volume>65</volume>, <fpage>964</fpage> (<year>1990</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevLett.65.964">doi:10.1103/PhysRevLett.65.964</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C64"><label>64</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Peskin</surname> <given-names>M. E.</given-names></string-name> and <string-name><surname>Takeuchi</surname> <given-names>T.</given-names></string-name></person-group>, <source>Phys. Rev. D</source> <volume>46</volume>, <fpage>381</fpage> (<year>1992</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.46.381">doi:10.1103/PhysRevD.46.381</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C65"><label>65</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Drees</surname> <given-names>M.</given-names></string-name> and <string-name><surname>Hagiwara</surname> <given-names>K.</given-names></string-name></person-group>, <source>Phys. Rev. D</source> <volume>42</volume>, <fpage>1709</fpage> (<year>1990</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.42.1709">doi:10.1103/PhysRevD.42.1709</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C66"><label>66</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Montero</surname> <given-names>J. C.</given-names></string-name>, <string-name><surname>de S. Pires</surname> <given-names>C. A.</given-names></string-name>, and <string-name><surname>Pleitez</surname> <given-names>V.</given-names></string-name></person-group>, <source>Phys. Rev. D</source> <volume>66</volume>, <fpage>113003</fpage> (<year>2002</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.66.113003">doi:10.1103/PhysRevD.66.113003</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C67"><label>67</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Maekawa</surname> <given-names>C. M.</given-names></string-name> and <string-name><surname>Rodriguez</surname> <given-names>M. C.</given-names></string-name></person-group>, <source>J. High Energy Phys.</source> <volume>0604</volume>, <fpage>031</fpage> (<year>2006</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1088/1126-6708/2006/04/031">doi:10.1088/1126-6708/2006/04/031</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C68"><label>68</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Montero</surname> <given-names>J. C.</given-names></string-name>, <string-name><surname>Pleitez</surname> <given-names>V.</given-names></string-name>, and <string-name><surname>Rodriguez</surname> <given-names>M. C.</given-names></string-name></person-group>, <source>Phys. Rev. D</source> <volume>65</volume>, <fpage>095008</fpage> (<year>2002</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.65.095008">doi:10.1103/PhysRevD.65.095008</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C69"><label>69</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Dong</surname> <given-names>P. V.</given-names></string-name>, <string-name><surname>Huong</surname> <given-names>D. T.</given-names></string-name>, <string-name><surname>Rodriguez</surname> <given-names>M. C.</given-names></string-name>, and <string-name><surname>Long</surname> <given-names>H. N.</given-names></string-name></person-group>, <source>Nucl. Phys. B</source> <volume>772</volume>, <fpage>150</fpage> (<year>2007</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1016/j.nuclphysb.2007.03.003">doi:10.1016/j.nuclphysb.2007.03.003</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C70"><label>70</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Dong</surname> <given-names>P. V.</given-names></string-name>, <string-name><surname>Huong</surname> <given-names>Tr.T.</given-names></string-name>, <string-name><surname>Thuy</surname> <given-names>N. T.</given-names></string-name>, and <string-name><surname>Long</surname> <given-names>H. N.</given-names></string-name></person-group>, <source>J. High Energy Phys.</source> <volume>0711</volume>, <fpage>073</fpage> (<year>2007</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1088/1126-6708/2007/11/073">doi:10.1088/1126-6708/2007/11/073</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C71"><label>71</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Dong</surname> <given-names>P. V.</given-names></string-name>, <string-name><surname>Huong</surname> <given-names>D. T.</given-names></string-name>, <string-name><surname>Thuy</surname> <given-names>N. T.</given-names></string-name>, and <string-name><surname>Long</surname> <given-names>H. N.</given-names></string-name></person-group>, <source>Nucl. Phys. B</source> <volume>795</volume>, <fpage>361</fpage> (<year>2008</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1016/j.nuclphysb.2007.11.035">doi:10.1016/j.nuclphysb.2007.11.035</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C72"><label>72</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Huong</surname> <given-names>D. T.</given-names></string-name> and <string-name><surname>Long</surname> <given-names>H. N.</given-names></string-name></person-group>, <source>J. High Energy Phys.</source> <volume>0807</volume>, <fpage>049</fpage> (<year>2008</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1088/1126-6708/2008/07/049">doi:10.1088/1126-6708/2008/07/049</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C73"><label>73</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Ng</surname> <given-names>D.</given-names></string-name></person-group>, <source>Phys. Rev. D</source> <volume>49</volume>, <fpage>4805</fpage> (<year>1994</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.49.4805">doi:10.1103/PhysRevD.49.4805</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C74"><label>74</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Cogollo</surname> <given-names>D.</given-names></string-name>, <string-name><surname>Queiroz</surname> <given-names>F. S.</given-names></string-name>, and <string-name><surname>Vasconcelos</surname> <given-names>P.</given-names></string-name></person-group>, <source>Mod. Phys. Lett. A</source> <volume>29</volume>, <fpage>1450173</fpage> (<year>2014</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1142/S0217732314501739">doi:10.1142/S0217732314501739</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C75"><label>75</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Kelso</surname> <given-names>C.</given-names></string-name>, <string-name><surname>Pinheiro</surname> <given-names>P. R. D.</given-names></string-name>, <string-name><surname>Queiroz</surname> <given-names>F. S.</given-names></string-name>, and <string-name><surname>Shepherd</surname> <given-names>W.</given-names></string-name></person-group>, <source>Eur. Phys. J. C</source> <volume>74</volume>, <fpage>2808</fpage> (<year>2014</year>) [<elocation-id content-type="arxiv">arXiv:1312.0051</elocation-id>] [<comment><ext-link ext-link-type="uri" xlink:href="http://inspirehep.net/search?p=find+EPRINT+arXiv:1312.0051">Search inSPIRE</ext-link></comment>]hep-ph. <comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1140/epjc/s10052-014-2808-4">doi:10.1140/epjc/s10052-014-2808-4</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C76"><label>76</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Dumm</surname> <given-names>D. G.</given-names></string-name>, <string-name><surname>Pisano</surname> <given-names>F.</given-names></string-name>, and <string-name><surname>Pleitez</surname> <given-names>V.</given-names></string-name></person-group>, <source>Mod. Phys. Lett. A</source> <volume>09</volume>, <fpage>1609</fpage> (<year>1994</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1142/S0217732394001441">doi:10.1142/S0217732394001441</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C77"><label>77</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Long</surname> <given-names>H. N.</given-names></string-name> and <string-name><surname>Van</surname> <given-names>V. T.</given-names></string-name></person-group>, <source>J. Phys. G</source> <volume>25</volume>, <fpage>2319</fpage> (<year>1999</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1088/0954-3899/25/12/302">doi:10.1088/0954-3899/25/12/302</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C78"><label>78</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Machado</surname> <given-names>A. C.</given-names></string-name>, <string-name><surname>Montero</surname> <given-names>J. C.</given-names></string-name>, and <string-name><surname>Pleitez</surname> <given-names>V.</given-names></string-name></person-group>, <source>Phys. Rev. D</source> <volume>88</volume>, <fpage>113002</fpage> (<year>2013</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.88.113002">doi:10.1103/PhysRevD.88.113002</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C79"><label>79</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Frampton</surname> <given-names>P. H.</given-names></string-name> and <string-name><surname>Harada</surname> <given-names>M.</given-names></string-name></person-group>, <source>Phys. Rev. D</source> <volume>58</volume>, <fpage>095013</fpage> (<year>1998</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.58.095013">doi:10.1103/PhysRevD.58.095013</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C80"><label>80</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Long</surname> <given-names>H. N.</given-names></string-name> and <string-name><surname>Inami</surname> <given-names>T.</given-names></string-name></person-group>, <source>Phys. Rev. D</source> <volume>61</volume>, <fpage>075002</fpage> (<year>2000</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.61.075002">doi:10.1103/PhysRevD.61.075002</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C81"><label>81</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Olive</surname> <given-names>K. A.</given-names></string-name></person-group> et al. <source>[Particle Data Group], Chin. Phys. C</source> <volume>38</volume>, <fpage>090001</fpage> (<year>2014</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1088/1674-1137/38/9/090001">doi:10.1088/1674-1137/38/9/090001</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C82"><label>82</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Djouadi</surname> <given-names>A.</given-names></string-name></person-group>, <source>Phys. Rept.</source> <volume>459</volume>, <fpage>1</fpage> (<year>2008</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1016/j.physrep.2007.10.005">doi:10.1016/j.physrep.2007.10.005</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C83"><label>83</label><mixed-citation publication-type="journal"><collab>LHCb Collaboration</collab>, <source>Phys. Rev. Lett.</source> <volume>111</volume>, <fpage>191801</fpage> (<year>2013</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevLett.111.191801">doi:10.1103/PhysRevLett.111.191801</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C84"><label>84</label><mixed-citation publication-type="other"><person-group person-group-type="author"><string-name><surname>Richard</surname> <given-names>F.</given-names></string-name></person-group>, [<elocation-id content-type="arxiv">arXiv:1312.2467</elocation-id>] [<comment><ext-link ext-link-type="uri" xlink:href="http://inspirehep.net/search?p=find+EPRINT+arXiv:1312.2467">Search inSPIRE</ext-link></comment>]hep-ph.</mixed-citation></ref>
<ref id="PTV155C85"><label>85</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Gauld</surname> <given-names>R.</given-names></string-name>, <string-name><surname>Goertz</surname> <given-names>F.</given-names></string-name>, and <string-name><surname>Haisch</surname> <given-names>U.</given-names></string-name></person-group>, <source>J. High Energy Phys.</source> <volume>1401</volume>, <fpage>069</fpage> (<year>2014</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1007/JHEP01(2014)069">doi:10.1007/JHEP01(2014)069</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C86"><label>86</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Rodriguez</surname> <given-names>M. C.</given-names></string-name></person-group>, <source>J. Mod. Phys.</source> <volume>2</volume>, <fpage>1193</fpage> (<year>2011</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.4236/jmp.2011.210149">doi:10.4236/jmp.2011.210149</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C87"><label>87</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Girardello</surname> <given-names>L.</given-names></string-name> and <string-name><surname>Grisaru</surname> <given-names>M. T.</given-names></string-name></person-group>, <source>Nucl. Phys. B</source> <volume>194</volume>, <fpage>65</fpage> (<year>1982</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1016/0550-3213(82)90512-0">doi:10.1016/0550-3213(82)90512-0</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C88"><label>88</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Barate</surname> <given-names>R.</given-names></string-name></person-group> et al. [<collab>LEP Working Group for Higgs boson searches and ALEPH, DELPHI, L3, and OPAL Collaborations</collab>], <source>Phys. Lett. B</source> <volume>565</volume>, <fpage>61</fpage> (<year>2003</year>) [<elocation-id content-type="arxiv">arXiv:hep-ex/0306033</elocation-id>[<comment><ext-link ext-link-type="uri" xlink:href="http://inspirehep.net/search?p=find+EPRINT+arXiv:hep-ex/0306033">Search inSPIRE</ext-link></comment>]. <comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1016/S0370-2693(03)00614-2">doi:10.1016/S0370-2693(03)00614-2</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C89"><label>89</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Dutta</surname> <given-names>B.</given-names></string-name>, <string-name><surname>Eusebi</surname> <given-names>R.</given-names></string-name>, <string-name><surname>Gao</surname> <given-names>Y.</given-names></string-name>, <string-name><surname>Ghosh</surname> <given-names>T.</given-names></string-name>, and <string-name><surname>Kamon</surname> <given-names>T.</given-names></string-name></person-group>, <source>Phys. Rev. D</source> <volume>90</volume>, <fpage>055015</fpage> (<year>2014</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.90.055015">doi:10.1103/PhysRevD.90.055015</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C90"><label>90</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Bambhaniya</surname> <given-names>G.</given-names></string-name>, <string-name><surname>Chakrabortty</surname> <given-names>J.</given-names></string-name>, <string-name><surname>Gluza</surname> <given-names>J.</given-names></string-name>, <string-name><surname>Kordiaczy&#x0144;ska</surname> <given-names>M.</given-names></string-name>, and <string-name><surname>Szafron</surname> <given-names>R.</given-names></string-name></person-group>, <source>J. High Energy Phys.</source> <volume>1405</volume>, <fpage>033</fpage> (<year>2014</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1007/JHEP05(2014)033">doi:10.1007/JHEP05(2014)033</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C91"><label>91</label><mixed-citation publication-type="other"><person-group person-group-type="author"><string-name><surname>Flechl</surname> <given-names>M.</given-names></string-name></person-group>, [<elocation-id content-type="arxiv">arXiv:1503.00632</elocation-id>] [<comment><ext-link ext-link-type="uri" xlink:href="http://inspirehep.net/search?p=find+EPRINT+arXiv:1503.00632">Search inSPIRE</ext-link></comment>]hep-ex.</mixed-citation></ref>
<ref id="PTV155C92"><label>92</label><mixed-citation publication-type="journal"><collab>ATLAS Collaboration</collab>, <source>Phys. Rev. D</source> <volume>90</volume>, <fpage>112015</fpage> (<year>2014</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.90.112015">doi:10.1103/PhysRevD.90.112015</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C93"><label>93</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Caetano</surname> <given-names>W.</given-names></string-name>, <string-name><surname>de S. Pires</surname> <given-names>C. A.</given-names></string-name>, <string-name><surname>da Silva</surname> <given-names>P. S. R.</given-names></string-name>, <string-name><surname>Cogollo</surname> <given-names>D.</given-names></string-name>, and <string-name><surname>Queiroz</surname> <given-names>F. S.</given-names></string-name></person-group>, <source>Eur. Phys. J. C</source> <volume>73</volume>, <fpage>2607</fpage> (<year>2013</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1140/epjc/s10052-013-2607-3">doi:10.1140/epjc/s10052-013-2607-3</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C94"><label>94</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Djouadi</surname> <given-names>A.</given-names></string-name></person-group>, <source>Phys. Rept.</source> <volume>457</volume>, <fpage>1</fpage> (<year>2008</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1016/j.physrep.2007.10.004">doi:10.1016/j.physrep.2007.10.004</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C95"><label>95</label><mixed-citation publication-type="other"><person-group person-group-type="author"><string-name><surname>Krau&#x00DF;</surname> <given-names>M.</given-names></string-name></person-group>, <comment>LHC phenomenology of a <inline-formula><tex-math notation="LaTeX" id="ImEquation924"><![CDATA[$Z'$]]></tex-math></inline-formula> decaying into supersymmetric particles, <italic>Master Thesis</italic>, University of W&#x00FC;rzburg</comment> (<year>2012</year>).</mixed-citation></ref>
<ref id="PTV155C96"><label>96</label><mixed-citation publication-type="journal"><person-group person-group-type="author"><string-name><surname>Dreiner</surname> <given-names>H. K.</given-names></string-name>, <string-name><surname>Haber</surname> <given-names>H. E.</given-names></string-name>, and <string-name><surname>Martin</surname> <given-names>S. P.</given-names></string-name></person-group>, <source>Phys. Rept.</source> <volume>494</volume>, <fpage>1</fpage> (<year>2010</year>).
<comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1016/j.physrep.2010.05.002">doi:10.1016/j.physrep.2010.05.002</ext-link>)</comment></mixed-citation></ref>
<ref id="PTV155C97"><label>97</label><mixed-citation publication-type="other"><person-group person-group-type="author"><string-name><surname>Martin</surname> <given-names>S. P.</given-names>, &#x201C;Phenomenology of Particle Physics&#x201D;</string-name></person-group>, <comment>NIU Spring 2002 PHYS586 Lecture Notes, the online version: <uri xlink:href="http://www.niu.edu/spmartin/phys686/">http://www.niu.edu/spmartin/phys686/</uri></comment>.</mixed-citation></ref>
</ref-list>
</back>
</article>
