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<front>
<journal-meta>
<journal-id journal-id-type="publisher-id">ptep</journal-id>
<journal-id journal-id-type="hwp">ptep</journal-id>
<journal-title>Progress of Theoretical and Experimental Physics</journal-title>
<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/ptv038</article-id>
<article-id pub-id-type="publisher-id">ptv038</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>B62</subject>
<subject>B69</subject>
<subject>D32</subject>
</subj-group>
</article-categories>
<title-group>
<article-title>Hidden-charm decays of <italic>X</italic>(3915) and <italic>Z</italic>(3930) as the P-wave charmonia</article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name><surname>Chen</surname><given-names>Dian-Yong</given-names></name>
<xref ref-type="aff" rid="af1">1</xref>
<xref ref-type="aff" rid="af2">2</xref>
<xref ref-type="corresp" rid="cor1">&ast;</xref>
</contrib>
<contrib contrib-type="author">
<name><surname>Liu</surname><given-names>Xiang</given-names></name>
<xref ref-type="aff" rid="af2">2</xref>
<xref ref-type="aff" rid="af3">3</xref>
<xref ref-type="corresp" rid="cor1">&ast;</xref>
</contrib>
<contrib contrib-type="author">
<name><surname>Matsuki</surname><given-names>Takayuki</given-names></name>
<xref ref-type="aff" rid="af4">4</xref>
<xref ref-type="aff" rid="af5">5</xref>
<xref ref-type="corresp" rid="cor1">&ast;</xref>
</contrib>
<aff id="af1"><label>1</label><addr-line>Nuclear Theory Group, Institute of Modern Physics, Chinese Academy of Sciences, Lanzhou 730000, China</addr-line></aff>
<aff id="af2"><label>2</label><addr-line>Research Center for Hadron and CSR Physics, Lanzhou University <inline-formula><tex-math notation="LaTeX" id="ImEquation3"><![CDATA[$\&$]]></tex-math></inline-formula> Institute of Modern Physics of CAS, Lanzhou 730000, China</addr-line></aff>
<aff id="af3"><label>3</label><addr-line>School of Physical Science and Technology, Lanzhou University, Lanzhou 730000, China</addr-line></aff>
<aff id="af4"><label>4</label><addr-line>Tokyo Kasei University, 1-18-1 Kaga, Itabashi, Tokyo 173-8602, Japan</addr-line></aff>
<aff id="af5"><label>5</label><addr-line>Theoretical Research Division, Nishina Center, RIKEN, Saitama 351-0198, Japan</addr-line></aff>
</contrib-group>
<author-notes>
<corresp id="cor1"><label>&ast;</label>E-mail: <email>chendy@impcas.ac.cn</email>, <email>xiangliu@lzu.edu.cn</email>, <email>matsuki@tokyo-kasei.ac.jp</email></corresp>
</author-notes>
<pub-date pub-type="ppub"><month>04</month><year>2015</year></pub-date>
<pub-date pub-type="epub"><day>07</day><month>04</month><year>2015</year></pub-date>
<volume>2015</volume>
<issue>4</issue>
<elocation-id>043B05</elocation-id>
<history>
<date date-type="received"><day>11</day><month>8</month><year>2014</year></date>
<date date-type="rev-recd"><day>19</day><month>2</month><year>2015</year></date>
<date date-type="accepted"><day>21</day><month>2</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/"><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 use, distribution, and reproduction in any medium, provided the original work is properly cited.</p>
<p>Funded by SCOAP<sup>3</sup></p></license>
</permissions>
<self-uri content-type="pdf" xlink:href="ptv038.pdf"/>
<abstract>
<p>In this work, we investigate the <inline-formula><tex-math notation="LaTeX" id="ImEquation4"><![CDATA[$X(3915)$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation5"><![CDATA[$Z(3930)$]]></tex-math></inline-formula> decays into <inline-formula><tex-math notation="LaTeX" id="ImEquation6"><![CDATA[$J/\psi \omega$]]></tex-math></inline-formula> with the <inline-formula><tex-math notation="LaTeX" id="ImEquation7"><![CDATA[$\chi _{c0}^\prime (2P)$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation8"><![CDATA[$\chi _{c2}^\prime (2P)$]]></tex-math></inline-formula> assignments to <inline-formula><tex-math notation="LaTeX" id="ImEquation9"><![CDATA[$X(3915)$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation10"><![CDATA[$Z(3930)$]]></tex-math></inline-formula>, respectively. The results show that the decay width of <inline-formula><tex-math notation="LaTeX" id="ImEquation11"><![CDATA[$Z(3930)\to J/\psi \omega$]]></tex-math></inline-formula> is at least one order smaller than that of <inline-formula><tex-math notation="LaTeX" id="ImEquation12"><![CDATA[$X(3915)\to J/\psi \omega$]]></tex-math></inline-formula>. This observation explains why only one structure, <inline-formula><tex-math notation="LaTeX" id="ImEquation13"><![CDATA[$X(3915)$]]></tex-math></inline-formula>, has been observed in the <inline-formula><tex-math notation="LaTeX" id="ImEquation14"><![CDATA[$J/\psi \omega$]]></tex-math></inline-formula> invariant mass spectrum for the process <inline-formula><tex-math notation="LaTeX" id="ImEquation15"><![CDATA[$\gamma \gamma \to J/\psi \omega$]]></tex-math></inline-formula>.</p>
</abstract>
<kwd-group kwd-group-type="jel">
<title>Subject Index</title>
<kwd>B62</kwd>
<kwd>B69</kwd>
<kwd>D32</kwd>
</kwd-group>
<counts><page-count count="8"/></counts>
<custom-meta-wrap>
<custom-meta>
<meta-name>arxiv-id</meta-name>
<meta-value>arXiv:1311.6274</meta-value>
</custom-meta>
</custom-meta-wrap>
</article-meta>
</front>
<body>
<sec id="s1"><title/>
<p>The <inline-formula><tex-math notation="LaTeX" id="ImEquation16"><![CDATA[$\gamma \gamma$]]></tex-math></inline-formula> fusion process is an ideal platform to produce charmonium-like states. In the past, the Belle and BaBar experiments have reported many charmonium-like states in the <inline-formula><tex-math notation="LaTeX" id="ImEquation17"><![CDATA[$\gamma \gamma$]]></tex-math></inline-formula> fusion processes. Among these observations, <inline-formula><tex-math notation="LaTeX" id="ImEquation18"><![CDATA[$X(3915)$]]></tex-math></inline-formula> has mass <inline-formula><tex-math notation="LaTeX" id="ImEquation19"><![CDATA[$M_{X(3915)} = (3915\pm 3({\rm stat.})\pm 2({\rm syst.}))$]]></tex-math></inline-formula> MeV and width <inline-formula><tex-math notation="LaTeX" id="ImEquation20"><![CDATA[$\Gamma _{X(3915)}=(17\pm 10({\rm stat.})\pm 3({\rm syst.}))$]]></tex-math></inline-formula> MeV. Since <inline-formula><tex-math notation="LaTeX" id="ImEquation21"><![CDATA[$X(3915)$]]></tex-math></inline-formula> was observed in the <inline-formula><tex-math notation="LaTeX" id="ImEquation22"><![CDATA[$J/\psi \omega$]]></tex-math></inline-formula> invariant mass spectrum of <inline-formula><tex-math notation="LaTeX" id="ImEquation23"><![CDATA[$\gamma \gamma \to J/\psi \omega$]]></tex-math></inline-formula>, the possible quantum number should be <inline-formula><tex-math notation="LaTeX" id="ImEquation24"><![CDATA[$J^{PC}=0^{+ + }$]]></tex-math></inline-formula> or <inline-formula><tex-math notation="LaTeX" id="ImEquation25"><![CDATA[$J^{PC}=2^{+ + }$]]></tex-math></inline-formula>, which results in the corresponding Belle measurement of <inline-formula><tex-math notation="LaTeX" id="ImEquation26"><![CDATA[$\Gamma _{X(3915)\to \gamma \gamma }{\cdot } BR(X(3915)\to J/\psi \omega ) = (61\pm 17({\rm stat.})\pm 8({\rm syst.}))$]]></tex-math></inline-formula> eV or <inline-formula><tex-math notation="LaTeX" id="ImEquation27"><![CDATA[$(18\pm 5({\rm stat.})\pm 2({\rm syst.}))$]]></tex-math></inline-formula> eV [<xref ref-type="bibr" rid="C1">1</xref>]. As a candidate for charmonium <inline-formula><tex-math notation="LaTeX" id="ImEquation28"><![CDATA[$\chi _{c2}^\prime (2P)$]]></tex-math></inline-formula> (<inline-formula><tex-math notation="LaTeX" id="ImEquation29"><![CDATA[$n^{2s+1}L_J=2^3P_2$]]></tex-math></inline-formula>), <inline-formula><tex-math notation="LaTeX" id="ImEquation30"><![CDATA[$Z(3930)$]]></tex-math></inline-formula> was first observed in the process <inline-formula><tex-math notation="LaTeX" id="ImEquation31"><![CDATA[$\gamma \gamma \to D\bar {D}$]]></tex-math></inline-formula> [<xref ref-type="bibr" rid="C2">2</xref>]. The experimental information on <inline-formula><tex-math notation="LaTeX" id="ImEquation32"><![CDATA[$Z(3930)$]]></tex-math></inline-formula> gives <inline-formula><tex-math notation="LaTeX" id="ImEquation33"><![CDATA[$M_{Z(3930)}=3929\pm ({\rm stat.})5\pm 2({\rm syst.})$]]></tex-math></inline-formula> MeV, <inline-formula><tex-math notation="LaTeX" id="ImEquation34"><![CDATA[$\Gamma _{Z(3930)}=29\pm 10({\rm stat.})\pm 2({\rm syst.})$]]></tex-math></inline-formula> MeV, and <inline-formula><tex-math notation="LaTeX" id="ImEquation35"><![CDATA[$\Gamma _{Z(3930)\to \gamma \gamma }{\cdot } BR(Z(3930)\to D\bar {D})=0.18\pm 0.05({\rm stat.})\pm 0.03({\rm syst.})$]]></tex-math></inline-formula> keV [<xref ref-type="bibr" rid="C2">2</xref>]. Later, the BaBar Collaboration also confirmed the observation of <inline-formula><tex-math notation="LaTeX" id="ImEquation36"><![CDATA[$Z(3930)$]]></tex-math></inline-formula> in <inline-formula><tex-math notation="LaTeX" id="ImEquation37"><![CDATA[$\gamma \gamma \to D\bar {D}$]]></tex-math></inline-formula> [<xref ref-type="bibr" rid="C3">3</xref>].</p>
<p>In Ref. [<xref ref-type="bibr" rid="C4">4</xref>], the assignments of <inline-formula><tex-math notation="LaTeX" id="ImEquation38"><![CDATA[$X(3915)$]]></tex-math></inline-formula> or <inline-formula><tex-math notation="LaTeX" id="ImEquation39"><![CDATA[$Z(3930)$]]></tex-math></inline-formula> as <inline-formula><tex-math notation="LaTeX" id="ImEquation40"><![CDATA[$\chi _{c0}^\prime (2P)$]]></tex-math></inline-formula> or <inline-formula><tex-math notation="LaTeX" id="ImEquation41"><![CDATA[$\chi _{c2}^\prime (2P)$]]></tex-math></inline-formula> charmonium states were proposed by analyzing the mass spectrum and calculating the strong decay of P-wave charmonium. Later, in Ref. [<xref ref-type="bibr" rid="C5">5</xref>], the BaBar Collaboration announced that the charmonium-like state <inline-formula><tex-math notation="LaTeX" id="ImEquation42"><![CDATA[$X(3915)$]]></tex-math></inline-formula> had been confirmed in the <inline-formula><tex-math notation="LaTeX" id="ImEquation43"><![CDATA[$\gamma \gamma \to J/\psi$]]></tex-math></inline-formula> process with a spin-parity <inline-formula><tex-math notation="LaTeX" id="ImEquation44"><![CDATA[$J^P=0^+ $]]></tex-math></inline-formula> [<xref ref-type="bibr" rid="C5">5</xref>], which is consistent with the prediction in Ref. [<xref ref-type="bibr" rid="C4">4</xref>].</p>
<p>If <inline-formula><tex-math notation="LaTeX" id="ImEquation45"><![CDATA[$Z(3930)$]]></tex-math></inline-formula> is a <inline-formula><tex-math notation="LaTeX" id="ImEquation46"><![CDATA[$\chi _{c2}^\prime (2P)$]]></tex-math></inline-formula> state, <inline-formula><tex-math notation="LaTeX" id="ImEquation47"><![CDATA[$Z(3930)$]]></tex-math></inline-formula> theoretically has the hidden-charm decay channel <inline-formula><tex-math notation="LaTeX" id="ImEquation48"><![CDATA[$J/\psi \omega$]]></tex-math></inline-formula> besides its observed open-charm decay <inline-formula><tex-math notation="LaTeX" id="ImEquation49"><![CDATA[$D\bar {D}$]]></tex-math></inline-formula>. Hence, the signal of <inline-formula><tex-math notation="LaTeX" id="ImEquation50"><![CDATA[$Z(3930)$]]></tex-math></inline-formula> should appear in the same <inline-formula><tex-math notation="LaTeX" id="ImEquation51"><![CDATA[$J/\psi \omega$]]></tex-math></inline-formula> invariant mass spectrum as <inline-formula><tex-math notation="LaTeX" id="ImEquation52"><![CDATA[$X(3915)$]]></tex-math></inline-formula>, which was observed by Belle [<xref ref-type="bibr" rid="C1">1</xref>]. However, the experimental data for the <inline-formula><tex-math notation="LaTeX" id="ImEquation53"><![CDATA[$J/\psi \omega$]]></tex-math></inline-formula> invariant mass spectrum show no evidence of <inline-formula><tex-math notation="LaTeX" id="ImEquation54"><![CDATA[$Z(3930)$]]></tex-math></inline-formula>. This fact urges us to explain why there only exists one signal, <inline-formula><tex-math notation="LaTeX" id="ImEquation55"><![CDATA[$X(3915)$]]></tex-math></inline-formula>, observed in the process <inline-formula><tex-math notation="LaTeX" id="ImEquation56"><![CDATA[$\gamma \gamma \to J/\psi \omega$]]></tex-math></inline-formula>.</p>
<p>In this work, we dedicate ourselves to studying the <inline-formula><tex-math notation="LaTeX" id="ImEquation57"><![CDATA[$X(3915)$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation58"><![CDATA[$Z(3930)$]]></tex-math></inline-formula> decays into <inline-formula><tex-math notation="LaTeX" id="ImEquation59"><![CDATA[$J/\psi \omega$]]></tex-math></inline-formula> under the <inline-formula><tex-math notation="LaTeX" id="ImEquation60"><![CDATA[$\chi _{c0}^\prime (2P)$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation61"><![CDATA[$\chi _{c2}^\prime (2P)$]]></tex-math></inline-formula> assignments to <inline-formula><tex-math notation="LaTeX" id="ImEquation62"><![CDATA[$X(3915)$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation63"><![CDATA[$Z(3930)$]]></tex-math></inline-formula>, respectively. By this study, we wan to answer whether the decay <inline-formula><tex-math notation="LaTeX" id="ImEquation64"><![CDATA[$Z(3930)\to J/\psi \omega$]]></tex-math></inline-formula> is suppressed compared with <inline-formula><tex-math notation="LaTeX" id="ImEquation65"><![CDATA[$X(3915)\to J/\psi \omega$]]></tex-math></inline-formula> under the P-wave charmonium assignments to <inline-formula><tex-math notation="LaTeX" id="ImEquation66"><![CDATA[$X(3915)$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation67"><![CDATA[$Z(3930)$]]></tex-math></inline-formula>, which can shed light on the above puzzle.</p>
<p>As higher charmonia, the <inline-formula><tex-math notation="LaTeX" id="ImEquation68"><![CDATA[$X(3915)$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation69"><![CDATA[$Z(3930)$]]></tex-math></inline-formula> decays into <inline-formula><tex-math notation="LaTeX" id="ImEquation70"><![CDATA[$J/\psi \omega$]]></tex-math></inline-formula> occur via hadronic loop effects with the open-charm decay channels as the intermediate state. This mechanism has been studied in Refs. [<xref ref-type="bibr" rid="C6">6</xref>&#x02013;<xref ref-type="bibr" rid="C13">13</xref>] when calculating the hidden-charm and open-charm decays of charmonium and other charmonium-like states.</p>
<p>The <inline-formula><tex-math notation="LaTeX" id="ImEquation71"><![CDATA[$X(3915)$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation72"><![CDATA[$Z(3930)$]]></tex-math></inline-formula> under discussion are candidates for the first radial excitations of <inline-formula><tex-math notation="LaTeX" id="ImEquation73"><![CDATA[$\chi _{c0}$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation74"><![CDATA[$\chi _{c2}$]]></tex-math></inline-formula>, respectively. Since the masses of <inline-formula><tex-math notation="LaTeX" id="ImEquation75"><![CDATA[$X(3915)$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation76"><![CDATA[$Z(3930)$]]></tex-math></inline-formula> are above the thresholds of <inline-formula><tex-math notation="LaTeX" id="ImEquation77"><![CDATA[$D\bar {D}$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation78"><![CDATA[$D\bar {D}^{\ast }$]]></tex-math></inline-formula> and below the <inline-formula><tex-math notation="LaTeX" id="ImEquation79"><![CDATA[$D^{\ast }\bar {D}^{\ast }$]]></tex-math></inline-formula> threshold, <inline-formula><tex-math notation="LaTeX" id="ImEquation80"><![CDATA[$X(3915)$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation81"><![CDATA[$Z(3930)$]]></tex-math></inline-formula> dominantly decay into <inline-formula><tex-math notation="LaTeX" id="ImEquation82"><![CDATA[$D\bar {D}$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation83"><![CDATA[$D\bar {D}^{\ast }$]]></tex-math></inline-formula>, which contribute to the total widths of <inline-formula><tex-math notation="LaTeX" id="ImEquation84"><![CDATA[$X(3915)$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation85"><![CDATA[$Z(3930)$]]></tex-math></inline-formula> (see Ref. [<xref ref-type="bibr" rid="C4">4</xref>] for more details). As the subordinate decay mode, <inline-formula><tex-math notation="LaTeX" id="ImEquation86"><![CDATA[$J/\psi \omega$]]></tex-math></inline-formula> is assumed from the rescattering contribution of the dominant decays <inline-formula><tex-math notation="LaTeX" id="ImEquation87"><![CDATA[$X(3915)/Z(3930)\to D\bar {D}, D\bar {D}^{\ast }$]]></tex-math></inline-formula>, which is the reason why we only consider the intermediate <inline-formula><tex-math notation="LaTeX" id="ImEquation88"><![CDATA[$D\bar {D}$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation89"><![CDATA[$D\bar {D}^{\ast }$]]></tex-math></inline-formula> contributions in this work. Under the <inline-formula><tex-math notation="LaTeX" id="ImEquation90"><![CDATA[$\chi _{c0}^\prime (2P)$]]></tex-math></inline-formula> assignment to <inline-formula><tex-math notation="LaTeX" id="ImEquation91"><![CDATA[$X(3915)$]]></tex-math></inline-formula>, the hidden-charm decay <inline-formula><tex-math notation="LaTeX" id="ImEquation92"><![CDATA[$X(3915)\to J/\psi \omega$]]></tex-math></inline-formula> occurs through the intermediate states <inline-formula><tex-math notation="LaTeX" id="ImEquation93"><![CDATA[$D\bar {D}$]]></tex-math></inline-formula> since <inline-formula><tex-math notation="LaTeX" id="ImEquation94"><![CDATA[$X(3915)$]]></tex-math></inline-formula> with <inline-formula><tex-math notation="LaTeX" id="ImEquation95"><![CDATA[$J^{PC}=0^{+ + }$]]></tex-math></inline-formula> dominantly decays into <inline-formula><tex-math notation="LaTeX" id="ImEquation96"><![CDATA[$D\bar {D}$]]></tex-math></inline-formula>, as indicated in Ref. [<xref ref-type="bibr" rid="C4">4</xref>]. The hadron level descriptions of <inline-formula><tex-math notation="LaTeX" id="ImEquation97"><![CDATA[$X(3915)\to D\bar {D}\to J/\psi \omega$]]></tex-math></inline-formula> are shown in Fig. <xref ref-type="fig" rid="F1">1</xref>(a). The expression for the decay amplitude of the hidden-charm decay <inline-formula><tex-math notation="LaTeX" id="ImEquation98"><![CDATA[$X(3915)\to D\bar {D}\to J/\psi \omega$]]></tex-math></inline-formula> reads
<disp-formula id="M1"><label>(1)</label><tex-math notation="LaTeX" id="DmEquation1"><![CDATA[\[\mathcal {M}[X(3915)\to J/\psi \omega ]=4 \left [ \mathcal {A}_{\rm (a)}^{D} + \mathcal {A}_{\rm (b)}^{D^\ast }\right ] .\]]]></tex-math></disp-formula>
As the <inline-formula><tex-math notation="LaTeX" id="ImEquation99"><![CDATA[$\chi _{c2}^\prime (2P)$]]></tex-math></inline-formula> state, <inline-formula><tex-math notation="LaTeX" id="ImEquation100"><![CDATA[$Z(3930)$]]></tex-math></inline-formula> mainly decays into <inline-formula><tex-math notation="LaTeX" id="ImEquation101"><![CDATA[$D\bar {D}$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation102"><![CDATA[$D\bar {D}^{\ast } + \hbox {h.c.}$]]></tex-math></inline-formula> [<xref ref-type="bibr" rid="C4">4</xref>]. Thus, its hidden-charm decay <inline-formula><tex-math notation="LaTeX" id="ImEquation103"><![CDATA[$Z(3930)\to J/\psi \omega$]]></tex-math></inline-formula> is shown in Figs. <xref ref-type="fig" rid="F1">1</xref>(b)&#x2013;(d). The amplitude for the processes <inline-formula><tex-math notation="LaTeX" id="ImEquation104"><![CDATA[$Z(3930)\to D^{(* )}\bar {D}^{(* )}\to J/\psi \omega$]]></tex-math></inline-formula> can be expressed as
<disp-formula id="M2"><label>(2)</label><tex-math notation="LaTeX" id="DmEquation2"><![CDATA[\[\mathcal {M}\left [ Z(3930)\to J/\psi \omega \right ] = 4\left [ \mathcal {M}_{\rm (b)}^{D}+ \mathcal {M}^{D^\ast }_{\rm (b)} + \mathcal {M}^{D}_{\rm (c)}+ \mathcal {M}^{D^\ast }_{\rm (c)}+ \mathcal {M}^{D}_{\rm (d)} + \mathcal {M}^{D^\ast }_{\rm (d)}\right ] ,\]]]></tex-math></disp-formula>
where the factor 4 in Eqs. (<xref ref-type="disp-formula" rid="M1">1</xref>) and (<xref ref-type="disp-formula" rid="M2">2</xref>) results from the charge conjugate and isospin transformations.
<fig id="F1"><label>Fig. 1.</label>
<caption><p>Typical diagrams describing the <inline-formula><tex-math notation="LaTeX" id="ImEquation105"><![CDATA[$X(3915)\to J/\psi \omega$]]></tex-math></inline-formula> (a) and <inline-formula><tex-math notation="LaTeX" id="ImEquation106"><![CDATA[$Z(3930)\to J/\psi \omega$]]></tex-math></inline-formula> ((b)&#x2013;(d)) decays. After making the charge conjugate transformation (<inline-formula><tex-math notation="LaTeX" id="ImEquation107"><![CDATA[$D^{(* )}\leftrightarrow \bar {D}^{(* )}$]]></tex-math></inline-formula>) and the isospin transformation (<inline-formula><tex-math notation="LaTeX" id="ImEquation108"><![CDATA[$D^{(* )0}\leftrightarrow D^{(* )+ }$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation109"><![CDATA[$\bar {D}^{(* )0} \leftrightarrow D^{(* )-}$]]></tex-math></inline-formula>), one gets other diagrams.</p></caption>
<graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ptv03801"/></fig></p>
<p>To write out the amplitudes corresponding to the diagrams listed in Fig. <xref ref-type="fig" rid="F1">1</xref>, we adopt the effective Lagrangian approach. The effective Lagrangian expressing the interactions of <inline-formula><tex-math notation="LaTeX" id="ImEquation110"><![CDATA[$X(3915)/Z(3930)$]]></tex-math></inline-formula> with <inline-formula><tex-math notation="LaTeX" id="ImEquation111"><![CDATA[$D\bar {D}$]]></tex-math></inline-formula> or <inline-formula><tex-math notation="LaTeX" id="ImEquation112"><![CDATA[$D\bar {D}^{\ast }+ \hbox {h.c.}$]]></tex-math></inline-formula> is given by [<xref ref-type="bibr" rid="C14">14</xref>]
<disp-formula id="M3"><label>(3)</label><tex-math notation="LaTeX" id="DmEquation3"><![CDATA[\begin{align} \mathcal {L}_{\chi _{cJ}^\prime D^{(\ast )}D^{(\ast )}} &= g_{_{\chi _{c0}^\prime DD}} \chi _{c0}^\prime \mathcal {DD}^\dagger -g_{_{\chi _{c2}^\prime DD}} {\chi _{c2}^\prime }_{\mu \nu } \partial ^{\mu } \mathcal {D} \partial ^{\nu }\mathcal {D}^\dagger \\ &\quad +ig_{_{\chi _{c2}^\prime D^\ast D}} \varepsilon _{\mu \nu \alpha \beta }\partial ^\mu \chi _{c2}^{\prime \nu \rho } (\partial ^\alpha \mathcal {D}^{\ast \beta } \partial _{\rho } \mathcal {D}^\dagger + \partial ^\alpha \mathcal {D}^{\ast \dagger \beta } \partial _{\rho } \mathcal {D}). \end{align}]]></tex-math></disp-formula>
The couplings of charmed mesons with the light vector meson <inline-formula><tex-math notation="LaTeX" id="ImEquation113"><![CDATA[$\omega$]]></tex-math></inline-formula> or charmonium <inline-formula><tex-math notation="LaTeX" id="ImEquation114"><![CDATA[$J/\psi$]]></tex-math></inline-formula> are constructed in Refs. [<xref ref-type="bibr" rid="C15">15</xref>, <xref ref-type="bibr" rid="C16">16</xref>], paying attention to the heavy quark symmetry and the chiral <inline-formula><tex-math notation="LaTeX" id="ImEquation115"><![CDATA[$SU(3)$]]></tex-math></inline-formula> symmetry, and are given below:
<disp-formula id="M4"><label>(4)</label><tex-math notation="LaTeX" id="DmEquation4"><![CDATA[\begin{align} \mathcal {L}_{J/\psi D^{(\ast )}D^{(\ast )}} &= i g_{_{J/\psi \mathcal {D}\mathcal {D}}} \psi _\mu \left ( \partial ^\mu \mathcal {D} {\mathcal {D}}^{\dagger } - \mathcal {D} \partial ^\mu {\mathcal {D}}^{\dagger }\right ) - g_{_{J/\psi \mathcal {D}^{\ast } \mathcal {D}}}^{} \varepsilon ^{\mu \nu \alpha \beta } \partial _\mu \psi _\nu \left ( \partial _\alpha \mathcal {D}^{\ast }_\beta {\mathcal {D}}^{\dagger } + \mathcal {D} \partial _\alpha {\mathcal {D}}^{* \dagger }_\beta \right ) \\ &\quad - i g_{_{J/\psi \mathcal {D}^{\ast } \mathcal {D}^{\ast }}}^{} \Bigl \{\psi ^\mu \left ( \partial _\mu \mathcal {D}^{* \nu } {\mathcal {D}}_\nu ^{* \dagger } - \mathcal {D}^{* \nu } \partial _\mu {\mathcal {D}}_\nu ^{* \dagger }\right ) + \left ( \partial _\mu \psi _\nu \mathcal {D}^{* \nu } - \psi _\nu \partial _\mu \mathcal {D}^{* \nu }\right ) {\mathcal {D}}^{* \mu \dagger } \\ &\quad + \mathcal {D}^{* \mu } (\psi ^\nu \partial _\mu {\mathcal {D}}^{* \dagger }_{\nu } - \partial _\mu \psi _\nu {\mathcal {D}}^{* \nu \dagger }) \Bigr \}, \end{align}]]></tex-math></disp-formula>
<disp-formula id="M5"><label>(5)</label><tex-math notation="LaTeX" id="DmEquation5"><![CDATA[\begin{align}\mathcal {L}_{_{\mathcal {D}^{(\ast )}\mathcal {D}^{(\ast )} \mathbb {V}}} &= -ig_{_{\mathcal {D}\mathcal {D} \mathbb {V}}}\mathcal {D}_{i}^{\dagger }{\stackrel {\leftrightarrow }{\partial }}_{\mu }\mathcal {D}^{j}(\mathbb {V}^{\mu })^{i}_{j} - 2f_{_{\mathcal {D^{* }} \mathcal {D}\mathbb {V}}} \varepsilon _{\mu \nu \alpha \beta }(\partial ^{\mu }\mathbb {V}^{\nu })^{i}_{j}\left ( \mathcal {D}_{i}^{\dagger }{\stackrel {\leftrightarrow }{\partial }}^{\alpha }\mathcal {D^{* }}^{\beta j} -\mathcal {D^{* }}_{i}^{\beta \dagger }{\stackrel {\leftrightarrow }{\partial }}^{\alpha }\mathcal {D}^{j}\right ) \\ &\quad +ig_{_{\mathcal {D^{* }}\mathcal {D^{* }}\mathbb {V}}}\mathcal {D^{* }}_{i}^{\nu \dagger }{\stackrel {\leftrightarrow }{\partial }}_{\mu }\mathcal {D^{* }}_{\nu }^{j}(\mathbb {V}^{\mu })^{i}_{j} 4if_{_{\mathcal {D^{* }}\mathcal {D^{* }}\mathbb {V}}}\mathcal {D^{* }}_{i\mu }^{\dagger }(\partial ^{\mu }\mathbb {V}^{\nu }-\partial ^{\nu } \mathbb {V}^{\mu })^{i}_{j} \mathcal {D^{* }}_{\nu }^{j}, \end{align}]]></tex-math></disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation116"><![CDATA[$\mathcal {D} = (D^0,D^+ ,D_s^+ )$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation117"><![CDATA[$(\mathcal {D}^\dagger )^T = (\bar {D}^0,D^-,D_s^-)$]]></tex-math></inline-formula>, and <inline-formula><tex-math notation="LaTeX" id="ImEquation118"><![CDATA[${\stackrel {\leftrightarrow }{\partial }}= {\stackrel {\rightarrow }{\partial }}-{\stackrel {\leftarrow }{\partial }}$]]></tex-math></inline-formula>. The light vector nonet meson can form the following <inline-formula><tex-math notation="LaTeX" id="ImEquation119"><![CDATA[$3\times 3$]]></tex-math></inline-formula> matrix <inline-formula><tex-math notation="LaTeX" id="ImEquation120"><![CDATA[$\mathbb {V}$]]></tex-math></inline-formula>:
<disp-formula id="M6"><label>(6)</label><tex-math notation="LaTeX" id="DmEquation6"><![CDATA[\[\mathbb {V} = \left ( \begin {matrix}\frac {\rho ^0}{\sqrt {2}} + \frac { \omega }{\sqrt {2}} & \rho ^+ & K^{\ast + } \\ \rho ^- & \frac {-\rho ^0}{\sqrt {2}}+ \frac {\omega }{\sqrt {2}} & K^{\ast 0} \\ K^{\ast -} & \bar {K}^{\ast 0} & \phi \end {matrix}\right ) .\]]]></tex-math></disp-formula>
The coupling constants of <inline-formula><tex-math notation="LaTeX" id="ImEquation121"><![CDATA[$\chi _{c0}^\prime \to D\bar {D}$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation122"><![CDATA[$\chi _{c2}^\prime \to D\bar {D},\,D\bar {D}^{\ast }+ \hbox {h.c.}$]]></tex-math></inline-formula> are obtained by fitting the total widths of <inline-formula><tex-math notation="LaTeX" id="ImEquation123"><![CDATA[$X(3915)$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation124"><![CDATA[$Z(3930)$]]></tex-math></inline-formula>, which will be presented later. The coupling constants of <inline-formula><tex-math notation="LaTeX" id="ImEquation125"><![CDATA[$J/\psi$]]></tex-math></inline-formula> interacting with a pair of charmed mesons and a coupling constant of charmed mesons interacting with a light vector meson are given in Table <xref ref-type="table" rid="TB1">1</xref> [<xref ref-type="bibr" rid="C15">15</xref>&#x02013;<xref ref-type="bibr" rid="C18">18</xref>].
<table-wrap id="TB1" position="float"><label>Table 1.</label>
<caption><p>The values of the coupling constants shown in Eqs. (<xref ref-type="disp-formula" rid="M3">3</xref>)&#x2013;(<xref ref-type="disp-formula" rid="M5">5</xref>). Here, we take <inline-formula><tex-math notation="LaTeX" id="ImEquation126"><![CDATA[$m_{D} = (m_{D^0}+m_{D^{\pm }})/2$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation127"><![CDATA[$m_{D^{\ast }}=(m_{D^{*0}}+m_{D^{* \pm }}) /2$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation128"><![CDATA[$g_V=m_\rho /f_\pi$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation129"><![CDATA[$m_\rho =0.77$]]></tex-math></inline-formula> MeV, <inline-formula><tex-math notation="LaTeX" id="ImEquation130"><![CDATA[$\beta =0.9$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation131"><![CDATA[$\lambda =0.56$]]></tex-math></inline-formula> GeV<inline-formula><tex-math notation="LaTeX" id="ImEquation132"><![CDATA[$^{-1}$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation133"><![CDATA[$g=0.59$]]></tex-math></inline-formula>, and <inline-formula><tex-math notation="LaTeX" id="ImEquation134"><![CDATA[$f_\pi =132$]]></tex-math></inline-formula> MeV [<xref ref-type="bibr" rid="C15">15</xref>&#x02013;<xref ref-type="bibr" rid="C18">18</xref>].</p></caption>
<table frame="hsides">
<colgroup>
<col align="left"/>
<col align="center"/>
<col align="center"/>
<col align="center"/>
<col align="center"/>
<col align="center"/>
</colgroup>
<thead>
<tr>
<th colspan="1" align="left">Coupling</th>
<th colspan="1" align="center">Expression</th>
<th colspan="1" align="center">Value</th>
<th colspan="1" align="center">Coupling</th>
<th colspan="1" align="center">Expression</th>
<th colspan="1" align="center">Value</th>
</tr>
</thead>
<tbody>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation135"><![CDATA[$g_{_{J/\psi \mathcal {D}\mathcal {D}}}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation136"><![CDATA[$-$]]></tex-math></inline-formula></td>
<td>7.71</td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation137"><![CDATA[$g_{_{\mathcal {D}^{\ast }\mathcal {D}^{\ast }\mathbb {V}}}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation138"><![CDATA[$\dfrac {\beta g_V}{\sqrt {2}}$]]></tex-math></inline-formula></td>
<td>3.71</td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation139"><![CDATA[$g_{_{J/\psi \mathcal {D}^{\ast } \mathcal {D}}}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation140"><![CDATA[$-$]]></tex-math></inline-formula></td>
<td>3.98&#x2009;GeV<inline-formula><tex-math notation="LaTeX" id="ImEquation141"><![CDATA[$^{-1}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation142"><![CDATA[$f_{_{\mathcal {D}^{\ast }\mathcal {D}^{\ast }\mathbb {V}}}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation143"><![CDATA[$\dfrac {\lambda g_V m_{D^{\ast }}}{\sqrt {2}}$]]></tex-math></inline-formula></td>
<td>4.64</td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation144"><![CDATA[$g_{_{J/\psi \mathcal {D}^{\ast }\mathcal {D}^{\ast }}}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation145"><![CDATA[$g_{_{J/\psi \mathcal {D}\mathcal {D}}}$]]></tex-math></inline-formula></td>
<td>7.71</td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation146"><![CDATA[$f_{_{\mathcal {D}^{\ast }\mathcal {D}\mathbb {V}}}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation147"><![CDATA[$\dfrac {\lambda g_V}{\sqrt {2}}$]]></tex-math></inline-formula></td>
<td>2.31&#x2009;GeV<inline-formula><tex-math notation="LaTeX" id="ImEquation148"><![CDATA[$^{-1}$]]></tex-math></inline-formula></td>
</tr>
<tr>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation149"><![CDATA[$g_{_{\mathcal {D}\mathcal {D}\mathbb {V}}}$]]></tex-math></inline-formula></td>
<td><inline-formula><tex-math notation="LaTeX" id="ImEquation150"><![CDATA[$\dfrac {\beta g_V}{\sqrt {2}}$]]></tex-math></inline-formula></td>
<td>3.71</td>
<td/>
<td/>
<td/>
</tr>
</tbody>
</table>
</table-wrap></p>
<p>The amplitudes for <inline-formula><tex-math notation="LaTeX" id="ImEquation151"><![CDATA[$\chi _{c0}^\prime (p_0) \to [D(p_1) \bar {D}(p_2)]D^{(\ast )} (q) \to J/\psi (p_3) \omega (p_4)$]]></tex-math></inline-formula> corresponding to Fig. <xref ref-type="fig" rid="F1">1</xref>(a) are given by
<disp-formula id="M7"><label>(7)</label><tex-math notation="LaTeX" id="DmEquation7"><![CDATA[\begin{align} \mathcal {A}_{\rm (a)}^{D} &= (i)^3\int \frac {d^4 q}{(2\pi ^4)} [g_{_{\chi _{c0}^\prime \mathcal {DD}}}] [ig_{_{J/\psi \mathcal {D}\mathcal {D}}} {\epsilon _{\psi }}_\mu (i q^\mu +i p_1^\mu )] [-ig_{_{\mathcal {D}\mathcal {D}\mathbb {V}}} (-ip_{2\nu }+iq_\nu ){\epsilon _\omega }^\nu ] \\ &\quad \times \frac {i}{p_1^2-m_{D}^2} \frac {i}{p_2^2-m_{D}^2} \frac {i}{q^2-m_{D}^2}\,\mathcal {F}^2 (q^2), \\ \mathcal {A}^{D^\ast }_{\rm (a)} &= (i)^3\int \frac {d^4 q}{(2\pi ^4)}[g_{_{\chi _{c0}^\prime \mathcal {DD}}}] [-g_{_{J/\psi \mathcal {D}^{\ast }\mathcal {D}}}\varepsilon ^{\mu \nu \alpha \beta }(ip_{3\mu }){\epsilon _{\psi }}_\nu (i q_\alpha )] \\ &\quad \times [-2f_{_{\mathcal {D}^{\ast }\mathcal {D}\mathbb {V}}} \varepsilon _{\sigma \lambda \rho \xi }(ip_4^\sigma )\epsilon _{\omega }^\lambda (ip_2^\rho -iq^\rho )]\frac {i}{p_1^2-m_{D}^2} \frac {i}{p_2^2-nm_{D}^2} \frac {i\tilde {g}_\beta ^{\xi }(q)}{q^2-m_{D^{\ast }}^2}\mathcal {F}^2 (q^2), \end{align}]]></tex-math></disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation152"><![CDATA[$\mathcal {A}_{\rm (a)}^{D}$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation153"><![CDATA[$\mathcal {A}_{\rm (a)}^{D^\ast }$]]></tex-math></inline-formula> are the amplitudes corresponding to diagram (a) in Fig. <xref ref-type="fig" rid="F1">1</xref> with the <inline-formula><tex-math notation="LaTeX" id="ImEquation154"><![CDATA[$D$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation155"><![CDATA[$D^\ast$]]></tex-math></inline-formula> meson exchanges, respectively. Similarly, we can easily write out the the expressions for the decay amplitudes of <inline-formula><tex-math notation="LaTeX" id="ImEquation156"><![CDATA[$Z(3930)\to J/\psi \omega$]]></tex-math></inline-formula> corresponding to Figs. <xref ref-type="fig" rid="F1">1</xref>(b)&#x2013;(d), which are
<disp-formula id="M8"><label>(8)</label><tex-math notation="LaTeX" id="DmEquation8"><![CDATA[\begin{align} \mathcal {M}^{D}_{\rm (b)} &= (i)^3\int \frac {d^4 q}{(2\pi ^4)} \left [ -g_{_{\chi _{c2}^\prime \mathcal {DD}}} \epsilon _{\chi _{c2}^\prime }^{\mu \nu }(ip_{1\mu })(ip_{2\nu })\right ] [ig_{_{J/\psi \mathcal {D}\mathcal {D}}}{\epsilon _{\psi }}_\rho (i q^\rho +i p_1^\rho )] \\ &\quad \times [-ig_{_{\mathcal {D}\mathcal {D}\omega }}(-i p_{2\tau }+iq_\tau ) \epsilon _\omega ^\tau ] \frac {i}{p_1^2-m_{D}^2}\frac {i}{p_2^2-m_{D}^2}\frac {i}{q^2-m_{D}^2}\,\mathcal {F}^2(q^2), \\ \mathcal {M}^{D^\ast }_{\rm (b)} &= (i)^3\int \frac {d^4 q}{(2\pi ^4)} \left [ -g_{_{\chi _{c2}^\prime \mathcal {DD}}} \epsilon _{\chi _{c2}^\prime }^{\mu \nu }(ip_{1\mu })(ip_{2\nu })\right ] [-g_{_{J/\psi \mathcal {D}^{\ast }\mathcal {D}}} \varepsilon _{\theta \rho \alpha \beta }(ip_{3}^{\theta })\epsilon _{\psi }^\rho (i q^\alpha )] \\ &\quad \times \left [ -2f_{_{\mathcal {D}^{\ast }\mathcal {D}\omega }}\varepsilon _{\sigma \tau \lambda \phi } (ip_4^\sigma ) \epsilon _{\omega }^\tau (ip_2^\lambda -iq^\lambda )\right ] \frac {i}{p_1^2-m_{D}^2} \frac {i}{p_2^2-m_{D}^2} \frac {i \tilde {g}^{\beta \phi }(q)}{q^2-m_{D^{\ast }}^2} \mathcal {F}^2(q^2),\\ \mathcal {M}^{D}_{\rm (c)} &= (i)^3\int \frac {d^4 q}{(2\pi ^4)} \left [ ig_{\chi _{c2}^\prime D^\ast D} \varepsilon _{\delta \mu \theta \phi }(-ip_0^\delta ) \epsilon _{\chi _{c2}^\prime }^{\mu \nu } (ip_2^{\theta }) (ip_{1 \nu })\right ] [ig_{_{J/\psi \mathcal {D}\mathcal {D}}} \epsilon _{\psi }^\rho (i q_\rho +i p_{1\rho })] \\ &\quad \times \left [ -2f_{_{\mathcal {D}^{\ast }\mathcal {D} \omega }}\varepsilon _{\sigma \tau \lambda \alpha } (ip_4^\sigma ) \epsilon _{\omega }^\tau (-ip_2^\lambda +iq^\lambda )\right ] \frac {i}{p_1^2-m_{D}^2} \frac {i\tilde {g}^{\phi \alpha }(p_2)}{p_2^2- m_{D^{\ast }}^2} \frac {i}{q^2-m_{D}^2}\,\mathcal {F}^2(q^2), \\ \mathcal {M}^{D^\ast }_{\rm (c)} &= (i)^3\int \frac {d^4 q}{(2\pi ^4)} \left [ ig_{\chi _{c2}^\prime D^\ast D} \varepsilon _{\delta \mu \theta \phi }(-ip_0^\delta ) \epsilon _{\chi _{c2}^\prime }^{\mu \nu } (ip_2^{\theta }) (ip_{1 \nu })\right ] [-g_{_{J/\psi \mathcal {D}^{\ast }\mathcal {D}}}\varepsilon _{\lambda \rho \alpha \beta } (ip_{3}^{\lambda }) \epsilon _{\psi }^\rho (iq^\alpha )] \\ &\quad \times \left [ ig_{_{\mathcal {D}^{\ast }\mathcal {D}^{\ast }\omega }} (-ip_{2\tau }+i q_{\tau }) \epsilon _{\omega }^\tau g_{\zeta \sigma } +4if_{_{\mathcal {D}^{\ast }\mathcal {D}^{\ast }\omega }} \epsilon _{\omega }^{\tau }(ip_{4 \zeta } g_{\sigma \tau } - i p_{4\sigma } g_{\tau \zeta })\right ] \\ &\quad \times \frac {i}{p_1^2-m_{D}^2} \frac {i\tilde {g}^{\phi \sigma }(p_2)}{p_2^2-m_{D^{\ast }}^2} \frac {i \tilde {g}^{\zeta \beta }(q)}{q^2-m_{D^{\ast }}^2}\,\mathcal {F}^2(q^2),\\ \mathcal {M}^{D}_{\rm (d)} &= (i)^3\int \frac {d^4 q}{(2\pi ^4)} \left [ ig_{\chi _{c2}^\prime D^\ast D} \varepsilon _{\delta \mu \theta \phi }(-ip_0^\delta ) \epsilon _{\chi _{c2}^\prime }^{\mu \nu } (ip_1^\theta ) (ip_2^\nu )\right ] [-g_{_{J/\psi D^\ast D}} \varepsilon _{\lambda \rho \alpha \beta } (ip_3^\lambda ) \epsilon _{\psi }^\rho (-ip_1^\alpha )] \\ &\quad \times [ig_{_{DD\omega }} \epsilon _{\omega }^\tau (ip_{2\tau } -iq_{\tau })] \frac {i\tilde {g}^{\phi \beta }(p_1)}{p_1^2-m_{D^\ast }^2} \frac {i}{p_2^2-m_{D}^2} \frac {i}{q^2-m_{D}^2}\,\mathcal {F}^2(q^2),\\ \mathcal {M}^{D^\ast }_{\rm (d)} &= (i)^3\int \frac {d^4 q}{(2\pi ^4)} \left [ ig_{\chi _{c2}^\prime D^\ast D} \varepsilon _{\delta \mu \theta \phi } (-ip_0^\delta ) \epsilon _{\chi _{c2}^\prime }^{\mu \nu } (ip_1^\theta )(ip_2^\nu )\right ] \\ &\quad \times \left [ -ig_{_{J/\psi D^\ast D^\ast }} \epsilon _{\psi }^\rho (g_{\alpha \beta } (-ip_{2\rho }+iq_{\rho }) +g_{\beta \rho } (ip_{3\alpha } +ip_{1\alpha }) +g_{\alpha \rho } (-iq_{\beta } -ip_{3 \beta }))\right ] \\ &\quad \times \left [ -2f_{_{D^\ast D \omega }} \varepsilon _{\sigma \tau \lambda \zeta } (ip_4^\sigma ) \epsilon _{\omega }^\tau (-iq^\lambda +ip_2^\lambda )\right ] \frac {i\tilde {g}^{\phi \beta }(p_1)}{p_1^2-m_{D^\ast }^2} \frac {i}{p_2^2-m_{D}^2} \frac {i\tilde {g}^{\alpha \zeta }(q)}{q^2-m_{D^{\ast }}^2}\,\mathcal {F}^2(q^2), \end{align}]]></tex-math></disp-formula>
with <inline-formula><tex-math notation="LaTeX" id="ImEquation157"><![CDATA[$\tilde {g}^{\alpha \beta }(p)=-g^{\alpha \beta }+p^\alpha p^\beta /m_{D^\ast }^2$]]></tex-math></inline-formula>, where <inline-formula><tex-math notation="LaTeX" id="ImEquation158"><![CDATA[$\mathcal {F}(q^2)$]]></tex-math></inline-formula> is the form factor, which is introduced not only to compensate the off-shell effects of the charmed meson but also to describe the structure effects of the vertex of a charmed meson pair interacting with <inline-formula><tex-math notation="LaTeX" id="ImEquation159"><![CDATA[$J/\psi$]]></tex-math></inline-formula> or <inline-formula><tex-math notation="LaTeX" id="ImEquation160"><![CDATA[$\omega$]]></tex-math></inline-formula>. In this work, we adopt the form factor in the form
<disp-formula id="M9"><label>(9)</label><tex-math notation="LaTeX" id="DmEquation9"><![CDATA[\[\mathcal {F}(q^2) = \left ( {m_{\rm E}^2 - \Lambda ^{2}}\over {q^2- \Lambda ^{2}}\right ) ^N, \quad \left \{\begin {array}{ll}N=1, &\hbox {monopole form;} \\ N=2, &\hbox {dipole form,} \end {array}\right .\]]]></tex-math></disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation161"><![CDATA[$q$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation162"><![CDATA[$m_{\rm E}$]]></tex-math></inline-formula> are the momentum and the mass of the exchanged charmed meson, respectively. Furthermore, <inline-formula><tex-math notation="LaTeX" id="ImEquation163"><![CDATA[$\Lambda$]]></tex-math></inline-formula> can be parameterized as <inline-formula><tex-math notation="LaTeX" id="ImEquation164"><![CDATA[$\Lambda =m_{\rm E}+ \alpha \Lambda _{\rm QCD}$]]></tex-math></inline-formula> with a dimensionless parameter <inline-formula><tex-math notation="LaTeX" id="ImEquation165"><![CDATA[$\alpha$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation166"><![CDATA[$\Lambda _{\rm QCD}=220$]]></tex-math></inline-formula> MeV. The parameter <inline-formula><tex-math notation="LaTeX" id="ImEquation167"><![CDATA[$\alpha$]]></tex-math></inline-formula> is of order unity and depends on the specific process [<xref ref-type="bibr" rid="C13">13</xref>, <xref ref-type="bibr" rid="C18">18</xref>].</p>
<p>With the above elaborate expressions for the amplitudes, one can obtain the partial decay width for <inline-formula><tex-math notation="LaTeX" id="ImEquation168"><![CDATA[$\chi _{cJ}^\prime \to J/\psi \omega \,(J=0,2)$]]></tex-math></inline-formula> as
<disp-formula id="M10"><label>(10)</label><tex-math notation="LaTeX" id="DmEquation10"><![CDATA[\[d\Gamma _{\chi _{cJ}^\prime \to J/\psi \omega } =\frac {1}{2J+1} \frac {1}{32 \pi ^2} \overline {\left | \mathcal {M}_{\chi _{cJ}^\prime \to J/\psi \omega } \right | ^2} \frac {|\vec {p}|}{m_{\chi _{cJ}^\prime }^2} d\Omega ,\]]]></tex-math></disp-formula>
where the overline indicates the sum over the polarizations of the vector meson <inline-formula><tex-math notation="LaTeX" id="ImEquation169"><![CDATA[$J/\psi , \omega$]]></tex-math></inline-formula> and tensor meson <inline-formula><tex-math notation="LaTeX" id="ImEquation170"><![CDATA[$\chi _{c2}^\prime$]]></tex-math></inline-formula>, and <inline-formula><tex-math notation="LaTeX" id="ImEquation171"><![CDATA[$\vec {p}$]]></tex-math></inline-formula> indicates the three-momentum of <inline-formula><tex-math notation="LaTeX" id="ImEquation172"><![CDATA[$J/\psi$]]></tex-math></inline-formula> in the initial state at rest.</p>
<p>If <inline-formula><tex-math notation="LaTeX" id="ImEquation173"><![CDATA[$X(3915)$]]></tex-math></inline-formula> is a <inline-formula><tex-math notation="LaTeX" id="ImEquation174"><![CDATA[$\chi _{c0}^\prime (2P)$]]></tex-math></inline-formula> state, <inline-formula><tex-math notation="LaTeX" id="ImEquation175"><![CDATA[$D\bar {D}$]]></tex-math></inline-formula> is its dominant decay. Hence, we can use the experimental width of <inline-formula><tex-math notation="LaTeX" id="ImEquation176"><![CDATA[$X(3915)$]]></tex-math></inline-formula> [<xref ref-type="bibr" rid="C1">1</xref>] to determine the coupling constant of <inline-formula><tex-math notation="LaTeX" id="ImEquation177"><![CDATA[$\chi _{c0}^\prime \to D\bar {D}$]]></tex-math></inline-formula> interaction, i.e., <inline-formula><tex-math notation="LaTeX" id="ImEquation178"><![CDATA[$g_{\chi _{c0}^{\prime }D\bar {D}}= 2.37$]]></tex-math></inline-formula> GeV. However, for <inline-formula><tex-math notation="LaTeX" id="ImEquation179"><![CDATA[$Z(3930)$]]></tex-math></inline-formula>, there exist two main decay modes <inline-formula><tex-math notation="LaTeX" id="ImEquation180"><![CDATA[$D\bar {D}$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation181"><![CDATA[$D\bar {D}^{\ast }+ \hbox {h.c.}$]]></tex-math></inline-formula> Since experiments have so far not given the ratio of <inline-formula><tex-math notation="LaTeX" id="ImEquation182"><![CDATA[$BR(Z(3930)\to D\bar {D})$]]></tex-math></inline-formula> to <inline-formula><tex-math notation="LaTeX" id="ImEquation183"><![CDATA[$BR(Z(3930)\to D\bar {D}^{\ast }+ \hbox {h.c.})$]]></tex-math></inline-formula>, we must determine these corresponding coupling constants from the theoretical results estimated by the quark pair creation model. In Ref. [<xref ref-type="bibr" rid="C4">4</xref>], the wave functions of <inline-formula><tex-math notation="LaTeX" id="ImEquation184"><![CDATA[$\chi _{cJ}^\prime$]]></tex-math></inline-formula> are simulated by a simple harmonic oscillator wave function with a parameter <inline-formula><tex-math notation="LaTeX" id="ImEquation185"><![CDATA[$R$]]></tex-math></inline-formula>, which means a root-mean-square radius of the wave function. The partial and total decay widths of <inline-formula><tex-math notation="LaTeX" id="ImEquation186"><![CDATA[$\chi _{cJ}^\prime$]]></tex-math></inline-formula> are dependent on this unique parameter <inline-formula><tex-math notation="LaTeX" id="ImEquation187"><![CDATA[$R$]]></tex-math></inline-formula>. One can determine the parameter value <inline-formula><tex-math notation="LaTeX" id="ImEquation188"><![CDATA[$R \simeq 1.9\, {\rm GeV}^{-1}$]]></tex-math></inline-formula> in the spatial wave function from the partial decay width of <inline-formula><tex-math notation="LaTeX" id="ImEquation189"><![CDATA[$\chi _{c0}^\prime$]]></tex-math></inline-formula> under the assumption <inline-formula><tex-math notation="LaTeX" id="ImEquation190"><![CDATA[$\Gamma _{\chi _{c0}^\prime \to D\bar {D}} \simeq \Gamma _{\chi _{c0}^\prime }^{{\rm tot}}$]]></tex-math></inline-formula>. With the parameter <inline-formula><tex-math notation="LaTeX" id="ImEquation191"><![CDATA[$R$]]></tex-math></inline-formula> estimated by the center value of <inline-formula><tex-math notation="LaTeX" id="ImEquation192"><![CDATA[$\Gamma _{\chi _{c0}^\prime }^{{\rm tot}}$]]></tex-math></inline-formula>, we obtain <inline-formula><tex-math notation="LaTeX" id="ImEquation193"><![CDATA[$|g_{\chi _{c2}^\prime D D}|=11.69$]]></tex-math></inline-formula> <inline-formula><tex-math notation="LaTeX" id="ImEquation194"><![CDATA[${\rm GeV}^{-1}$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation195"><![CDATA[$|g_{\chi _{c2}^\prime D^\ast D}|= 7.83$]]></tex-math></inline-formula> <inline-formula><tex-math notation="LaTeX" id="ImEquation196"><![CDATA[${\rm GeV}^{-2}$]]></tex-math></inline-formula>.</p>
<p>For <inline-formula><tex-math notation="LaTeX" id="ImEquation197"><![CDATA[$Z(3930)$]]></tex-math></inline-formula> with the assignment of <inline-formula><tex-math notation="LaTeX" id="ImEquation198"><![CDATA[$\chi _{c2}^\prime$]]></tex-math></inline-formula>, it dominantly decays into <inline-formula><tex-math notation="LaTeX" id="ImEquation199"><![CDATA[$D\bar {D}$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation200"><![CDATA[$D^\ast \bar {D}+ \hbox {h.c.}$]]></tex-math></inline-formula> The absolute values of the coupling constants between <inline-formula><tex-math notation="LaTeX" id="ImEquation201"><![CDATA[$\chi _{c2}^\prime$]]></tex-math></inline-formula> and the charmed meson pairs are evaluated by the quark pair creation model. However, the relative sign of the coupling constants <inline-formula><tex-math notation="LaTeX" id="ImEquation202"><![CDATA[$g_{\chi _{c2}^\prime DD}$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation203"><![CDATA[$g_{\chi _{c2}^\prime D^{\ast }D}$]]></tex-math></inline-formula> in Eq. (<xref ref-type="disp-formula" rid="M3">3</xref>) can be either positive or negative, which corresponds to the subscripts <inline-formula><tex-math notation="LaTeX" id="ImEquation204"><![CDATA[$+ + $]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation205"><![CDATA[$+ -$]]></tex-math></inline-formula> shown in Fig. <xref ref-type="fig" rid="F2">2</xref>, respectively. Thus, we discuss two cases for <inline-formula><tex-math notation="LaTeX" id="ImEquation206"><![CDATA[$Z(3930)\to J/\psi \omega$]]></tex-math></inline-formula>.
<fig id="F2"><label>Fig. 2.</label>
<caption><p><inline-formula><tex-math notation="LaTeX" id="ImEquation207"><![CDATA[$\alpha$]]></tex-math></inline-formula> dependence of the ratio of the width of <inline-formula><tex-math notation="LaTeX" id="ImEquation208"><![CDATA[$X(3915)\to J/\psi \omega$]]></tex-math></inline-formula> to that of <inline-formula><tex-math notation="LaTeX" id="ImEquation209"><![CDATA[$Z(3930)\to J/\psi \omega$]]></tex-math></inline-formula>. Here, we define <inline-formula><tex-math notation="LaTeX" id="ImEquation210"><![CDATA[$R_{+ + }=\Gamma [X(3915)\to J/\psi \omega ]/\Gamma [Z(3930)\to J/\psi \omega ]_{+ + }$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation211"><![CDATA[$R_{+ -}=\Gamma [X(3915)\to J/\psi \omega ]/\Gamma [Z(3930)\to J/\psi \omega ]_{+ -}$]]></tex-math></inline-formula>. In addition, we use the superscripts &#x201C;Monopole&#x201D; and &#x201C;Dipole&#x201D; to distinguish different results by taking monopole and dipole form factors in the calculation, respectively. The calculated results are <inline-formula><tex-math notation="LaTeX" id="ImEquation212"><![CDATA[$R_{+ + }^{{\rm Monopole}}=850$]]></tex-math></inline-formula>&#x2013;1400, <inline-formula><tex-math notation="LaTeX" id="ImEquation213"><![CDATA[$R_{+ + }^{{\rm Dipole}}=239$]]></tex-math></inline-formula>&#x2013;558, <inline-formula><tex-math notation="LaTeX" id="ImEquation214"><![CDATA[$R_{+ -}^{{\rm Monopole}}=87$]]></tex-math></inline-formula>&#x2013;130, and <inline-formula><tex-math notation="LaTeX" id="ImEquation215"><![CDATA[$R_{+ -}^{{{\rm Dipole}}}=27$]]></tex-math></inline-formula>&#x2013;59.</p></caption>
<graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ptv03802"/></fig></p>
<p>In Fig. <xref ref-type="fig" rid="F2">2</xref>, we give the ratio of the width of <inline-formula><tex-math notation="LaTeX" id="ImEquation216"><![CDATA[$X(3915)\to J/\psi \omega$]]></tex-math></inline-formula> to that of <inline-formula><tex-math notation="LaTeX" id="ImEquation217"><![CDATA[$Z(3930)\to J/\psi \omega$]]></tex-math></inline-formula>. This result shows that the width of <inline-formula><tex-math notation="LaTeX" id="ImEquation218"><![CDATA[$X(3915) \to J/\psi \omega$]]></tex-math></inline-formula> is at least one order of magnitude larger than that of <inline-formula><tex-math notation="LaTeX" id="ImEquation219"><![CDATA[$Z(3930)\to J/\psi \omega$]]></tex-math></inline-formula> in two different cases (see Fig. <xref ref-type="fig" rid="F2">2</xref> for more details). Although the decay width for <inline-formula><tex-math notation="LaTeX" id="ImEquation220"><![CDATA[$\chi _{c0}^\prime /\chi _{c2}^\prime \to J/\psi \omega$]]></tex-math></inline-formula> calculated in this work strongly depends on the parameter <inline-formula><tex-math notation="LaTeX" id="ImEquation221"><![CDATA[$\alpha$]]></tex-math></inline-formula>, the ratio of the width of <inline-formula><tex-math notation="LaTeX" id="ImEquation222"><![CDATA[$X(3915)\to J/\psi \omega$]]></tex-math></inline-formula> to that of <inline-formula><tex-math notation="LaTeX" id="ImEquation223"><![CDATA[$Z(3930)\to J/\psi \omega$]]></tex-math></inline-formula> has a very large value and is weakly dependent on the parameter <inline-formula><tex-math notation="LaTeX" id="ImEquation224"><![CDATA[$\alpha$]]></tex-math></inline-formula>, as shown in Fig. <xref ref-type="fig" rid="F2">2</xref>. Such a large ratio could explain why Belle only reported one enhancement structure, <inline-formula><tex-math notation="LaTeX" id="ImEquation225"><![CDATA[$X(3915)$]]></tex-math></inline-formula>, in the <inline-formula><tex-math notation="LaTeX" id="ImEquation226"><![CDATA[$J/\psi \omega$]]></tex-math></inline-formula> invariant mass spectrum of the <inline-formula><tex-math notation="LaTeX" id="ImEquation227"><![CDATA[$\gamma \gamma \to J/\psi \omega$]]></tex-math></inline-formula> process.</p>
<p>In addition, the <inline-formula><tex-math notation="LaTeX" id="ImEquation228"><![CDATA[$\alpha$]]></tex-math></inline-formula> dependence of the <inline-formula><tex-math notation="LaTeX" id="ImEquation229"><![CDATA[$\chi _{cJ}^\prime \to J/\psi \omega$]]></tex-math></inline-formula> partial decay widths is presented in Fig. <xref ref-type="fig" rid="F3">3</xref>. Here, we take the monopole form factor as an example. As one finds in Fig. <xref ref-type="fig" rid="F3">3</xref>, the partial decay widths are strongly dependent on the parameter <inline-formula><tex-math notation="LaTeX" id="ImEquation230"><![CDATA[$\alpha$]]></tex-math></inline-formula>. As for <inline-formula><tex-math notation="LaTeX" id="ImEquation231"><![CDATA[$\chi _{c0}^\prime \to J/\psi \omega$]]></tex-math></inline-formula>, the partial decay width varies from <inline-formula><tex-math notation="LaTeX" id="ImEquation232"><![CDATA[$3.5 \times 10^{-3}~{\rm MeV}$]]></tex-math></inline-formula> to 0.15 MeV in the range <inline-formula><tex-math notation="LaTeX" id="ImEquation233"><![CDATA[$1\lt \alpha \lt 4$]]></tex-math></inline-formula>, while, for <inline-formula><tex-math notation="LaTeX" id="ImEquation234"><![CDATA[$\chi _{c2}^\prime$]]></tex-math></inline-formula>, the partial decay width of <inline-formula><tex-math notation="LaTeX" id="ImEquation235"><![CDATA[$\chi _{c2}^\prime \to J/\psi \omega$]]></tex-math></inline-formula> varies from <inline-formula><tex-math notation="LaTeX" id="ImEquation236"><![CDATA[$4.1 \times 10^{-6}$]]></tex-math></inline-formula>MeV to <inline-formula><tex-math notation="LaTeX" id="ImEquation237"><![CDATA[$1.1 \times 10^{-4}$]]></tex-math></inline-formula>MeV or <inline-formula><tex-math notation="LaTeX" id="ImEquation238"><![CDATA[$4.0 \times 10^{-5}$]]></tex-math></inline-formula>MeV to <inline-formula><tex-math notation="LaTeX" id="ImEquation239"><![CDATA[$1.1 \times 10^{-3}$]]></tex-math></inline-formula>MeV depending on the relative sign between <inline-formula><tex-math notation="LaTeX" id="ImEquation240"><![CDATA[$g_{\chi _{c2}^\prime DD}$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation241"><![CDATA[$g_{\chi _{c2}^\prime D^\ast D}$]]></tex-math></inline-formula>. In the present calculations, the loop integrals in Eqs. (<xref ref-type="disp-formula" rid="M7">7</xref>) and (<xref ref-type="disp-formula" rid="M8">8</xref>) are evaluated by the Cutkosky cutting rules, where only the imaginary part of the amplitudes is considered. As for the case of the dipole form factor, the magnitudes of the partial decay widths are at least one order smaller than the corresponding ones estimated by the monopole form factor. The calculations in Ref. [<xref ref-type="bibr" rid="C26">26</xref>] also indicate that the monopole form factor is more suitable to estimate the partial decay widths of the <inline-formula><tex-math notation="LaTeX" id="ImEquation242"><![CDATA[$\chi _{cJ}^\prime \to J/\psi \omega$]]></tex-math></inline-formula> process.
<fig id="F3"><label>Fig. 3.</label>
<caption><p><inline-formula><tex-math notation="LaTeX" id="ImEquation243"><![CDATA[$\alpha$]]></tex-math></inline-formula> dependence of the partial decay widths of <inline-formula><tex-math notation="LaTeX" id="ImEquation244"><![CDATA[$\chi _{cJ}^\prime \to J/\psi \omega$]]></tex-math></inline-formula>, where <inline-formula><tex-math notation="LaTeX" id="ImEquation245"><![CDATA[$X(3915)$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation246"><![CDATA[$Z(3930)$]]></tex-math></inline-formula> are assigned as <inline-formula><tex-math notation="LaTeX" id="ImEquation247"><![CDATA[$\chi _{c0}^\prime$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation248"><![CDATA[$\chi _{c2}^\prime$]]></tex-math></inline-formula>, respectively. The loop integrals in Eqs. (<xref ref-type="disp-formula" rid="M7">7</xref>) and (<xref ref-type="disp-formula" rid="M8">8</xref>) are evaluated by the Cutkosky cutting rules. The subscripts <inline-formula><tex-math notation="LaTeX" id="ImEquation249"><![CDATA[$+ + $]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation250"><![CDATA[$+ -$]]></tex-math></inline-formula> are the same as those in Fig. <xref ref-type="fig" rid="F2">2</xref>.</p></caption>
<graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="ptv03803"/></fig></p>
<p>As indicated above, the absolute decay widths of <inline-formula><tex-math notation="LaTeX" id="ImEquation251"><![CDATA[$X(3915)\to J/\psi \omega$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation252"><![CDATA[$Z(3930)\to J/\psi \omega$]]></tex-math></inline-formula> are strongly dependent on the parameter <inline-formula><tex-math notation="LaTeX" id="ImEquation253"><![CDATA[$\alpha$]]></tex-math></inline-formula>, which means that there exists uncertainty in the prediction of these decay widths. In addition, we notice that extracting the decay widths of <inline-formula><tex-math notation="LaTeX" id="ImEquation254"><![CDATA[$X(3915)\to J/\psi \omega$]]></tex-math></inline-formula> from that of <inline-formula><tex-math notation="LaTeX" id="ImEquation255"><![CDATA[$Z(3930)\to J/\psi \omega$]]></tex-math></inline-formula> via the experimental data depends on our understanding of the two-photon decay width of <inline-formula><tex-math notation="LaTeX" id="ImEquation256"><![CDATA[$X(3915)$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation257"><![CDATA[$Z(3930)$]]></tex-math></inline-formula>, where its predicted two-photon decay width varies with different models. In Refs. [<xref ref-type="bibr" rid="C20">20</xref>&#x02013;<xref ref-type="bibr" rid="C23">23</xref>], the two-photon decay width is about 1&#x2013;2&#x2009;keV in the relativistic quark model, while the Salpeter method indicates that the decay width for <inline-formula><tex-math notation="LaTeX" id="ImEquation258"><![CDATA[$\chi _{c0}^\prime$]]></tex-math></inline-formula> can be larger than 3&#x2009;keV in a relativistic form and about 5.47&#x2009;keV in a non-relativistic form [<xref ref-type="bibr" rid="C24">24</xref>]. If the center values of the total decay width of <inline-formula><tex-math notation="LaTeX" id="ImEquation259"><![CDATA[$\chi _{c0}^\prime$]]></tex-math></inline-formula> and the measured branching ratio <inline-formula><tex-math notation="LaTeX" id="ImEquation260"><![CDATA[$\Gamma _{\chi _{c0}^\prime \to \gamma \gamma }\mathcal {B}(\chi _{c0}^\prime \to J/\psi \omega )$]]></tex-math></inline-formula> are adopted, the partial decay width of <inline-formula><tex-math notation="LaTeX" id="ImEquation261"><![CDATA[$\chi _{c0}^\prime \to J/\psi \omega$]]></tex-math></inline-formula> can be less than two hundred keV to 1 MeV, depending on the choice of <inline-formula><tex-math notation="LaTeX" id="ImEquation262"><![CDATA[$\Gamma _{\chi _{c0}^\prime \to \gamma \gamma }$]]></tex-math></inline-formula>. In the present work, the evaluated partial decay width can reach 150 keV for <inline-formula><tex-math notation="LaTeX" id="ImEquation263"><![CDATA[$\alpha =4$]]></tex-math></inline-formula>, which is consistent with the experimental measurements [<xref ref-type="bibr" rid="C1">1</xref>].</p>
<p>In summary, <inline-formula><tex-math notation="LaTeX" id="ImEquation264"><![CDATA[$X(3915)$]]></tex-math></inline-formula>, reported by the Belle Collaboration, is the second enhancement observed in the <inline-formula><tex-math notation="LaTeX" id="ImEquation265"><![CDATA[$\gamma \gamma$]]></tex-math></inline-formula> fusion process. As indicated in Ref. [<xref ref-type="bibr" rid="C4">4</xref>], <inline-formula><tex-math notation="LaTeX" id="ImEquation266"><![CDATA[$X(3915)$]]></tex-math></inline-formula> is a good candidate for <inline-formula><tex-math notation="LaTeX" id="ImEquation267"><![CDATA[$\chi _{c0}^\prime (2P)$]]></tex-math></inline-formula>, i.e., the first radial excitation of <inline-formula><tex-math notation="LaTeX" id="ImEquation268"><![CDATA[$\chi _{c0}(3414)$]]></tex-math></inline-formula>. Besides its open-charm decay, study of the hidden-charm decay of <inline-formula><tex-math notation="LaTeX" id="ImEquation269"><![CDATA[$X(3915)$]]></tex-math></inline-formula> will provide a key hint to understanding the properties of <inline-formula><tex-math notation="LaTeX" id="ImEquation270"><![CDATA[$X(3915)$]]></tex-math></inline-formula> and further test the P-wave charmonium explanation of <inline-formula><tex-math notation="LaTeX" id="ImEquation271"><![CDATA[$X(3915)$]]></tex-math></inline-formula> in Ref. [<xref ref-type="bibr" rid="C4">4</xref>]. Since the mass of <inline-formula><tex-math notation="LaTeX" id="ImEquation272"><![CDATA[$X(3915)$]]></tex-math></inline-formula> is above the threshold of <inline-formula><tex-math notation="LaTeX" id="ImEquation273"><![CDATA[$D\bar D$]]></tex-math></inline-formula> and dominantly decays into <inline-formula><tex-math notation="LaTeX" id="ImEquation274"><![CDATA[$D\bar {D}$]]></tex-math></inline-formula>, hadronic loop effects [<xref ref-type="bibr" rid="C6">6</xref>&#x02013;<xref ref-type="bibr" rid="C13">13</xref>] will play an important role in the hidden-charm decay <inline-formula><tex-math notation="LaTeX" id="ImEquation275"><![CDATA[$X(3915)\to J/\psi \omega$]]></tex-math></inline-formula>, which, in fact, results from the coupled-channel effects. In this work, we have performed the calculation of the <inline-formula><tex-math notation="LaTeX" id="ImEquation276"><![CDATA[$X(3915)\to J/\psi \omega$]]></tex-math></inline-formula> processes.</p>
<p>Before the observation of <inline-formula><tex-math notation="LaTeX" id="ImEquation277"><![CDATA[$X(3915)$]]></tex-math></inline-formula>, Belle reported a state named <inline-formula><tex-math notation="LaTeX" id="ImEquation278"><![CDATA[$Z(3930)$]]></tex-math></inline-formula> in <inline-formula><tex-math notation="LaTeX" id="ImEquation279"><![CDATA[$\gamma \gamma$]]></tex-math></inline-formula> fusion [<xref ref-type="bibr" rid="C2">2</xref>, <xref ref-type="bibr" rid="C3">3</xref>], which is also a P-wave charmonium state of the first radial excitation. <inline-formula><tex-math notation="LaTeX" id="ImEquation280"><![CDATA[$Z(3930)$]]></tex-math></inline-formula> should decay into <inline-formula><tex-math notation="LaTeX" id="ImEquation281"><![CDATA[$J/\psi \omega$]]></tex-math></inline-formula>, which seems to indicate that there should exist two peaks close to each other in the <inline-formula><tex-math notation="LaTeX" id="ImEquation282"><![CDATA[$J/\psi \omega$]]></tex-math></inline-formula> invariant mass spectrum given by Belle [<xref ref-type="bibr" rid="C1">1</xref>]. However, currently, only one structure corresponding to <inline-formula><tex-math notation="LaTeX" id="ImEquation283"><![CDATA[$X(3915)$]]></tex-math></inline-formula> has been observed [<xref ref-type="bibr" rid="C1">1</xref>]. In order to explain this contradiction, in this work we have further studied <inline-formula><tex-math notation="LaTeX" id="ImEquation284"><![CDATA[$Z(3930)\to J/\psi \omega$]]></tex-math></inline-formula> by the intermediate states <inline-formula><tex-math notation="LaTeX" id="ImEquation285"><![CDATA[$D\bar {D}$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation286"><![CDATA[$D\bar {D}^{\ast }+ \hbox {h.c.}$]]></tex-math></inline-formula> The results illustrated in Fig. <xref ref-type="fig" rid="F2">2</xref> show that the partial decay width of <inline-formula><tex-math notation="LaTeX" id="ImEquation287"><![CDATA[$Z(3930)\to J/\psi \omega$]]></tex-math></inline-formula> is suppressed when compared with that of <inline-formula><tex-math notation="LaTeX" id="ImEquation288"><![CDATA[$X(3915)\to J/\psi \omega$]]></tex-math></inline-formula>, which explains why <inline-formula><tex-math notation="LaTeX" id="ImEquation289"><![CDATA[$Z(3930)$]]></tex-math></inline-formula> cannot be observed in the <inline-formula><tex-math notation="LaTeX" id="ImEquation290"><![CDATA[$J/\psi \omega$]]></tex-math></inline-formula> invariant mass spectrum.</p>
<p>As more charmonium-like states are observed in the <inline-formula><tex-math notation="LaTeX" id="ImEquation291"><![CDATA[$\gamma \gamma$]]></tex-math></inline-formula> fusion process [<xref ref-type="bibr" rid="C1">1</xref>&#x02013;<xref ref-type="bibr" rid="C3">3</xref>, <xref ref-type="bibr" rid="C25">25</xref>], they provide us with a better chance to explore the properties of these states, especially P-wave charmonium states [<xref ref-type="bibr" rid="C4">4</xref>]. The study of the hidden-charm decay of <inline-formula><tex-math notation="LaTeX" id="ImEquation292"><![CDATA[$X(3915)$]]></tex-math></inline-formula> in this work supports the proposal of <inline-formula><tex-math notation="LaTeX" id="ImEquation293"><![CDATA[$\chi _{c0}^\prime (2P)$]]></tex-math></inline-formula> assignment to <inline-formula><tex-math notation="LaTeX" id="ImEquation294"><![CDATA[$X(3915)$]]></tex-math></inline-formula> in Ref. [<xref ref-type="bibr" rid="C4">4</xref>]. Besides applying the hidden-charm and open-charm decays of <inline-formula><tex-math notation="LaTeX" id="ImEquation295"><![CDATA[$X(3915)$]]></tex-math></inline-formula> to test the <inline-formula><tex-math notation="LaTeX" id="ImEquation296"><![CDATA[$\chi _{c0}^\prime$]]></tex-math></inline-formula> assignment to <inline-formula><tex-math notation="LaTeX" id="ImEquation297"><![CDATA[$X(3915)$]]></tex-math></inline-formula>, we suggest that an angular distribution analysis of <inline-formula><tex-math notation="LaTeX" id="ImEquation298"><![CDATA[$X(3915)$]]></tex-math></inline-formula> in future experiments will be valuable to test the <inline-formula><tex-math notation="LaTeX" id="ImEquation299"><![CDATA[$\chi _{c0}^\prime (2P)$]]></tex-math></inline-formula> explanation of <inline-formula><tex-math notation="LaTeX" id="ImEquation300"><![CDATA[$X(3915)$]]></tex-math></inline-formula>, since the <inline-formula><tex-math notation="LaTeX" id="ImEquation301"><![CDATA[$J^{PC}$]]></tex-math></inline-formula> quantum number of <inline-formula><tex-math notation="LaTeX" id="ImEquation302"><![CDATA[$X(3915)$]]></tex-math></inline-formula> must be <inline-formula><tex-math notation="LaTeX" id="ImEquation303"><![CDATA[$0^{+ + }$]]></tex-math></inline-formula>. Although <inline-formula><tex-math notation="LaTeX" id="ImEquation304"><![CDATA[$Z(3930)$]]></tex-math></inline-formula> is well established as a <inline-formula><tex-math notation="LaTeX" id="ImEquation305"><![CDATA[$\chi _{c2}^\prime (2P)$]]></tex-math></inline-formula> state [<xref ref-type="bibr" rid="C2">2</xref>, <xref ref-type="bibr" rid="C3">3</xref>], its hidden-charm decay behavior was unclear before this work. Performing the calculation of <inline-formula><tex-math notation="LaTeX" id="ImEquation306"><![CDATA[$Z(3930)\to J/\psi \omega$]]></tex-math></inline-formula> by the hadronic loop mechanism, we further learn that the branching ratio of <inline-formula><tex-math notation="LaTeX" id="ImEquation307"><![CDATA[$Z(3930)\to J/\psi \omega$]]></tex-math></inline-formula> is at least one order smaller than that of <inline-formula><tex-math notation="LaTeX" id="ImEquation308"><![CDATA[$X(3915)\to J/\psi \omega$]]></tex-math></inline-formula>, which not only successfully explains the appearance of only one enhancement, <inline-formula><tex-math notation="LaTeX" id="ImEquation309"><![CDATA[$X(3915)$]]></tex-math></inline-formula>, in the <inline-formula><tex-math notation="LaTeX" id="ImEquation310"><![CDATA[$J/\psi \omega$]]></tex-math></inline-formula> invariant mass spectrum but also tests the hadronic loop effects, which is an important non-perturbative mechanism in the decays of charmonium or charmonium-like states [<xref ref-type="bibr" rid="C6">6</xref>&#x02013;<xref ref-type="bibr" rid="C13">13</xref>].</p>
</sec>
<sec id="s2"><title>Funding</title>
<p>Open Access funding: <grant-sponsor>SCOAP<sup>3</sup></grant-sponsor>.</p>
</sec>
</body>
<back>
<ack>
<title>Acknowledgements</title>
<p>This project is supported by the National Natural Science Foundation of China under Grant Nos. 11175073, 11005129, 11375240, 11035006, the Ministry of Education of China (FANEDD under Grant No. 200924, DPFIHE under Grant No. 20090211120029, NCET, the Fundamental Research Funds for the Central Universities), the Fok Ying Tung Education Foundation (No. 131006), and the West Doctoral Project of the Chinese Academy of Sciences.</p>
</ack>
<ref-list><title>References</title>
<ref id="C1"><label>1</label><citation citation-type="journal"><person-group person-group-type="author"><name><surname>Uehara</surname><given-names>S.</given-names></name></person-group> <collab>[Belle Collaboration]</collab>, <source>Phys. Rev. Lett.</source> <volume>104</volume>, <fpage>092001</fpage> (<year>2010</year>) [<elocation-id content-type="arxiv">arXiv:0912.4451</elocation-id> <comment>[hep-ex]</comment>] [<comment><ext-link xlink:href="http://inspirehep.net/search?p=find+EPRINT+arXiv:0912.4451">Search inSPIRE</ext-link></comment>]. <comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevLett.104.092001">doi:10.1103/PhysRevLett.104.092001</ext-link>)</comment></citation></ref>
<ref id="C2"><label>2</label><citation citation-type="journal"><person-group person-group-type="author"><name><surname>Uehara</surname><given-names>S.</given-names></name><etal/></person-group> <collab>[Belle Collaboration]</collab>, <source>Phys. Rev. Lett.</source> <volume>96</volume>, <fpage>082003</fpage> (<year>2006</year>) [<elocation-id content-type="arxiv">arXiv:0512035</elocation-id> <comment>[hep-ex]</comment>] [<comment><ext-link xlink:href="http://inspirehep.net/search?p=find+EPRINT+arXiv:0512035">Search inSPIRE</ext-link></comment>]. <comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevLett.96.082003">doi:10.1103/PhysRevLett.96.082003</ext-link>)</comment></citation></ref>
<ref id="C3"><label>3</label><citation citation-type="journal"><person-group person-group-type="author"><name><surname>Aubert</surname><given-names>B.</given-names></name><etal/></person-group> <collab>[BaBar Collaboration]</collab>, <source>Phys. Rev. D</source> <volume>81</volume>, <fpage>092003</fpage> (<year>2010</year>) [<elocation-id content-type="arxiv">arXiv:1002.0281</elocation-id> <comment>[hep-ex]</comment>] [<comment><ext-link xlink:href="http://inspirehep.net/search?p=find+EPRINT+arXiv:1002.0281">Search inSPIRE</ext-link></comment>]. <comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.81.092003">doi:10.1103/PhysRevD.81.092003</ext-link>)</comment></citation></ref>
<ref id="C4"><label>4</label><citation citation-type="journal"><person-group person-group-type="author"><name><surname>Liu</surname><given-names>X.</given-names></name><name><surname>Luo</surname><given-names>Z. G.</given-names></name><name><surname>Sun</surname><given-names>Z. F.</given-names></name></person-group>, <source>Phys. Rev. Lett.</source> <volume>104</volume>, <fpage>122001</fpage> (<year>2010</year>) [<elocation-id content-type="arxiv">arXiv:0911.3694</elocation-id> <comment>[hep-ph]</comment>] [<comment><ext-link xlink:href="http://inspirehep.net/search?p=find+EPRINT+arXiv:0911.3694">Search inSPIRE</ext-link></comment>]. <comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevLett.104.122001">doi:10.1103/PhysRevLett.104.122001</ext-link>)</comment></citation></ref>
<ref id="C5"><label>5</label><citation citation-type="journal"><person-group person-group-type="author"><name><surname>Lees</surname><given-names>J. P.</given-names></name><etal/></person-group> <collab>[BaBar Collaboration]</collab>, <source>Phys. Rev. D</source> <volume>86</volume>, <fpage>072002</fpage> (<year>2012</year>) [<elocation-id content-type="arxiv">arXiv:1207.2651</elocation-id> <comment>[hep-ex]</comment>] [<comment><ext-link xlink:href="http://inspirehep.net/search?p=find+EPRINT+arXiv:1207.2651">Search inSPIRE</ext-link></comment>]. <comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.86.072002">doi:10.1103/PhysRevD.86.072002</ext-link>)</comment></citation></ref>
<ref id="C6"><label>6</label><citation citation-type="journal"><person-group person-group-type="author"><name><surname>Liu</surname><given-names>X.</given-names></name><name><surname>Zhang</surname><given-names>B.</given-names></name><name><surname>Zhu</surname><given-names>S. L.</given-names></name></person-group>, <source>Phys. Lett. B</source> <volume>645</volume>, <fpage>185</fpage> (<year>2007</year>) [<elocation-id content-type="arxiv">arXiv:0610278</elocation-id> <comment>[hep-ph]</comment>] [<comment><ext-link xlink:href="http://inspirehep.net/search?p=find+EPRINT+arXiv:0610278">Search inSPIRE</ext-link></comment>]. <comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1016/j.physletb.2006.12.031">doi:10.1016/j.physletb.2006.12.031</ext-link>)</comment></citation></ref>
<ref id="C7"><label>7</label><citation citation-type="journal"><person-group person-group-type="author"><name><surname>Liu</surname><given-names>X.</given-names></name></person-group>, <source>Eur. Phys. J. C</source> <volume>54</volume>, <fpage>471</fpage> (<year>2008</year>) <elocation-id content-type="arxiv">arXiv:0708.4167</elocation-id> <comment>[hep-ph]</comment>. <comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1140/epjc/s10052-008-0551-4">doi:10.1140/epjc/s10052-008-0551-4</ext-link>)</comment></citation></ref>
<ref id="C8"><label>8</label><citation citation-type="journal"><person-group person-group-type="author"><name><surname>Liu</surname><given-names>X.</given-names></name><name><surname>Zhang</surname><given-names>B.</given-names></name><name><surname>Zhu</surname><given-names>S. L.</given-names></name></person-group>, <source>Phys. Rev. D</source> <volume>77</volume>, <fpage>114021</fpage> (<year>2008</year>) <elocation-id content-type="arxiv">arXiv:0803.4270</elocation-id> [hep-ph]. <comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.77.114021">doi:10.1103/PhysRevD.77.114021</ext-link>)</comment></citation></ref>
<ref id="C9"><label>9</label><citation citation-type="journal"><person-group person-group-type="author"><name><surname>Liu</surname><given-names>X.</given-names></name></person-group>, <source>Phys. Lett. B</source> <volume>680</volume>, <fpage>137</fpage> (<year>2009</year>) <elocation-id content-type="arxiv">arXiv:0904.0136</elocation-id> <comment>[hep-ph]</comment>. <comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1016/j.physletb.2009.08.049">doi:10.1016/j.physletb.2009.08.049</ext-link>)</comment></citation></ref>
<ref id="C10"><label>10</label><citation citation-type="other"><person-group person-group-type="author"><name><surname>Meng</surname><given-names>C.</given-names></name><name><surname>Chao</surname><given-names>K. T.</given-names></name></person-group>, <elocation-id content-type="arxiv">arXiv:0708.4222</elocation-id> [hep-ph].</citation></ref>
<ref id="C11"><label>11</label><citation citation-type="journal"><person-group person-group-type="author"><name><surname>Liu</surname><given-names>X.</given-names></name><name><surname>Zeng</surname><given-names>X. Q.</given-names></name><name><surname>Li</surname><given-names>X. Q.</given-names></name></person-group>, <source>Phys. Rev. D</source> <volume>74</volume>, <fpage>074003</fpage> (<year>2006</year>) [<elocation-id content-type="arxiv">arXiv:0606191</elocation-id> <comment>[hep-ph]</comment>] [<comment><ext-link xlink:href="http://inspirehep.net/search?p=find+EPRINT+arXiv:0606191">Search inSPIRE</ext-link></comment>]. <comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.74.074003">doi:10.1103/PhysRevD.74.074003</ext-link>)</comment></citation></ref>
<ref id="C12"><label>12</label><citation citation-type="journal"><person-group person-group-type="author"><name><surname>Liu</surname><given-names>X.</given-names></name><name><surname>Zhang</surname><given-names>B.</given-names></name><name><surname>Li</surname><given-names>X. Q.</given-names></name></person-group>, <source>Phys. Lett. B</source> <volume>675</volume>, <fpage>441</fpage> (<year>2009</year>) [<elocation-id content-type="arxiv">arXiv:0902.0480</elocation-id> <comment>[hep-ph]</comment>] [<comment><ext-link xlink:href="http://inspirehep.net/search?p=find+EPRINT+arXiv:0902.0480">Search inSPIRE</ext-link></comment>]. <comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1016/j.physletb.2009.04.047">doi:10.1016/j.physletb.2009.04.047</ext-link>)</comment></citation></ref>
<ref id="C13"><label>13</label><citation citation-type="journal"><person-group person-group-type="author"><name><surname>Chen</surname><given-names>D.-Y.</given-names></name><name><surname>He</surname><given-names>J.</given-names></name><name><surname>Li</surname><given-names>X.-Q.</given-names></name><name><surname>Liu</surname><given-names>X.</given-names></name></person-group>, <source>Phys. Rev. D</source> <volume>81</volume>, <fpage>074006</fpage> (<year>2010</year>) [<elocation-id content-type="arxiv">arXiv:0912.4860</elocation-id> <comment>[hep-ph]</comment>] [<comment><ext-link xlink:href="http://inspirehep.net/search?p=find+EPRINT+arXiv:0912.4860">Search inSPIRE</ext-link></comment>]. <comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.81.074006">doi:10.1103/PhysRevD.81.074006</ext-link>)</comment></citation></ref>
<ref id="C14"><label>14</label><citation citation-type="journal"><person-group person-group-type="author"><name><surname>Colangelo</surname><given-names>P.</given-names></name><name><surname>De Fazio</surname><given-names>F.</given-names></name><name><surname>Pham</surname><given-names>T. N.</given-names></name></person-group>, <source>Phys. Rev. D</source> <volume>69</volume>, <fpage>054023</fpage> (<year>2004</year>) [<elocation-id content-type="arxiv">arXiv:0310084</elocation-id> <comment>[hep-ph]</comment>] [<comment><ext-link xlink:href="http://inspirehep.net/search?p=find+EPRINT+arXiv:0310084">Search inSPIRE</ext-link></comment>]. <comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.69.054023">doi:10.1103/PhysRevD.69.054023</ext-link>)</comment></citation></ref>
<ref id="C15"><label>15</label><citation citation-type="journal"><person-group person-group-type="author"><name><surname>Casalbuoni</surname><given-names>R.</given-names></name><name><surname>Deandrea</surname><given-names>A.</given-names></name><name><surname>Di Bartolomeo</surname><given-names>N.</given-names></name><name><surname>Gatto</surname><given-names>R.</given-names></name><name><surname>Feruglio</surname><given-names>F.</given-names></name><name><surname>Nardulli</surname><given-names>G.</given-names></name></person-group>, <source>Phys. Rept.</source> <volume>281</volume>, <fpage>145</fpage> (<year>1997</year>) [<elocation-id content-type="arxiv">arXiv:9605342</elocation-id> <comment>[hep-ph]</comment>] [<comment><ext-link xlink:href="http://inspirehep.net/search?p=find+EPRINT+arXiv:9605342">Search inSPIRE</ext-link></comment>]. <comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1016/S0370-1573(96)00027-0">doi:10.1016/S0370-1573(96)00027-0</ext-link>)</comment></citation></ref>
<ref id="C16"><label>16</label><citation citation-type="journal"><person-group person-group-type="author"><name><surname>Oh</surname><given-names>Y. S.</given-names></name><name><surname>Song</surname><given-names>T.</given-names></name><name><surname>Lee</surname><given-names>S. H.</given-names></name></person-group>, <source>Phys. Rev. C</source> <volume>63</volume>, <fpage>034901</fpage> (<year>2001</year>) <comment>[<uri xlink:href="http://arxiv.org/abs/nucl-th/0010064">http://arxiv.org/abs/nucl-th/0010064</uri>]</comment>. <comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevC.63.034901">doi:10.1103/PhysRevC.63.034901</ext-link>)</comment></citation></ref>
<ref id="C17"><label>17</label><citation citation-type="journal"><person-group person-group-type="author"><name><surname>Isola</surname><given-names>C.</given-names></name><name><surname>Ladisa</surname><given-names>M.</given-names></name><name><surname>Nardulli</surname><given-names>G.</given-names></name><name><surname>Santorelli</surname><given-names>P.</given-names></name></person-group>, <source>Phys. Rev. D</source> <volume>68</volume>, <fpage>114001</fpage> (<year>2003</year>) [<elocation-id content-type="arxiv">arXiv:0307367</elocation-id> <comment>[hep-ph]</comment>] [<comment><ext-link xlink:href="http://inspirehep.net/search?p=find+EPRINT+arXiv:0307367">Search inSPIRE</ext-link></comment>]. <comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.68.114001">doi:10.1103/PhysRevD.68.114001</ext-link>)</comment></citation></ref>
<ref id="C18"><label>18</label><citation citation-type="journal"><person-group person-group-type="author"><name><surname>Cheng</surname><given-names>H. Y.</given-names></name><name><surname>Chua</surname><given-names>C. K.</given-names></name><name><surname>Soni</surname><given-names>A.</given-names></name></person-group>, <source>Phys. Rev. D</source> <volume>71</volume>, <fpage>014030</fpage> (<year>2005</year>) [<elocation-id content-type="arxiv">arXiv:0409317</elocation-id> <comment>[hep-ph]</comment>] [<comment><ext-link xlink:href="http://inspirehep.net/search?p=find+EPRINT+arXiv:0409317">Search inSPIRE</ext-link></comment>]. <comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.71.014030">doi:10.1103/PhysRevD.71.014030</ext-link>)</comment></citation></ref>
<ref id="C19"><label>19</label><citation citation-type="journal"><person-group person-group-type="author"><name><surname>Liu</surname><given-names>X. H.</given-names></name><name><surname>Zhao</surname><given-names>Q.</given-names></name></person-group>, <source>Phys. Rev. D</source> <volume>81</volume>, <fpage>014017</fpage> (<year>2010</year>) [<elocation-id content-type="arxiv">arXiv:0912.1508</elocation-id> <comment>[hep-ph]</comment>] [<comment><ext-link xlink:href="http://inspirehep.net/search?p=find+EPRINT+arXiv:0912.1508">Search inSPIRE</ext-link></comment>]. <comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.81.014017">doi:10.1103/PhysRevD.81.014017</ext-link>)</comment></citation></ref>
<ref id="C20"><label>20</label><citation citation-type="journal"><person-group person-group-type="author"><name><surname>Godfrey</surname><given-names>S.</given-names></name><name><surname>Isgur</surname><given-names>N.</given-names></name></person-group>, <source>Phys. Rev. D</source> <volume>32</volume>, <fpage>189</fpage> (<year>1985</year>). <comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.32.189">doi:10.1103/PhysRevD.32.189</ext-link>)</comment></citation></ref>
<ref id="C21"><label>21</label><citation citation-type="journal"><person-group person-group-type="author"><name><surname>Munz</surname><given-names>C. R.</given-names></name></person-group>, <source>Nucl. Phys. A</source> <volume>609</volume>, <fpage>364</fpage> (<year>1996</year>) [<elocation-id content-type="arxiv">arXiv:9601206</elocation-id> <comment>[hep-ph]</comment>] [<comment><ext-link xlink:href="http://inspirehep.net/search?p=find+EPRINT+arXiv:9601206">Search inSPIRE</ext-link></comment>]. <comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1016/S0375-9474(96)00265-5">doi:10.1016/S0375-9474(96)00265-5</ext-link>)</comment></citation></ref>
<ref id="C22"><label>22</label><citation citation-type="journal"><person-group person-group-type="author"><name><surname>Ebert</surname><given-names>D.</given-names></name><name><surname>Faustov</surname><given-names>R. N.</given-names></name><name><surname>Galkin</surname><given-names>V. O.</given-names></name></person-group>, <source>Mod. Phys. Lett. A</source> <volume>18</volume>, <fpage>601</fpage> (<year>2003</year>) [<elocation-id content-type="arxiv">arXiv:0302044</elocation-id> <comment>[hep-ph]</comment>] [<comment><ext-link xlink:href="http://inspirehep.net/search?p=find+EPRINT+arXiv:0302044">Search inSPIRE</ext-link></comment>]. <comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1142/S021773230300971X">doi:10.1142/S021773230300971X</ext-link>)</comment></citation></ref>
<ref id="C23"><label>23</label><citation citation-type="journal"><person-group person-group-type="author"><name><surname>Hwang</surname><given-names>C.-W.</given-names></name><name><surname>Guo</surname><given-names>R.-S.</given-names></name></person-group>, <source>Phys. Rev. D</source> <volume>82</volume>, <fpage>034021</fpage> (<year>2010</year>) [<elocation-id content-type="arxiv">arXiv:1005.2811</elocation-id> <comment>[hep-ph]</comment>] [<comment><ext-link xlink:href="http://inspirehep.net/search?p=find+EPRINT+arXiv:1005.2811">Search inSPIRE</ext-link></comment>]. <comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.82.034021">doi:10.1103/PhysRevD.82.034021</ext-link>)</comment></citation></ref>
<ref id="C24"><label>24</label><citation citation-type="journal"><person-group person-group-type="author"><name><surname>Wang</surname><given-names>G.-L.</given-names></name></person-group>, <source>Phys. Lett. B</source> <volume>653</volume>, <fpage>206</fpage> (<year>2007</year>) [<elocation-id content-type="arxiv">arXiv:0708.3516</elocation-id> <comment>[hep-ph]</comment>] [<comment><ext-link xlink:href="http://inspirehep.net/search?p=find+EPRINT+arXiv:0708.3516">Search inSPIRE</ext-link></comment>]. <comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1016/j.physletb.2007.08.017">doi:10.1016/j.physletb.2007.08.017</ext-link>)</comment></citation></ref>
<ref id="C25"><label>25</label><citation citation-type="journal"><person-group person-group-type="author"><name><surname>Shen</surname><given-names>C. P.</given-names></name><etal/></person-group> <collab>[Belle Collaboration]</collab>, <source>Phys. Rev. Lett.</source> <volume>104</volume>, <fpage>112004</fpage> (<year>2010</year>) [<elocation-id content-type="arxiv">arXiv:0912.2383</elocation-id> <comment>[hep-ex]</comment>] [<comment><ext-link xlink:href="http://inspirehep.net/search?p=find+EPRINT+arXiv:0912.2383">Search inSPIRE</ext-link></comment>]. <comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevLett.104.112004">doi:10.1103/PhysRevLett.104.112004</ext-link>)</comment></citation></ref>
<ref id="C26"><label>26</label><citation citation-type="journal"><person-group person-group-type="author"><name><surname>Chen</surname><given-names>D. Y.</given-names></name><name><surname>Liu</surname><given-names>X.</given-names></name><name><surname>Matsuki</surname><given-names>T.</given-names></name></person-group>, <source>Phys. Rev. D</source> <volume>87</volume>, <fpage>054006</fpage> (<year>2013</year>) [<elocation-id content-type="arxiv">arXiv:1209.0064</elocation-id> <comment>[hep-ph]</comment>] [<comment><ext-link xlink:href="http://inspirehep.net/search?p=find+EPRINT+arXiv:1209.0064">Search inSPIRE</ext-link></comment>]. <comment>(<ext-link ext-link-type="uri" xlink:href="http://dx.doi.org/10.1103/PhysRevD.87.054006">doi:10.1103/PhysRevD.87.054006</ext-link>)</comment></citation></ref>
</ref-list>
</back>
</article>