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<front>
<journal-meta>
<journal-id journal-id-type="publisher-id">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/ptx154</article-id>
<article-id pub-id-type="publisher-id">ptx154</article-id>
<article-id pub-id-type="arxiv">arXiv:1708.08657</article-id>
<article-categories>
<subj-group subj-group-type="category-toc-heading">
<subject>Papers</subject>
<subj-group subj-group-type="category-toc-heading">
<subject>Theoretical Particle Physics</subject>
</subj-group>
</subj-group>
<subj-group subj-group-type="category-journal-collection">
<subject>PTEP/B04</subject>
<subject>PTEP/B21</subject>
</subj-group>
</article-categories>
<title-group>
<article-title>Correlators in higher-spin AdS<sub>3</sub> holography from Wilson lines with loop corrections</article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author" corresp="yes">
<name><surname>Hikida</surname><given-names>Yasuaki</given-names></name>
<xref ref-type="aff" rid="AFF1"/>
<xref ref-type="corresp" rid="COR1"/>
<email xlink:type="simple">yhikida@yukawa.kyoto-u.ac.jp</email>
</contrib>
<contrib contrib-type="author" corresp="yes">
<name><surname>Uetoko</surname><given-names>Takahiro</given-names></name>
<xref ref-type="aff" rid="AFF2"/>
<xref ref-type="corresp" rid="COR1"/>
<email xlink:type="simple">rp0019fr@ed.ritsumei.ac.jp</email>
</contrib>
</contrib-group>
<aff id="AFF1"><label>1</label><italic>Center for Gravitational Physics, Yukawa Institute for Theoretical Physics, Kyoto University, Kyoto 606-8502, Japan</italic></aff>
<aff id="AFF2"><label>2</label><italic>Department of Physical Sciences, College of Science and Engineering, Ritsumeikan University, Shiga 525-8577, Japan</italic></aff>
<author-notes>
<corresp id="COR1"><label>*</label>E-mail: <email>yhikida@yukawa.kyoto-u.ac.jp</email>; <email>rp0019fr@ed.ritsumei.ac.jp</email></corresp>
</author-notes>
<pub-date pub-type="cover">
<month>11</month>
<year>2017</year>
</pub-date>
<pub-date pub-type="collection">
<day>01</day>
<month>11</month>
<year>2017</year>
</pub-date>
<pub-date pub-type="epub" iso-8601-date="2017-11-29">
<day>29</day>
<month>11</month>
<year>2017</year>
</pub-date>
<volume>2017</volume>
<issue>11</issue>
<elocation-id>113B03</elocation-id>
<history>
<date date-type="received">
<day>12</day>
<month>9</month>
<year>2017</year>
</date>
<date date-type="rev-recd">
<day>19</day>
<month>10</month>
<year>2017</year>
</date>
<date date-type="accepted">
<day>21</day>
<month>10</month>
<year>2017</year>
</date>
</history>
<permissions>
<copyright-statement>&#x00A9; The Author(s) 2017. Published by Oxford University Press on behalf of the Physical Society of Japan.</copyright-statement>
<copyright-year>2017</copyright-year>
<license license-type="cc-by" 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 ext-link-type="uri" xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://creativecommons.org/licenses/by/4.0/">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 xlink:href="ptx154.pdf"/>
<abstract abstract-type="abstract"><title>Abstract</title>
<p>We study the correlators of the 2D W<inline-formula><tex-math notation="LaTeX" id="ImEquation2"><![CDATA[$_N$]]></tex-math></inline-formula> minimal model in the semiclassical regime with large central charge from the bulk viewpoint by utilizing open Wilson lines in <inline-formula><tex-math notation="LaTeX" id="ImEquation3"><![CDATA[$\text{sl}(N) $]]></tex-math></inline-formula> Chern&#x2013;Simons gauge theory. We extend previous works for the tree level of bulk theory to incorporate loop corrections in this paper. We offer a way to regularize divergences associated with loop diagrams such that three-point functions with two scalars and a higher-spin current agree with the values fixed by the boundary W<inline-formula><tex-math notation="LaTeX" id="ImEquation4"><![CDATA[$_N$]]></tex-math></inline-formula> symmetry. With the prescription, we reproduce the conformal weight of the operator corresponding to a bulk scalar up to two-loop order for explicit examples with <inline-formula><tex-math notation="LaTeX" id="ImEquation5"><![CDATA[$N=2,3$]]></tex-math></inline-formula>.</p>
</abstract>
<kwd-group kwd-group-type="jel">
<kwd>B04</kwd>
<kwd>B21</kwd>
</kwd-group>
<counts>
<page-count count="28"/>
</counts>
</article-meta>
</front>
<body>
<sec sec-type="intro" id="SEC1"><title>1. Introduction</title>
<p>In Ref. [<xref ref-type="bibr" rid="B1">1</xref>] we computed three-point functions with two scalar operators and a higher-spin current in the 2D W<inline-formula><tex-math notation="LaTeX" id="ImEquation6"><![CDATA[$_N$]]></tex-math></inline-formula> minimal model with <inline-formula><tex-math notation="LaTeX" id="ImEquation7"><![CDATA[$1/N$]]></tex-math></inline-formula> corrections. The main aim of this paper is to give a bulk interpretation of the conformal field theory results.<xref ref-type="fn" rid="FN1"><sup>1</sup></xref> The <inline-formula><tex-math notation="LaTeX" id="ImEquation8"><![CDATA[$1/N$]]></tex-math></inline-formula> corrections (or <inline-formula><tex-math notation="LaTeX" id="ImEquation9"><![CDATA[$1/c$]]></tex-math></inline-formula> corrections with <inline-formula><tex-math notation="LaTeX" id="ImEquation10"><![CDATA[$c$]]></tex-math></inline-formula> as the central charge) in the minimal model should be interpreted as loop corrections in the bulk gravity description. However, it is notoriously difficult to deal with divergences associated with gravitational loop diagrams in general. Applying holography, it is expected that boundary theory can define bulk quantum theory of gravity generically. For our case, the minimal model would determine the way to regularize these gravitational divergences, and we would like to show that this is indeed the case in this paper.</p>
<p>The 2D W<inline-formula><tex-math notation="LaTeX" id="ImEquation11"><![CDATA[$_N$]]></tex-math></inline-formula> minimal model has a coset description as
<disp-formula id="ptx154-M1"><label>(1)</label><tex-math notation="LaTeX" id="Equation1"><![CDATA[
\begin{align}
\frac{\text{su}(N)_k \oplus \text{su}(N)_1 }{ \text{su}(N)_{k+1} }
\label{coset}
\end{align}
]]></tex-math></disp-formula>
with the central charge
<disp-formula id="ptx154-M2"><label>(2)</label><tex-math notation="LaTeX" id="Equation2"><![CDATA[
\begin{align}
c = (N-1) \left( 1 - \frac{N(N+1)}{(k+N) (k+N+1)}\right).
\label{central}
\end{align}
]]></tex-math></disp-formula></p>
<p>In Ref. [<xref ref-type="bibr" rid="B11">11</xref>] the &#x2019;t Hooft limit with large <inline-formula><tex-math notation="LaTeX" id="ImEquation12"><![CDATA[$N$]]></tex-math></inline-formula> but finite <inline-formula><tex-math notation="LaTeX" id="ImEquation13"><![CDATA[$\lambda = N/(k+N)$]]></tex-math></inline-formula> of the minimal model is conjectured to be dual to the classical 3D Prokushkin&#x2013;Vasiliev theory of Ref. [<xref ref-type="bibr" rid="B12">12</xref>]. Instead of the &#x2019;t Hooft limit, we consider the semiclassical regime with large <inline-formula><tex-math notation="LaTeX" id="ImEquation14"><![CDATA[$c$]]></tex-math></inline-formula> but finite <inline-formula><tex-math notation="LaTeX" id="ImEquation15"><![CDATA[$N$]]></tex-math></inline-formula>. The bulk description for the semiclassical regime is supposed to be given by Chern&#x2013;Simons gauge theory based on <inline-formula><tex-math notation="LaTeX" id="ImEquation16"><![CDATA[$\text{sl}(N) \oplus \text{sl} (N)$]]></tex-math></inline-formula> dressed by perturbative matters [<xref ref-type="bibr" rid="B13">13</xref>&#x2013;<xref ref-type="bibr" rid="B15">15</xref>]. The large-<inline-formula><tex-math notation="LaTeX" id="ImEquation17"><![CDATA[$c$]]></tex-math></inline-formula> regime should be realized with a negative level <inline-formula><tex-math notation="LaTeX" id="ImEquation18"><![CDATA[$k = -1 - N + \mathcal{O}(c^{-1})$]]></tex-math></inline-formula>, thus the conformal field theory is non-unitary in the regime.<xref ref-type="fn" rid="FN2"><sup>2</sup></xref> In Ref. [<xref ref-type="bibr" rid="B1">1</xref>] we evaluated correlators at the &#x2019;t Hooft limit with <inline-formula><tex-math notation="LaTeX" id="ImEquation19"><![CDATA[$1/N$]]></tex-math></inline-formula> corrections, but the results can be generalized for the semiclassical limit with <inline-formula><tex-math notation="LaTeX" id="ImEquation20"><![CDATA[$1/c$]]></tex-math></inline-formula> corrections. We try to interpret the <inline-formula><tex-math notation="LaTeX" id="ImEquation21"><![CDATA[$1/c$]]></tex-math></inline-formula> corrections in terms of <inline-formula><tex-math notation="LaTeX" id="ImEquation22"><![CDATA[$\text{sl}(N) $]]></tex-math></inline-formula> Chern&#x2013;Simons gauge theory.</p>
<p>The W<inline-formula><tex-math notation="LaTeX" id="ImEquation23"><![CDATA[$_N$]]></tex-math></inline-formula> symmetry of the minimal model is generated by higher-spin currents <inline-formula><tex-math notation="LaTeX" id="ImEquation24"><![CDATA[$J^{(s)} (z)$]]></tex-math></inline-formula> with <inline-formula><tex-math notation="LaTeX" id="ImEquation25"><![CDATA[$s=2,3,\ldots,N$]]></tex-math></inline-formula>. We examine the following two- and three-point functions as
<disp-formula id="ptx154-M3"><label>(3)</label><tex-math notation="LaTeX" id="Equation3"><![CDATA[
\begin{align}
\langle \mathcal{O}_{h_+} (z_1) \bar{\mathcal{O}}_{h_+} (z_2) \rangle \, , \quad
\langle \mathcal{O}_{h_+} (z_1) \bar{\mathcal{O}}_{h_+} (z_2) J^{(s)} (z_3) \rangle
\label{2&3pt}
\end{align}
]]></tex-math></disp-formula>
including <inline-formula><tex-math notation="LaTeX" id="ImEquation26"><![CDATA[$1/c$]]></tex-math></inline-formula> corrections. Here <inline-formula><tex-math notation="LaTeX" id="ImEquation27"><![CDATA[$\mathcal{O}_{h_+} $]]></tex-math></inline-formula> is a scalar operator with conformal weight <inline-formula><tex-math notation="LaTeX" id="ImEquation28"><![CDATA[$h_+ = (1 - N)/2 + \mathcal{O}(c^{-1})$]]></tex-math></inline-formula>. The negative value of the conformal weight reflects the non-unitarity of the theory. At the leading order in <inline-formula><tex-math notation="LaTeX" id="ImEquation29"><![CDATA[$1/c$]]></tex-math></inline-formula>, it was claimed in Ref. [<xref ref-type="bibr" rid="B16">16</xref>] that correlators or conformal blocks can be computed by the networks of open Wilson lines in <inline-formula><tex-math notation="LaTeX" id="ImEquation30"><![CDATA[$\text{sl}(N) $]]></tex-math></inline-formula> Chern&#x2013;Simons gauge theory.<xref ref-type="fn" rid="FN3"><sup>3</sup></xref> For instance, the expectation value of an open Wilson line computes the two-point function <inline-formula><tex-math notation="LaTeX" id="ImEquation31"><![CDATA[$\langle \mathcal{O}_{h_+} \bar{\mathcal{O}}_{h_+} \rangle$]]></tex-math></inline-formula>. Roughly speaking, the open Wilson line corresponds to a particle running in the bulk, which is dual to the boundary two-point function. Furthermore, the three-point function <inline-formula><tex-math notation="LaTeX" id="ImEquation32"><![CDATA[$\langle \mathcal{O}_{h_+} \bar{\mathcal{O}}_{h_+} J^{(s)} \rangle$]]></tex-math></inline-formula> can be evaluated with the extra insertion of the boundary current <inline-formula><tex-math notation="LaTeX" id="ImEquation33"><![CDATA[$J^{(s)}$]]></tex-math></inline-formula>. The main aim of this paper is to interpret the <inline-formula><tex-math notation="LaTeX" id="ImEquation34"><![CDATA[$1/c$]]></tex-math></inline-formula> corrections of the correlators (<xref ref-type="disp-formula" rid="ptx154-M3">3</xref>) as loop corrections in the bulk computations with open Wilson lines. For <inline-formula><tex-math notation="LaTeX" id="ImEquation35"><![CDATA[$N=2$]]></tex-math></inline-formula>, the Chern&#x2013;Simons theory reduces pure gravity theory as in Refs. [<xref ref-type="bibr" rid="B21">21</xref>,<xref ref-type="bibr" rid="B22">22</xref>], and in that case <inline-formula><tex-math notation="LaTeX" id="ImEquation36"><![CDATA[$1/c$]]></tex-math></inline-formula> corrections have been examined in Virasoro conformal blocks [<xref ref-type="bibr" rid="B23">23</xref>] and the conformal weight of the scalar operator [<xref ref-type="bibr" rid="B24">24</xref>]. The validity of the method with <inline-formula><tex-math notation="LaTeX" id="ImEquation37"><![CDATA[$N=2$]]></tex-math></inline-formula> is formally supported by the analysis of conformal Ward identity [<xref ref-type="bibr" rid="B23">23</xref>,<xref ref-type="bibr" rid="B25">25</xref>]. See also Ref. [<xref ref-type="bibr" rid="B26">26</xref>] for a recent application.</p>
<p>During loop computations with open Wilson lines, we would meet divergences and a main issue in this paper is to propose a prescription to regularize the divergences. There are three main steps in the prescription. Firstly, we have to decide how to introduce a regulator <inline-formula><tex-math notation="LaTeX" id="ImEquation38"><![CDATA[$\epsilon$]]></tex-math></inline-formula> to make integrals finite. We adopt a kind of dimensional regularization such that scaling invariance is not broken. Secondly, we have to remove the terms diverging for <inline-formula><tex-math notation="LaTeX" id="ImEquation39"><![CDATA[$\epsilon \to 0$]]></tex-math></inline-formula>. Here we choose to shift parameters in the open Wilson line since we cannot remove divergences in the current setup with the shift of parameters in the Lagrangian as for the usual quantum field theory. Finally, we have to remove ambiguities arising from <inline-formula><tex-math notation="LaTeX" id="ImEquation40"><![CDATA[$\epsilon$]]></tex-math></inline-formula>-independent parts in the shift of parameters. We offer a way to fix them so as to be consistent with the W<inline-formula><tex-math notation="LaTeX" id="ImEquation41"><![CDATA[$_N$]]></tex-math></inline-formula> symmetry of the minimal model.</p>
<p>It is easy to show that the Wilson line method reproduces the leading-order results for correlators in Eq. (<xref ref-type="disp-formula" rid="ptx154-M3">3</xref>) with generic <inline-formula><tex-math notation="LaTeX" id="ImEquation42"><![CDATA[$N$]]></tex-math></inline-formula>. For <inline-formula><tex-math notation="LaTeX" id="ImEquation43"><![CDATA[$1/c$]]></tex-math></inline-formula> corrections, we mainly focus on the simplest examples with <inline-formula><tex-math notation="LaTeX" id="ImEquation44"><![CDATA[$N=2$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation45"><![CDATA[$N=3$]]></tex-math></inline-formula>. We find that the three-point functions from the Wilson line method are regularization-scheme dependent at the <inline-formula><tex-math notation="LaTeX" id="ImEquation46"><![CDATA[$1/c$]]></tex-math></inline-formula> order. Since the three-point functions of the minimal model are fixed by the symmetry, we adopt a regularization such that the Wilson line results match the minimal model ones. For <inline-formula><tex-math notation="LaTeX" id="ImEquation47"><![CDATA[$N=2$]]></tex-math></inline-formula>, the authors in Ref. [<xref ref-type="bibr" rid="B24">24</xref>] tried to reproduce the <inline-formula><tex-math notation="LaTeX" id="ImEquation48"><![CDATA[$1/c$]]></tex-math></inline-formula> corrections in the conformal weight of the scalar operator from the bulk theory. They succeeded in doing so up to the <inline-formula><tex-math notation="LaTeX" id="ImEquation49"><![CDATA[$1/c$]]></tex-math></inline-formula> order since it is regularization independent, but they failed at the <inline-formula><tex-math notation="LaTeX" id="ImEquation50"><![CDATA[$1/c^2$]]></tex-math></inline-formula> order due to the regularization issue. Adopting our prescription for regularization, we succeed in reproducing the <inline-formula><tex-math notation="LaTeX" id="ImEquation51"><![CDATA[$1/c^2$]]></tex-math></inline-formula>-order corrections of conformal weight both for <inline-formula><tex-math notation="LaTeX" id="ImEquation52"><![CDATA[$N=2$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation53"><![CDATA[$N=3$]]></tex-math></inline-formula>.</p>
<p>The organization of this paper is as follows. In the next section, we summarize the results on two- and three-point functions (<xref ref-type="disp-formula" rid="ptx154-M3">3</xref>) in the 2D W<inline-formula><tex-math notation="LaTeX" id="ImEquation54"><![CDATA[$_N$]]></tex-math></inline-formula> minimal model of Eq. (<xref ref-type="disp-formula" rid="ptx154-M1">1</xref>) at the semiclassical limit with <inline-formula><tex-math notation="LaTeX" id="ImEquation55"><![CDATA[$1/c$]]></tex-math></inline-formula> corrections. In <xref ref-type="sec" rid="SEC3">Sect. 3</xref>, we explain our prescription to compute boundary correlators in terms of open Wilson lines in sl<inline-formula><tex-math notation="LaTeX" id="ImEquation56"><![CDATA[$(N)$]]></tex-math></inline-formula> Chern&#x2013;Simons gauge theory. We reproduce the minimal model results at the leading order in <inline-formula><tex-math notation="LaTeX" id="ImEquation57"><![CDATA[$1/c$]]></tex-math></inline-formula> and describe our prescription to regularize divergences arising from loop diagrams. In <xref ref-type="sec" rid="SEC4">Sect. 4</xref>, we apply our method to the simplest case with <inline-formula><tex-math notation="LaTeX" id="ImEquation58"><![CDATA[$N=2$]]></tex-math></inline-formula>. In particular, we reproduce the result in Ref. [<xref ref-type="bibr" rid="B24">24</xref>] for the two-point function at the <inline-formula><tex-math notation="LaTeX" id="ImEquation59"><![CDATA[$1/c$]]></tex-math></inline-formula> order and improve their argument for the next order in <inline-formula><tex-math notation="LaTeX" id="ImEquation60"><![CDATA[$1/c$]]></tex-math></inline-formula> with the help of our analysis for the three-point function. In <xref ref-type="sec" rid="SEC5">Sect. 5</xref>, we proceed to the <inline-formula><tex-math notation="LaTeX" id="ImEquation61"><![CDATA[$N=3$]]></tex-math></inline-formula> case and show that our prescription also works for this example. In <xref ref-type="sec" rid="SEC6">Sect. 6</xref>, we conclude this paper and discuss open problems.</p>
</sec>
<sec id="SEC2"><title>2. W<inline-formula><tex-math notation="LaTeX" id="ImEquation62"><![CDATA[$_N$]]></tex-math></inline-formula> minimal model in the semiclassical regime</title>
<p>In this section, we examine the two- and three-point functions (<xref ref-type="disp-formula" rid="ptx154-M3">3</xref>) of the coset model (<xref ref-type="disp-formula" rid="ptx154-M1">1</xref>) with large <inline-formula><tex-math notation="LaTeX" id="ImEquation63"><![CDATA[$c$]]></tex-math></inline-formula> but finite <inline-formula><tex-math notation="LaTeX" id="ImEquation64"><![CDATA[$N$]]></tex-math></inline-formula> in <inline-formula><tex-math notation="LaTeX" id="ImEquation65"><![CDATA[$1/c$]]></tex-math></inline-formula> expansion. For this purpose we should describe the model in terms of <inline-formula><tex-math notation="LaTeX" id="ImEquation66"><![CDATA[$c,N$]]></tex-math></inline-formula> instead of <inline-formula><tex-math notation="LaTeX" id="ImEquation67"><![CDATA[$k,N$]]></tex-math></inline-formula> in Eq. (<xref ref-type="disp-formula" rid="ptx154-M1">1</xref>). The parameter <inline-formula><tex-math notation="LaTeX" id="ImEquation68"><![CDATA[$k$]]></tex-math></inline-formula> is related to <inline-formula><tex-math notation="LaTeX" id="ImEquation69"><![CDATA[$c,N$]]></tex-math></inline-formula> as
<disp-formula id="ptx154-M4"><label>(4)</label><tex-math notation="LaTeX" id="Equation4"><![CDATA[
\begin{align}
k = - 1 - N + \frac{N (N^2 -1)}{c} + \frac{N (1-N^2)(1-N^3)}{c^2} + \mathcal{O} (c^{-3})
\end{align}
]]></tex-math></disp-formula>
in <inline-formula><tex-math notation="LaTeX" id="ImEquation70"><![CDATA[$1/c$]]></tex-math></inline-formula> expansion. Originally <inline-formula><tex-math notation="LaTeX" id="ImEquation71"><![CDATA[$k$]]></tex-math></inline-formula> is a positive integer, but here we assume an analytic continuation of <inline-formula><tex-math notation="LaTeX" id="ImEquation72"><![CDATA[$k$]]></tex-math></inline-formula> to a real value. See Ref. [<xref ref-type="bibr" rid="B14">14</xref>] for details on the issue. Using this relation, we can expand the physical quantities in <inline-formula><tex-math notation="LaTeX" id="ImEquation73"><![CDATA[$1/c$]]></tex-math></inline-formula>, and the terms at each order depend only on <inline-formula><tex-math notation="LaTeX" id="ImEquation74"><![CDATA[$N$]]></tex-math></inline-formula>.</p>
<p>The two-point function is fixed by the symmetry as
<disp-formula id="ptx154-M5"><label>(5)</label><tex-math notation="LaTeX" id="Equation5"><![CDATA[
\begin{align}
\langle \mathcal{O}_{h} (z) \bar{\mathcal{O}}_{h} (0) \rangle =
\frac{1}{|z|^{4 h}} \, ,
\label{2ptcan0}
\end{align}
]]></tex-math></disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation75"><![CDATA[$h$]]></tex-math></inline-formula> is the conformal weight of the scalar operator <inline-formula><tex-math notation="LaTeX" id="ImEquation76"><![CDATA[$\mathcal{O}_h$]]></tex-math></inline-formula>. The overall normalization can be set as <inline-formula><tex-math notation="LaTeX" id="ImEquation77"><![CDATA[$1$]]></tex-math></inline-formula> by changing the definition of <inline-formula><tex-math notation="LaTeX" id="ImEquation78"><![CDATA[$\mathcal{O}_{h}$]]></tex-math></inline-formula>. This implies that the two-point function is obtained only from knowledge of the spectrum. Throughout the paper, we only focus on the holomorphic sector; thus we may write
<disp-formula id="ptx154-M6"><label>(6)</label><tex-math notation="LaTeX" id="Equation6"><![CDATA[
\begin{align}
\langle \mathcal{O}_{h} (z) \bar{\mathcal{O}}_{h} (0) \rangle =
\frac{1}{z^{2 h}}
\label{2ptcan}
\end{align}
]]></tex-math></disp-formula>
instead of Eq. (<xref ref-type="disp-formula" rid="ptx154-M5">5</xref>).</p>
<p>The spectrum of primary states can be obtained with finite <inline-formula><tex-math notation="LaTeX" id="ImEquation79"><![CDATA[$k,N$]]></tex-math></inline-formula> by applying standard methods like coset construction as in Ref. [<xref ref-type="bibr" rid="B27">27</xref>]. The states are labeled as <inline-formula><tex-math notation="LaTeX" id="ImEquation80"><![CDATA[$(\Lambda_+ , \omega; \Lambda_-)$]]></tex-math></inline-formula>, where <inline-formula><tex-math notation="LaTeX" id="ImEquation81"><![CDATA[$\Lambda_+ , \omega, \Lambda_-$]]></tex-math></inline-formula> are the highest weights of <inline-formula><tex-math notation="LaTeX" id="ImEquation82"><![CDATA[$\text{su}(N)_{k}, \text{su}(N)_{1}, \text{su}(N)_{k+1}$]]></tex-math></inline-formula>, respectively. The selection rule determines <inline-formula><tex-math notation="LaTeX" id="ImEquation83"><![CDATA[$\omega$]]></tex-math></inline-formula> in terms of <inline-formula><tex-math notation="LaTeX" id="ImEquation84"><![CDATA[$\Lambda_+ , \Lambda_-$]]></tex-math></inline-formula>, so we may instead use the label <inline-formula><tex-math notation="LaTeX" id="ImEquation85"><![CDATA[$(\Lambda_+ ; \Lambda_-)$]]></tex-math></inline-formula>. We should take care with the field identification in Ref. [<xref ref-type="bibr" rid="B28">28</xref>] as well. The conformal weight of the state can be obtained by coset construction [<xref ref-type="bibr" rid="B27">27</xref>] or Drinfeld&#x2013;Sokolov reduction; see, e.g., Refs. [<xref ref-type="bibr" rid="B29">29</xref>,<xref ref-type="bibr" rid="B30">30</xref>]. For instance, the latter gives the formula
<disp-formula id="ptx154-M7"><label>(7)</label><tex-math notation="LaTeX" id="Equation7"><![CDATA[
\begin{align}
h (\Lambda_+ ; \Lambda_-) = \frac{| (k+N+1) (\Lambda_+ + \hat \rho ) - (k + N) (\Lambda_- + \hat \rho)|^2 - \hat \rho^2 }{2 (k + N ) (k+N+1)} \, ,
\end{align}
]]></tex-math></disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation86"><![CDATA[$\hat \rho$]]></tex-math></inline-formula> is the Weyl vector of <inline-formula><tex-math notation="LaTeX" id="ImEquation87"><![CDATA[$\text{su}(N)$]]></tex-math></inline-formula>. According to Ref. [<xref ref-type="bibr" rid="B15">15</xref>] (see also Ref. [<xref ref-type="bibr" rid="B13">13</xref>] for the original proposal), the state <inline-formula><tex-math notation="LaTeX" id="ImEquation88"><![CDATA[$(0;\Lambda_-)$]]></tex-math></inline-formula> corresponds to a conical defect geometry, and the generic state <inline-formula><tex-math notation="LaTeX" id="ImEquation89"><![CDATA[$(\Lambda_+;\Lambda_-)$]]></tex-math></inline-formula> is mapped to the geometry dressed by perturbative matters. In particular, the states <inline-formula><tex-math notation="LaTeX" id="ImEquation90"><![CDATA[$(0;0)$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation91"><![CDATA[$(\text{f};0)$]]></tex-math></inline-formula> correspond to the AdS vacuum, and a bulk scalar field on the background. Here we denote <inline-formula><tex-math notation="LaTeX" id="ImEquation92"><![CDATA[$\text{f}$]]></tex-math></inline-formula> as the fundamental representation. The conformal weight of the state <inline-formula><tex-math notation="LaTeX" id="ImEquation93"><![CDATA[$(\text{f};0)$]]></tex-math></inline-formula> is
<disp-formula id="ptx154-M8"><label>(8)</label><tex-math notation="LaTeX" id="Equation8"><![CDATA[
\begin{align}
&h_+ \equiv h(\text{f};0) = \frac{(N-1) (k + 2N + 1)}{2 N (k + N)} \, ,
\label{hexact}
\end{align}
]]></tex-math></disp-formula>
and we mainly deal with the operator <inline-formula><tex-math notation="LaTeX" id="ImEquation94"><![CDATA[$\mathcal{O}_{h_+} $]]></tex-math></inline-formula> corresponding to the state in this paper.</p>
<p>Expanding the conformal weight <inline-formula><tex-math notation="LaTeX" id="ImEquation95"><![CDATA[$h$]]></tex-math></inline-formula> in <inline-formula><tex-math notation="LaTeX" id="ImEquation96"><![CDATA[$1/c$]]></tex-math></inline-formula> as
<disp-formula id="ptx154-M9"><label>(9)</label><tex-math notation="LaTeX" id="Equation9"><![CDATA[
\begin{align}
h = h_0 + \frac{1}{c} h_1 + \frac{1}{c^2} h_2 + \mathcal{O} (c^{-3}) \, ,
\label{hexp}
\end{align}
]]></tex-math></disp-formula>
the two-point function becomes
<disp-formula id="ptx154-M10"><label>(10)</label><tex-math notation="LaTeX" id="Equation10"><![CDATA[
\begin{align}
\langle \mathcal{O}_{h} (z) \bar{\mathcal{O}}_{h} (0) \rangle = \frac{1}{z^{2 h_0}} \left[ 1 - \frac1c 2 h_1 \log (z) + \frac{1}{c^2} \left( 2 h_1^2 \log ^2 (z) - 2 h_2 \log (z) \right) \right] + \mathcal{O} (c^{-3}) \, . \label{2ptexp}
\end{align}
]]></tex-math></disp-formula></p>
<p>For the operator <inline-formula><tex-math notation="LaTeX" id="ImEquation97"><![CDATA[$\mathcal{O}_{h_+} $]]></tex-math></inline-formula> we have
<disp-formula id="ptx154-M11"><label>(11)</label><tex-math notation="LaTeX" id="Equation11"><![CDATA[
\begin{align}
h_0 = \frac{1-N}{2} \, , \quad
h_1 = -\frac{\left(N^2-1\right)^2}{2 } \, , \quad
h_2 = -\frac{(N+1)^2 (2 N (N+1)+1) (N-1)^3}{2} \, , \label{h012}
\end{align}
]]></tex-math></disp-formula>
which is obtained from Eq. (<xref ref-type="disp-formula" rid="ptx154-M8">8</xref>) with finite <inline-formula><tex-math notation="LaTeX" id="ImEquation98"><![CDATA[$k,N$]]></tex-math></inline-formula>. The problem will be whether we can reproduce the correct coefficients in front of <inline-formula><tex-math notation="LaTeX" id="ImEquation99"><![CDATA[$\log (z)$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation100"><![CDATA[$\log^2 (z)$]]></tex-math></inline-formula> from the bulk viewpoint with open Wilson lines.</p>
<p>We also examine the three-point functions in Eq. (<xref ref-type="disp-formula" rid="ptx154-M3">3</xref>). In Ref. [<xref ref-type="bibr" rid="B1">1</xref>] we have evaluated the three-point functions by decomposing the four-point function of <inline-formula><tex-math notation="LaTeX" id="ImEquation101"><![CDATA[$\mathcal{O}_{h_+} $]]></tex-math></inline-formula> with Virasoro conformal blocks. As seen below, we have effectively decomposed the W<inline-formula><tex-math notation="LaTeX" id="ImEquation102"><![CDATA[$_N$]]></tex-math></inline-formula> vacuum block, which is fixed by the W<inline-formula><tex-math notation="LaTeX" id="ImEquation103"><![CDATA[$_N$]]></tex-math></inline-formula> symmetry in principle, and this implies that the three-point functions can be fixed solely by the symmetry. Notice that the three-point function with spin-two current as
<disp-formula id="ptx154-M12"><label>(12)</label><tex-math notation="LaTeX" id="Equation12"><![CDATA[
\begin{align}
\langle \mathcal{O}_{h} (z_1) \bar{\mathcal{O}}_{h} (z_2) J^{(2)} (z_3) \rangle
\end{align}
]]></tex-math></disp-formula>
is determined by the conformal Ward identity, and our conclusion may be regarded as a higher-spin generalization.</p>
<p>We decompose the following four-point function as
<disp-formula id="ptx154-M13"><label>(13)</label><tex-math notation="LaTeX" id="Equation13"><![CDATA[
\begin{align}
G_{++} (z) &= \langle \mathcal{O}_{h_+} (\infty) \bar{\mathcal{O}}_{h_+} (1) \mathcal{O}_{h_+} (z) \bar{\mathcal{O}}_{h_+} (0) \rangle,
\label{4pt}
\end{align}
]]></tex-math></disp-formula>
for which the expression with finite <inline-formula><tex-math notation="LaTeX" id="ImEquation104"><![CDATA[$k,N$]]></tex-math></inline-formula> is given by [<xref ref-type="bibr" rid="B31">31</xref>]
<disp-formula id="ptx154-M14"><label>(14)</label><tex-math notation="LaTeX" id="Equation14"><![CDATA[
\begin{align}
G_{++} (z) = |\mathcal{F}_1 (z)|^2 + \mathcal{N}_1 |\mathcal{F}_2 (z)|^2
\, .
\end{align}
]]></tex-math></disp-formula></p>
<p>Here the W<inline-formula><tex-math notation="LaTeX" id="ImEquation105"><![CDATA[$_N$]]></tex-math></inline-formula> conformal blocks are
<disp-formula id="ptx154-M15"><label>(15)</label><tex-math notation="LaTeX" id="Equation15"><![CDATA[
\begin{align}
\mathcal{F}_1 (z) = z^{- 2 h_+}(1 - z)^{ - 2 h_+ + \frac{k +2N}{k+N}}
{}_2 F_1 \left( \frac{k+N+1}{k+N} , - \frac{1}{k+N} ; - \frac{N}{k+N} ; z \right) \, ,\nonumber \\
\mathcal{F}_2 (z) = z^{- 2 h_+ + \frac{k +2N}{k+N}}(1 - x)^{ - 2 h_+ }
{}_2 F_1 \left( \frac{k+N+1}{k+N} , - \frac{1}{k+N} ; \frac{2 k + 3N}{k+N} ; z \right) \, ,
\end{align}
]]></tex-math></disp-formula>
and the relative coefficient is
<disp-formula id="ptx154-M16"><label>(16)</label><tex-math notation="LaTeX" id="Equation16"><![CDATA[
\begin{align}
\mathcal{N}_1 = - \frac{\Gamma \left(\frac{k + 2N -1}{k+N}\right) \Gamma
\left(\frac{-N}{k+N}\right)^2\Gamma \left(\frac{2 k + 3N +1}{k+N}\right)}{\Gamma\left(\frac{- k - 2N - 1}{k+N}\right) \Gamma
\left(\frac{1-N}{k+N}\right) \Gamma \left(\frac{2k+3N}{k+N}\right)^2}\,.
\end{align}
]]></tex-math></disp-formula></p>
<p>From the leading terms in <inline-formula><tex-math notation="LaTeX" id="ImEquation106"><![CDATA[$z$]]></tex-math></inline-formula> expansion, we can read off the conformal weights of the intermediate state. For <inline-formula><tex-math notation="LaTeX" id="ImEquation107"><![CDATA[$\mathcal{F}_1 (z)$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation108"><![CDATA[$\mathcal{F}_2 (z)$]]></tex-math></inline-formula>, the intermediate states are found to be the identity and the state <inline-formula><tex-math notation="LaTeX" id="ImEquation109"><![CDATA[$(\text{adj};0)$]]></tex-math></inline-formula>, respectively. Here adj represents the adjoint representation of sl<inline-formula><tex-math notation="LaTeX" id="ImEquation110"><![CDATA[$(N)$]]></tex-math></inline-formula>, and the conformal weight of the state is <inline-formula><tex-math notation="LaTeX" id="ImEquation111"><![CDATA[$h (\text{adj};0) = (k +2N)/(k+N)$]]></tex-math></inline-formula>. This is consistent with the decomposition as <inline-formula><tex-math notation="LaTeX" id="ImEquation112"><![CDATA[$\text{f} \otimes \bar{\text{f}} = 1 \oplus \text{adj}$]]></tex-math></inline-formula> with <inline-formula><tex-math notation="LaTeX" id="ImEquation113"><![CDATA[$\bar{\text{f}}$]]></tex-math></inline-formula> as the anti-fundamental representation of sl<inline-formula><tex-math notation="LaTeX" id="ImEquation114"><![CDATA[$(N)$]]></tex-math></inline-formula>. As discussed in Ref. [<xref ref-type="bibr" rid="B1">1</xref>], we only need to consider the W<inline-formula><tex-math notation="LaTeX" id="ImEquation115"><![CDATA[$_N$]]></tex-math></inline-formula> vacuum block <inline-formula><tex-math notation="LaTeX" id="ImEquation116"><![CDATA[$\mathcal{F}_1 (z) $]]></tex-math></inline-formula> in order to obtain the three-point functions in Eq. (<xref ref-type="disp-formula" rid="ptx154-M3">3</xref>). Therefore, we conclude that these three-point functions are fixed by W<inline-formula><tex-math notation="LaTeX" id="ImEquation117"><![CDATA[$_N$]]></tex-math></inline-formula> symmetry even with finite <inline-formula><tex-math notation="LaTeX" id="ImEquation118"><![CDATA[$k,N$]]></tex-math></inline-formula>.</p>
<p>We obtain the three-point functions with <inline-formula><tex-math notation="LaTeX" id="ImEquation119"><![CDATA[$1/c$]]></tex-math></inline-formula> corrections by slightly modifying the analysis in Ref. [<xref ref-type="bibr" rid="B1">1</xref>]. We decompose the four-point function (<xref ref-type="disp-formula" rid="ptx154-M13">13</xref>) as
<disp-formula id="ptx154-M17"><label>(17)</label><tex-math notation="LaTeX" id="Equation17"><![CDATA[
\begin{align}
|z|^{4 h_+} G_{++} (z) = \mathcal{V}_0 (z)+ \sum_{s =3}^\infty (C^{(s)})^2 \mathcal{V}_s (z)
+ \cdots \, ,
\label{cbd}
\end{align}
]]></tex-math></disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation120"><![CDATA[$\mathcal{V}_0 (z)$]]></tex-math></inline-formula> is the Virasoro vacuum block and <inline-formula><tex-math notation="LaTeX" id="ImEquation121"><![CDATA[$\mathcal{V}_s (z)$]]></tex-math></inline-formula> is the Virasoro block of spin-<inline-formula><tex-math notation="LaTeX" id="ImEquation122"><![CDATA[$s$]]></tex-math></inline-formula> current. The coefficient <inline-formula><tex-math notation="LaTeX" id="ImEquation123"><![CDATA[$C^{(s)}$]]></tex-math></inline-formula> is related to the three-point function in Eq. (<xref ref-type="disp-formula" rid="ptx154-M3">3</xref>) as
<disp-formula id="ptx154-M18"><label>(18)</label><tex-math notation="LaTeX" id="Equation18"><![CDATA[
\begin{align}
C^{(s)} = \frac{\langle \mathcal{O}_{h_+} \bar{\mathcal{O}}_{h_+} J^{(s)} \rangle }{\langle J^{(s)}J^{(s)} \rangle^{1/2} } \, .
\end{align}
]]></tex-math></disp-formula></p>
<p>Since <inline-formula><tex-math notation="LaTeX" id="ImEquation124"><![CDATA[$\mathcal{V}_s (z)$]]></tex-math></inline-formula> start to contribute at the order of <inline-formula><tex-math notation="LaTeX" id="ImEquation125"><![CDATA[$1/c$]]></tex-math></inline-formula>, we expand as
<disp-formula id="ptx154-M19"><label>(19)</label><tex-math notation="LaTeX" id="Equation19"><![CDATA[
\begin{align}
C^{(s)} = c^{-1/2} \left[ C^{(s)}_0 + c^{-1} C^{(s)}_1 + \mathcal{O} (c^{-2}) \right] \, .
\end{align}
]]></tex-math></disp-formula></p>
<p>The relevant part of the four-point function (<xref ref-type="disp-formula" rid="ptx154-M13">13</xref>) can be expanded in <inline-formula><tex-math notation="LaTeX" id="ImEquation126"><![CDATA[$z$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation127"><![CDATA[$1/c$]]></tex-math></inline-formula> as
<disp-formula id="ptx154-M20"><label>(20)</label><tex-math notation="LaTeX" id="Equation20"><![CDATA[
\begin{align}
& |z|^{4 h_+} G_{++}(z) \nonumber\\
& \quad \sim 1 + \frac{1}{c} \sum_{n=1}^\infty (1 - N^2)
\left( - \frac{1}{n} + \frac{N \Gamma(N) \Gamma(n)}{\Gamma(N +n)} \right) z^n + \frac{1}{c^2} \sum_{n = 2}^\infty f_c^{(n)} z^n + \cdots \, ,
\end{align}
]]></tex-math></disp-formula>
where we have defined
<disp-formula id="ptx154-M21"><label>(21)</label><tex-math notation="LaTeX" id="Equation21"><![CDATA[
\begin{align}
\frac{f_c^{(n)}}{(1 - N^2)^2} &= \frac{1}{n} \sum_{l=1}^{n-1} \frac{1}{l}+ \frac{\Gamma(n) \Gamma(N) N^2}{\Gamma(N + n)}
\left( \sum_{l=0}^{n-1} \frac{N}{N + l} - \frac{1}{n} - 2 - \frac{1}{N} + \frac{1}{1+N} \right) \nonumber \\
& \quad - \sum_{l=1}^{n-1} \frac{N\Gamma(N)\Gamma(l)}{(n-l) \Gamma(N+l)} + \left(2N + \frac{1}{1 + N}\right) \frac{1}{n} \, .
\end{align}
]]></tex-math></disp-formula></p>
<p>Solving the constraint equations from Eq. (<xref ref-type="disp-formula" rid="ptx154-M17">17</xref>), we find
<disp-formula id="ptx154-M22"><label>(22)</label><tex-math notation="LaTeX" id="Equation22"><![CDATA[
\begin{align}
(C^{(s)}_0)^2 = \frac{(1 - N^2) \Gamma(1+N) \Gamma(s-N)}{\Gamma(1 - N) \Gamma(s + N)} \frac{\Gamma(s)^2}{\Gamma(2s-1)}
\label{3pt0}
\end{align}
]]></tex-math></disp-formula>
for the leading order in <inline-formula><tex-math notation="LaTeX" id="ImEquation128"><![CDATA[$1/c$]]></tex-math></inline-formula>. The first few examples are
<disp-formula id="ptx154-M23"><label>(23)</label><tex-math notation="LaTeX" id="Equation23"><![CDATA[
\begin{align}
(C^{(2)}_0)^2 = \frac{1}{2} (1-N)^2 \, , \quad
(C^{(3)}_0)^2 = \frac{1}{6} \frac{(1-N)^2 (2 - N)}{(2 + N)} \, .
\end{align}
]]></tex-math></disp-formula></p>
<p>The square of the three-point function could be negative for <inline-formula><tex-math notation="LaTeX" id="ImEquation129"><![CDATA[$N \geq 3$]]></tex-math></inline-formula>, and this is related to the fact that we are working in a non-unitary theory.</p>
<p>Examining Eq. (<xref ref-type="disp-formula" rid="ptx154-M17">17</xref>) at the next order in <inline-formula><tex-math notation="LaTeX" id="ImEquation130"><![CDATA[$1/c$]]></tex-math></inline-formula>, we can obtain <inline-formula><tex-math notation="LaTeX" id="ImEquation131"><![CDATA[$1/c$]]></tex-math></inline-formula> corrections to the three-point functions as well. At this order, the constraint equations for <inline-formula><tex-math notation="LaTeX" id="ImEquation132"><![CDATA[$s=3,4,5$]]></tex-math></inline-formula> are found to be
<disp-formula id="ptx154-M24"><label>(24)</label><tex-math notation="LaTeX" id="Equation24"><![CDATA[
\begin{align}
f^{(3)}_c &= f^{(2)}_c + 2 C_{0}^{(3)}C_{1}^{(3)} \, , \nonumber
\\
f^{(4)}_c &= f^{(2)}_c\frac{9}{10} + \frac{(1-N)^2}{8(1+N)^2} + \frac{1-N}{10(1+N)^2} + \frac{1}{50(1+N)^2} + 2 C_{0}^{(3)}C_{1}^{(3)}\frac{3}{2} + 2 C_{0}^{(4)}C_{1}^{(4)} \, , \nonumber \\
f^{(5)}_c &= f^{(2)}_c\frac{4}{5} + \frac{(1-N)^2}{4(1+N)^2} + \frac{1-N}{5(1+N)^2} + \frac{1}{25(1+N)^2} + 2 C_{0}^{(3)}C_{1}^{(3)} \frac{12}{7} + 2 C_{0}^{(4)}C_{1}^{(4)}\cdot2 \nonumber \\
& \quad + 2 C_{0}^{(5)}C_{1}^{(5)} + (C_{0}^{(3)})^2\left[\frac{1}{2}\frac{1-N}{1+N}+\frac{6}{7(1+N)}+\frac{18}{49(1-N^2)}\right] \, . \end{align}
]]></tex-math></disp-formula></p>
<p>From these equations, we obtain
<disp-formula id="ptx154-M25"><label>(25)</label><tex-math notation="LaTeX" id="Equation25"><![CDATA[
\begin{align}
\frac{C_{1}^{(3)}}{C_{0}^{(3)}} &= N^3+3 N^2-3 N-\frac{6}{N+2}+1 \, , \nonumber \\
\frac{C_{1}^{(4)}}{C_{0}^{(4)}} &= N^3+\frac{29 N^2}{4}+\frac{3 N}{2}+\frac{189}{2 (N-3)}-\frac{8}{N-2}+\frac{47}{40 (N-1)}-\frac{3}{10 (N-1)^2} \nonumber \\
& \quad -\frac{27}{40 (N+1)}-\frac{3}{10 (N+1)^2}-\frac{6}{N+2}-\frac{36}{N+3}+\frac{161}{4} \, , \\
\frac{C_{1}^{(5)}}{C_{0}^{(5)}} &= N^3+\frac{155 N^2}{12}+\frac{29 N}{2}+\frac{800}{N-4}-\frac{180}{N-3}+\frac{25}{7 (N-1)}
-\frac{25}{7 (N+1)}-\frac{6}{N+2} \nonumber \\
& \quad -\frac{36}{N+3}-\frac{120}{N+4}+\frac{359}{2} \, . \nonumber
\end{align}
]]></tex-math></disp-formula></p>
<p>In particular, <inline-formula><tex-math notation="LaTeX" id="ImEquation133"><![CDATA[$C_{1}^{(3)}/C_{0}^{(3)} = 224/5$]]></tex-math></inline-formula> for <inline-formula><tex-math notation="LaTeX" id="ImEquation134"><![CDATA[$N=3$]]></tex-math></inline-formula>. It is not difficult to extend the analysis for <inline-formula><tex-math notation="LaTeX" id="ImEquation135"><![CDATA[$C_{1}^{(s)}/C_{0}^{(s)}$]]></tex-math></inline-formula> at least up to <inline-formula><tex-math notation="LaTeX" id="ImEquation136"><![CDATA[$s=8$]]></tex-math></inline-formula> by directly applying the analysis in Ref. [<xref ref-type="bibr" rid="B9">9</xref>].</p>
</sec>
<sec id="SEC3"><title>3. Preliminaries for bulk computations</title>
<p>In this section, we explain our prescription to compute the two- and three-point functions (<xref ref-type="disp-formula" rid="ptx154-M3">3</xref>) from bulk theory. In the next subsection, we introduce sl<inline-formula><tex-math notation="LaTeX" id="ImEquation137"><![CDATA[$(N)$]]></tex-math></inline-formula> Chern&#x2013;Simons gauge theory and open Wilson lines. In <xref ref-type="sec" rid="SEC3.2">Sect. 3.2</xref> we explain the representation of sl<inline-formula><tex-math notation="LaTeX" id="ImEquation138"><![CDATA[$(N)$]]></tex-math></inline-formula> generators in terms of <inline-formula><tex-math notation="LaTeX" id="ImEquation139"><![CDATA[$x$]]></tex-math></inline-formula>-derivatives. In <xref ref-type="sec" rid="SEC3.3">Sect. 3.3</xref>, we compute the two- and three-point functions in Eq. (<xref ref-type="disp-formula" rid="ptx154-M3">3</xref>) at the leading order in <inline-formula><tex-math notation="LaTeX" id="ImEquation140"><![CDATA[$1/c$]]></tex-math></inline-formula>. In <xref ref-type="sec" rid="SEC3.4">Sect. 3.4</xref>, we give a prescription to regularize divergences arising from loop diagrams, and prepare for explicit computations for <inline-formula><tex-math notation="LaTeX" id="ImEquation141"><![CDATA[$N=2,3$]]></tex-math></inline-formula> in succeeding sections.</p>
<sec id="SEC3.1"><title>3.1. Chern&#x2013;Simons gauge theory and open Wilson lines</title>
<p>In three dimensions, pure gravity with a negative cosmological constant can be described by <inline-formula><tex-math notation="LaTeX" id="ImEquation142"><![CDATA[$\text{sl}(2) \oplus \text{sl}(2)$]]></tex-math></inline-formula> Chern&#x2013;Simons gauge theory [<xref ref-type="bibr" rid="B21">21</xref>,<xref ref-type="bibr" rid="B22">22</xref>]. As a natural extension, we can construct a higher-spin gauge theory using Chern&#x2013;Simons theory based on a higher-rank gauge algebra [<xref ref-type="bibr" rid="B32">32</xref>]. We are interested in <inline-formula><tex-math notation="LaTeX" id="ImEquation143"><![CDATA[$\text{sl}(N) \oplus \text{sl}(N)$]]></tex-math></inline-formula> Chern&#x2013;Simons theory, whose action is given by
<disp-formula id="ptx154-M26"><label>(26)</label><tex-math notation="LaTeX" id="Equation26"><![CDATA[
\begin{align}
S = S_\text{CS} [A] - S_\text{CS} [\tilde A] \, , \quad
S_\text{CS} [A] = \frac{\hat k}{4 \pi} \int \text{tr} \left( A \wedge d A + \frac{2}{3} A \wedge A \wedge A \right) \, .
\end{align}
]]></tex-math></disp-formula></p>
<p>Here <inline-formula><tex-math notation="LaTeX" id="ImEquation144"><![CDATA[$\hat k$]]></tex-math></inline-formula> is the level of Chern&#x2013;Simons theory and <inline-formula><tex-math notation="LaTeX" id="ImEquation145"><![CDATA[$A, \tilde A$]]></tex-math></inline-formula> are one-forms taking values in <inline-formula><tex-math notation="LaTeX" id="ImEquation146"><![CDATA[$\text{sl}(N)$]]></tex-math></inline-formula>. The generators of sl<inline-formula><tex-math notation="LaTeX" id="ImEquation147"><![CDATA[$(N)$]]></tex-math></inline-formula> can be decomposed in terms of the adjoint action of embedded sl<inline-formula><tex-math notation="LaTeX" id="ImEquation148"><![CDATA[$(2)$]]></tex-math></inline-formula> as
<disp-formula id="ptx154-M27"><label>(27)</label><tex-math notation="LaTeX" id="Equation27"><![CDATA[
\begin{align}
\text{sl} (N) = \text{sl} (2) \oplus \left( \bigoplus_{s=3}^{N} g^{(s)} \right) \, .
\end{align}
]]></tex-math></disp-formula></p>
<p>Here <inline-formula><tex-math notation="LaTeX" id="ImEquation149"><![CDATA[$g^{(s)}$]]></tex-math></inline-formula> denotes the spin-<inline-formula><tex-math notation="LaTeX" id="ImEquation150"><![CDATA[$(s-1)$]]></tex-math></inline-formula> representation of sl<inline-formula><tex-math notation="LaTeX" id="ImEquation151"><![CDATA[$(2)$]]></tex-math></inline-formula>, and we have adopted the principal embedding of sl<inline-formula><tex-math notation="LaTeX" id="ImEquation152"><![CDATA[$(2)$]]></tex-math></inline-formula>. The generators in sl<inline-formula><tex-math notation="LaTeX" id="ImEquation153"><![CDATA[$(2)$]]></tex-math></inline-formula> (adjoint representation) and <inline-formula><tex-math notation="LaTeX" id="ImEquation154"><![CDATA[$g^{(s)}$]]></tex-math></inline-formula> are denoted as <inline-formula><tex-math notation="LaTeX" id="ImEquation155"><![CDATA[$V^2_n$]]></tex-math></inline-formula> <inline-formula><tex-math notation="LaTeX" id="ImEquation156"><![CDATA[$(n=-1,0,1)$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation157"><![CDATA[$V^s_n$]]></tex-math></inline-formula> <inline-formula><tex-math notation="LaTeX" id="ImEquation158"><![CDATA[$(n= - s+1,-s+2,\ldots , s-1)$]]></tex-math></inline-formula>, respectively.</p>
<p>For the application to higher-spin AdS<inline-formula><tex-math notation="LaTeX" id="ImEquation159"><![CDATA[$_3$]]></tex-math></inline-formula> gravity, we need to assign an asymptotic AdS condition to the gauge fields. We use the metric of Euclidean AdS<inline-formula><tex-math notation="LaTeX" id="ImEquation160"><![CDATA[$_3$]]></tex-math></inline-formula> as <inline-formula><tex-math notation="LaTeX" id="ImEquation161"><![CDATA[$ds^2 = d \rho^2 + e^{2\rho} dz d \bar z$]]></tex-math></inline-formula>, where the boundary is at <inline-formula><tex-math notation="LaTeX" id="ImEquation162"><![CDATA[$\rho \to \infty$]]></tex-math></inline-formula>. In a gauge choice, we can set
<disp-formula id="ptx154-M28"><label>(28)</label><tex-math notation="LaTeX" id="Equation28"><![CDATA[
\begin{align}
A = e^{- \rho V_0^{2}} a (z) e^{\rho V_0^{2}} dz + V_0^2 d \rho \, .
\end{align}
]]></tex-math></disp-formula></p>
<p>We have a similar expression for <inline-formula><tex-math notation="LaTeX" id="ImEquation163"><![CDATA[$\tilde A$]]></tex-math></inline-formula> but suppress it here and in the following. The configuration corresponding to AdS<inline-formula><tex-math notation="LaTeX" id="ImEquation164"><![CDATA[$_3$]]></tex-math></inline-formula> background is given by <inline-formula><tex-math notation="LaTeX" id="ImEquation165"><![CDATA[$a(z) = V_{1}^2$]]></tex-math></inline-formula>. The asymptotic AdS condition restricts the form of <inline-formula><tex-math notation="LaTeX" id="ImEquation166"><![CDATA[$a(z)$]]></tex-math></inline-formula> as [<xref ref-type="bibr" rid="B33">33</xref>&#x2013;<xref ref-type="bibr" rid="B36">36</xref>]
<disp-formula id="ptx154-M29"><label>(29)</label><tex-math notation="LaTeX" id="Equation29"><![CDATA[
\begin{align}
a (z) = V_1^{2} - \frac{1}{\hat k} \sum_{s \geq 2} ^N \frac{1}{N_s} J^{(s)} (z) V^s_{-s + 1} \, , \quad N_s = \text{tr} (V_{-s +1}^s V_{s-1}^s) \, .
\label{dsgauge}
\end{align}
]]></tex-math></disp-formula></p>
<p>There are residual gauge symmetries preserving the condition (<xref ref-type="disp-formula" rid="ptx154-M29">29</xref>), and some of them generate W<inline-formula><tex-math notation="LaTeX" id="ImEquation167"><![CDATA[$_N$]]></tex-math></inline-formula> symmetry near the AdS boundary. We can define classical Poisson brackets for the reduced phase space. Moreover, we can see that <inline-formula><tex-math notation="LaTeX" id="ImEquation168"><![CDATA[$J^{(s)}(z)$]]></tex-math></inline-formula> in Eq. (<xref ref-type="disp-formula" rid="ptx154-M29">29</xref>) generate the W<inline-formula><tex-math notation="LaTeX" id="ImEquation169"><![CDATA[$_N$]]></tex-math></inline-formula> symmetry in terms of the Poisson brackets. At the classical level, the relation between the Chern&#x2013;Simons level <inline-formula><tex-math notation="LaTeX" id="ImEquation170"><![CDATA[$\hat k$]]></tex-math></inline-formula> and the central charge <inline-formula><tex-math notation="LaTeX" id="ImEquation171"><![CDATA[$c$]]></tex-math></inline-formula> of the dual conformal field theory is given by the Brown&#x2013;Henneaux one as [<xref ref-type="bibr" rid="B37">37</xref>]
<disp-formula id="ptx154-M30"><label>(30)</label><tex-math notation="LaTeX" id="Equation30"><![CDATA[
\begin{align}
c = 6 \hat k \, .
\label{bhclassical}
\end{align}
]]></tex-math></disp-formula></p>
<p>See Refs. [<xref ref-type="bibr" rid="B33">33</xref>&#x2013;<xref ref-type="bibr" rid="B36">36</xref>] for more details.</p>
<p>At the leading order in <inline-formula><tex-math notation="LaTeX" id="ImEquation172"><![CDATA[$1/c$]]></tex-math></inline-formula>, the rules for computing conformal blocks from the Chern&#x2013;Simons theory with open Wilson lines were given in Ref. [<xref ref-type="bibr" rid="B16">16</xref>]; see also Ref. [<xref ref-type="bibr" rid="B38">38</xref>] for <inline-formula><tex-math notation="LaTeX" id="ImEquation173"><![CDATA[$N=2$]]></tex-math></inline-formula>. For the two- and three-point functions in Eq. (<xref ref-type="disp-formula" rid="ptx154-M3">3</xref>), we use
<disp-formula id="ptx154-M31"><label>(31)</label><tex-math notation="LaTeX" id="Equation31"><![CDATA[
\begin{align}
\langle \text{lw} | W (z_2 ; z_1) | \text{hw} \rangle \, , \quad
W(z_2 ; z_1) = P \exp \left(\int _{z_1}^{z_2} dz a(z) \right) \, .
\label{classicalwilson}
\end{align}
]]></tex-math></disp-formula></p>
<p>Here hw and lw denote the highest and lowest weight states in finite-dimensional representations of sl<inline-formula><tex-math notation="LaTeX" id="ImEquation174"><![CDATA[$(N)$]]></tex-math></inline-formula>, respectively, and <inline-formula><tex-math notation="LaTeX" id="ImEquation175"><![CDATA[$P$]]></tex-math></inline-formula> represents the path ordering. Moreover, we remove the <inline-formula><tex-math notation="LaTeX" id="ImEquation176"><![CDATA[$\rho$]]></tex-math></inline-formula> dependence in the gauge field as <inline-formula><tex-math notation="LaTeX" id="ImEquation177"><![CDATA[$A(z) = a(z)$]]></tex-math></inline-formula> using a gauge transformation. We include <inline-formula><tex-math notation="LaTeX" id="ImEquation178"><![CDATA[$1/c$]]></tex-math></inline-formula> corrections by extending the analysis in Refs. [<xref ref-type="bibr" rid="B23">23</xref>,<xref ref-type="bibr" rid="B24">24</xref>] for <inline-formula><tex-math notation="LaTeX" id="ImEquation179"><![CDATA[$N=2$]]></tex-math></inline-formula>. At the leading order in <inline-formula><tex-math notation="LaTeX" id="ImEquation180"><![CDATA[$1/c$]]></tex-math></inline-formula>, we treat the coefficient <inline-formula><tex-math notation="LaTeX" id="ImEquation181"><![CDATA[$J^{(s)}(z)$]]></tex-math></inline-formula> in Eq. (<xref ref-type="disp-formula" rid="ptx154-M29">29</xref>) as a function of <inline-formula><tex-math notation="LaTeX" id="ImEquation182"><![CDATA[$z$]]></tex-math></inline-formula>. At higher orders in <inline-formula><tex-math notation="LaTeX" id="ImEquation183"><![CDATA[$1/c$]]></tex-math></inline-formula>, we regard <inline-formula><tex-math notation="LaTeX" id="ImEquation184"><![CDATA[$J^{(s)}(z)$]]></tex-math></inline-formula> as an operator, and the expectation values of open Wilson lines are evaluated by using the correlators of <inline-formula><tex-math notation="LaTeX" id="ImEquation185"><![CDATA[$J^{(s)}(z)$]]></tex-math></inline-formula>, which are uniquely fixed by the W<inline-formula><tex-math notation="LaTeX" id="ImEquation186"><![CDATA[$_N$]]></tex-math></inline-formula> symmetry.</p>
</sec>
<sec id="SEC3.2"><title>3.2. Generators of <inline-formula><tex-math notation="LaTeX" id="ImEquation187"><![CDATA[$\text{sl}(N)$]]></tex-math></inline-formula> algebra</title>
<p>In this subsection we explain our prescription to compute the matrix elements of sl<inline-formula><tex-math notation="LaTeX" id="ImEquation188"><![CDATA[$(N)$]]></tex-math></inline-formula> algebra for evaluating the expectation values of open Wilson lines as in Eq. (<xref ref-type="disp-formula" rid="ptx154-M31">31</xref>). We start with the simplest case with <inline-formula><tex-math notation="LaTeX" id="ImEquation189"><![CDATA[$N=2$]]></tex-math></inline-formula> and then extend the argument for generic <inline-formula><tex-math notation="LaTeX" id="ImEquation190"><![CDATA[$N$]]></tex-math></inline-formula>. For <inline-formula><tex-math notation="LaTeX" id="ImEquation191"><![CDATA[$N=2$]]></tex-math></inline-formula>, there are several previous works in Refs. [<xref ref-type="bibr" rid="B23">23</xref>&#x2013;<xref ref-type="bibr" rid="B25">25</xref>], and we start by clarifying the representation with <inline-formula><tex-math notation="LaTeX" id="ImEquation192"><![CDATA[$x$]]></tex-math></inline-formula>-derivatives in Ref. [<xref ref-type="bibr" rid="B23">23</xref>].</p>
<p>For two-point functions we evaluate
<disp-formula id="ptx154-M32"><label>(32)</label><tex-math notation="LaTeX" id="Equation32"><![CDATA[
\begin{align}
\langle j , - j | W_{-j} (z_2 ; z_1) |\,j , j \rangle \, ,
\label{Gjz1z2}
\end{align}
]]></tex-math></disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation193"><![CDATA[$| j , m \rangle$]]></tex-math></inline-formula> belongs to the spin-<inline-formula><tex-math notation="LaTeX" id="ImEquation194"><![CDATA[$j$]]></tex-math></inline-formula> representation of sl(2) with <inline-formula><tex-math notation="LaTeX" id="ImEquation195"><![CDATA[$m= -j , - j+1 , \ldots ,j$]]></tex-math></inline-formula>. We set the norm of these states as
<disp-formula id="ptx154-M33"><label>(33)</label><tex-math notation="LaTeX" id="Equation33"><![CDATA[
\begin{align}
\langle j , m| j , m' \rangle = \delta_{m,m'} \, .
\end{align}
]]></tex-math></disp-formula></p>
<p>With these states, the sl(2) generators in the Wilson line are described by <inline-formula><tex-math notation="LaTeX" id="ImEquation196"><![CDATA[$(2j+1) \times (2j+1)$]]></tex-math></inline-formula> matrices.</p>
<p>As in Refs. [<xref ref-type="bibr" rid="B23">23</xref>,<xref ref-type="bibr" rid="B25">25</xref>], it would be convenient to map the expression as
<disp-formula id="ptx154-M34"><label>(34)</label><tex-math notation="LaTeX" id="Equation34"><![CDATA[
\begin{align}
\langle j , - j | W_{-j} (z_2 ; z_1) | j , j \rangle =
\int dx
\langle j , - j |x \rangle W_{-j} (z_2 ; z_1) \langle x | j , j \rangle \, ,
\end{align}
]]></tex-math></disp-formula>
then the sl<inline-formula><tex-math notation="LaTeX" id="ImEquation197"><![CDATA[$(2)$]]></tex-math></inline-formula> generators can be written as
<disp-formula id="ptx154-M35"><label>(35)</label><tex-math notation="LaTeX" id="Equation35"><![CDATA[
\begin{align}
J_+ (= V_{-1}^2)= x^2 \partial_x - 2 j x \, , \quad
J_3 (= - V_{0}^2)= - x \partial_x + j \, , \quad
J_- (= V_{+1}^2)= \partial_x \, .
\label{xsl2}
\end{align}
]]></tex-math></disp-formula></p>
<p>In Ref. [<xref ref-type="bibr" rid="B23">23</xref>], they proposed that the wave functions are given by
<disp-formula id="ptx154-M36"><label>(36)</label><tex-math notation="LaTeX" id="Equation36"><![CDATA[
\begin{align}
\langle x | j , j \rangle = x^{2j} \, , \quad \langle j , - j |x \rangle = \delta (x) \, .
\label{basisx}
\end{align}
]]></tex-math></disp-formula></p>
<p>We would like to give a derivation such that it can be extended for generic <inline-formula><tex-math notation="LaTeX" id="ImEquation198"><![CDATA[$N$]]></tex-math></inline-formula>. It is easy to obtain <inline-formula><tex-math notation="LaTeX" id="ImEquation199"><![CDATA[$\langle x | j , j \rangle = x^{2j}$]]></tex-math></inline-formula> as a solution to the equation <inline-formula><tex-math notation="LaTeX" id="ImEquation200"><![CDATA[$J_+ | j , j \rangle = 0$]]></tex-math></inline-formula>. The others follow as
<disp-formula id="ptx154-M37"><label>(37)</label><tex-math notation="LaTeX" id="Equation37"><![CDATA[
\begin{align}
\langle x |j , m \rangle \propto (J_-)^{j-m} \langle x | j , j \rangle = \frac{\Gamma(2j+1)}{\Gamma(j+m+1)} x^{j + m} \, .
\end{align}
]]></tex-math></disp-formula></p>
<p>The dual states <inline-formula><tex-math notation="LaTeX" id="ImEquation201"><![CDATA[$\langle j , m' |x \rangle $]]></tex-math></inline-formula> should satisfy
<disp-formula id="ptx154-M38"><label>(38)</label><tex-math notation="LaTeX" id="Equation38"><![CDATA[
\begin{align}
\int dx
\langle j , m' |x \rangle \langle x | j , m \rangle = \delta_{m,m'} \, ,
\end{align}
]]></tex-math></disp-formula>
which leads to
<disp-formula id="ptx154-M39"><label>(39)</label><tex-math notation="LaTeX" id="Equation39"><![CDATA[
\begin{align}
\langle j , m' |x \rangle \propto \partial_x^{j + m'} \delta (x) \, .
\end{align}
]]></tex-math></disp-formula></p>
<p>In particular, we have <inline-formula><tex-math notation="LaTeX" id="ImEquation202"><![CDATA[$\langle j , - j |x \rangle = \delta (x) $]]></tex-math></inline-formula> as in Eq. (<xref ref-type="disp-formula" rid="ptx154-M36">36</xref>). The normalization is set to be a convenient value.</p>
<p>We then apply the analysis to the case with generic <inline-formula><tex-math notation="LaTeX" id="ImEquation203"><![CDATA[$N$]]></tex-math></inline-formula>. A way to represent the generators of <inline-formula><tex-math notation="LaTeX" id="ImEquation204"><![CDATA[$\text{sl}(N)$]]></tex-math></inline-formula> is using <inline-formula><tex-math notation="LaTeX" id="ImEquation205"><![CDATA[$N \times N$]]></tex-math></inline-formula> matrices, and sl(2) generators <inline-formula><tex-math notation="LaTeX" id="ImEquation206"><![CDATA[$V^{2}_{n}$]]></tex-math></inline-formula> <inline-formula><tex-math notation="LaTeX" id="ImEquation207"><![CDATA[$(n=-1,0,1)$]]></tex-math></inline-formula> can be embedded as described, e.g., in Appendix A of Ref. [<xref ref-type="bibr" rid="B13">13</xref>]. Then the other generators may be obtained as
<disp-formula id="ptx154-M40"><label>(40)</label><tex-math notation="LaTeX" id="Equation40"><![CDATA[
\begin{align}
V^{s}_n = (-1)^{s-1-n} \frac{(n+s-1)!}{(2s - 2)!} [V_{-1}^2 [V_{-1}^2 , ... , [ V_{-1}^2 , (V_{1}^2)^{s-1} ]]] \, ,
\label{slNgenerators}
\end{align}
]]></tex-math></disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation208"><![CDATA[$(s - n - 1)$]]></tex-math></inline-formula> of <inline-formula><tex-math notation="LaTeX" id="ImEquation209"><![CDATA[$V_{-1}^2$]]></tex-math></inline-formula> are inserted. The fundamental representation of sl<inline-formula><tex-math notation="LaTeX" id="ImEquation210"><![CDATA[$(N)$]]></tex-math></inline-formula> can be described by an <inline-formula><tex-math notation="LaTeX" id="ImEquation211"><![CDATA[$N$]]></tex-math></inline-formula>-dimensional vector, which behaves as a spin-<inline-formula><tex-math notation="LaTeX" id="ImEquation212"><![CDATA[$(N-1)/2$]]></tex-math></inline-formula> representation under the action of the embedded sl<inline-formula><tex-math notation="LaTeX" id="ImEquation213"><![CDATA[$(2)$]]></tex-math></inline-formula>. Therefore, the description with <inline-formula><tex-math notation="LaTeX" id="ImEquation214"><![CDATA[$N \times N$]]></tex-math></inline-formula> matrices can be given by Eq. (<xref ref-type="disp-formula" rid="ptx154-M32">32</xref>) with <inline-formula><tex-math notation="LaTeX" id="ImEquation215"><![CDATA[$j= (N-1)/2$]]></tex-math></inline-formula> and open Wilson lines based on sl<inline-formula><tex-math notation="LaTeX" id="ImEquation216"><![CDATA[$(N)$]]></tex-math></inline-formula> algebra. In this specific case, we can map the matrix representation to the one with <inline-formula><tex-math notation="LaTeX" id="ImEquation217"><![CDATA[$x$]]></tex-math></inline-formula>-derivatives using Eqs. (<xref ref-type="disp-formula" rid="ptx154-M35">35</xref>) and (<xref ref-type="disp-formula" rid="ptx154-M40">40</xref>). In the representation with <inline-formula><tex-math notation="LaTeX" id="ImEquation218"><![CDATA[$x$]]></tex-math></inline-formula>-derivatives, the generators of sl<inline-formula><tex-math notation="LaTeX" id="ImEquation219"><![CDATA[$(N)$]]></tex-math></inline-formula> should be given by [<xref ref-type="bibr" rid="B39">39</xref>]
<disp-formula id="ptx154-M41"><label>(41)</label><tex-math notation="LaTeX" id="Equation41"><![CDATA[
\begin{align}
V^s_n = \sum_{i=0}^{s-1} (n - s + 1)_{s - 1 - i} a^{i} (s , h_0) x^{- n+i} \partial_x^{i} \, ,
\label{generators0}
\end{align}
]]></tex-math></disp-formula>
where
<disp-formula id="ptx154-M42"><label>(42)</label><tex-math notation="LaTeX" id="Equation42"><![CDATA[
\begin{align}
\quad a^i (s , h_0) = \binom{s-1}{i} \frac{(- 2 h_0 - s + 2)_{s - 1 - i}}{(s + i)_{s - 1 -i}}
\label{generators}
\end{align}
]]></tex-math></disp-formula>
with <inline-formula><tex-math notation="LaTeX" id="ImEquation220"><![CDATA[$h_0 = - j = (1 - N)/2$]]></tex-math></inline-formula>. The wave functions are precisely those in Eq. (<xref ref-type="disp-formula" rid="ptx154-M36">36</xref>). The generators (<xref ref-type="disp-formula" rid="ptx154-M41">41</xref>) with Eq. (<xref ref-type="disp-formula" rid="ptx154-M42">42</xref>) are those of higher-spin algebra hs<inline-formula><tex-math notation="LaTeX" id="ImEquation221"><![CDATA[$[\lambda]$]]></tex-math></inline-formula> for <inline-formula><tex-math notation="LaTeX" id="ImEquation222"><![CDATA[$h_0 = (1 + \lambda)/2 $]]></tex-math></inline-formula>, and sl<inline-formula><tex-math notation="LaTeX" id="ImEquation223"><![CDATA[$(N)$]]></tex-math></inline-formula> can be realized by hs<inline-formula><tex-math notation="LaTeX" id="ImEquation224"><![CDATA[$[-N]/\chi_N$]]></tex-math></inline-formula> with <inline-formula><tex-math notation="LaTeX" id="ImEquation225"><![CDATA[$\chi_N$]]></tex-math></inline-formula> as an ideal, which removes generators with <inline-formula><tex-math notation="LaTeX" id="ImEquation226"><![CDATA[$s > N$]]></tex-math></inline-formula>.</p>
<p>With the realization of generators, <inline-formula><tex-math notation="LaTeX" id="ImEquation227"><![CDATA[$N_s$]]></tex-math></inline-formula> in Eq. (<xref ref-type="disp-formula" rid="ptx154-M29">29</xref>) are computed as
<disp-formula id="ptx154-M43"><label>(43)</label><tex-math notation="LaTeX" id="Equation43"><![CDATA[
\begin{align}
N_s
= \frac{3 \sqrt{\pi } \Gamma (s) (1-N)_{s-1} (N+1)_{s-1}}{ 2^{2s-2} \left(N^2-1\right) \Gamma \left(s+\frac{1}{2}\right)} \, ,
\end{align}
]]></tex-math></disp-formula>
where the first few expressions are
<disp-formula id="ptx154-M44"><label>(44)</label><tex-math notation="LaTeX" id="Equation44"><![CDATA[
\begin{align}
N_2 = -1 \, , \quad N_3 = \frac{1}{5} (N^2 - 4) \, ,\quad N_4 = - \frac{3}{70} (N^2 - 4) (N^2 - 9) \, .
\end{align}
]]></tex-math></disp-formula></p>
<p>In particular, we have <inline-formula><tex-math notation="LaTeX" id="ImEquation228"><![CDATA[$N_3 = 1$]]></tex-math></inline-formula> for <inline-formula><tex-math notation="LaTeX" id="ImEquation229"><![CDATA[$N=3$]]></tex-math></inline-formula>.</p>
</sec>
<sec id="SEC3.3"><title>3.3. Correlators at the leading order in <inline-formula><tex-math notation="LaTeX" id="ImEquation230"><![CDATA[$1/c$]]></tex-math></inline-formula></title>
<p>In order to compute the correlators in Eq. (<xref ref-type="disp-formula" rid="ptx154-M3">3</xref>), we need to consider the expectation values of open Wilson lines with <inline-formula><tex-math notation="LaTeX" id="ImEquation231"><![CDATA[$| \text{hw} \rangle$]]></tex-math></inline-formula> corresponding to the highest weight in the fundamental representation of sl<inline-formula><tex-math notation="LaTeX" id="ImEquation232"><![CDATA[$(N)$]]></tex-math></inline-formula>. As explained above, they can be expressed for <inline-formula><tex-math notation="LaTeX" id="ImEquation233"><![CDATA[$(z_1,z_2) = (0,z)$]]></tex-math></inline-formula> as
<disp-formula id="ptx154-M45"><label>(45)</label><tex-math notation="LaTeX" id="Equation45"><![CDATA[
\begin{align}
W_{h_0} (z) &= \int dx \delta (x) P \exp \left[ \int^{z}_{0} d z ' \left( V_1^{2} - \frac{1}{\hat k} \sum_{s = 2}^N \frac{1}{N_s} J^{(s)} (z ') V^s_{-s + 1} \right) \right] \frac{1}{x^{2h_0}} \nonumber \\
&= \left. P \exp \left[ \int^{z}_{0} d z ' \left( V_1^{2} - \frac{1}{\hat k} \sum_{s = 2}^N \frac{1}{N_s} J^{(s)} (z ') V^s_{-s + 1} \right) \right] \frac{1}{x^{2h_0}} \right |_{x=0}
\label{Wilson}
\end{align}
]]></tex-math></disp-formula>
with <inline-formula><tex-math notation="LaTeX" id="ImEquation234"><![CDATA[$h_0= (1-N)/2$]]></tex-math></inline-formula>. Here the <inline-formula><tex-math notation="LaTeX" id="ImEquation235"><![CDATA[$\text{sl}(N)$]]></tex-math></inline-formula> generators are written in terms of <inline-formula><tex-math notation="LaTeX" id="ImEquation236"><![CDATA[$x$]]></tex-math></inline-formula>-derivatives as in Eq. (<xref ref-type="disp-formula" rid="ptx154-M42">42</xref>). We would like to treat them perturbatively in <inline-formula><tex-math notation="LaTeX" id="ImEquation237"><![CDATA[$1/\hat k$]]></tex-math></inline-formula> (or <inline-formula><tex-math notation="LaTeX" id="ImEquation238"><![CDATA[$1/c$]]></tex-math></inline-formula>). Following the analysis in Ref. [<xref ref-type="bibr" rid="B24">24</xref>], we compute
<disp-formula id="ptx154-M46"><label>(46)</label><tex-math notation="LaTeX" id="Equation46"><![CDATA[
\begin{align}
\frac{d}{dz} \left[e^{-z \partial_x } W_{h_0} (z) \right]
= \left( - \frac{1}{\hat k} \sum_{s = 2}^N \frac{1}{N_s} J^{(s)} (z) e^{- z\partial_x } V^s_{-s + 1} e^{ z \partial_x } \right) \left[e^{- z\partial_x } W_{h_0} (z) \right] \, .
\end{align}
]]></tex-math></disp-formula></p>
<p>Integrating over <inline-formula><tex-math notation="LaTeX" id="ImEquation239"><![CDATA[$z$]]></tex-math></inline-formula>, we find
<disp-formula id="ptx154-M47"><label>(47)</label><tex-math notation="LaTeX" id="Equation47"><![CDATA[
\begin{align}
\label{Wilson1/c}
W_{h_0} (z) & = \sum_{n=0}^\infty \left( - \frac{1}{\hat k} \right )^n
\int_0^z dz_n \cdots \int_0^{z_2} dz_1 \sum_{s_j = 2}^N
\left[ \prod_{j=1}^n \frac{1 }{N_{s_j}} J^{(s_j)} (z_j) \right]
f_n^{(s_n,\ldots , s_1)} (z_n ,\ldots , z_1) \, ,
\end{align}
]]></tex-math></disp-formula>
where
<disp-formula id="ptx154-M48"><label>(48)</label><tex-math notation="LaTeX" id="Equation48"><![CDATA[
\begin{align}
\label{fnss}
&f_n^{(s_n,\ldots , s_1)} (z_n ,\ldots , z_1) \nonumber\\
& \quad = \left.
\prod_{j=1}^n \left[
\sum_{i=0}^{s_j-1} ( - 2 s_j + 2)_{s_j - 1 - i} a^{i} (s_j , h_0) (x + z - z_j)^{s_j - 1+i} \partial_x^{i} \right] \frac{1}{(x + z)^{2h_0}} \right |_{x=0} \, ;
\end{align}
]]></tex-math></disp-formula>
see Eq. (3.3) of Ref. [<xref ref-type="bibr" rid="B23">23</xref>] for <inline-formula><tex-math notation="LaTeX" id="ImEquation240"><![CDATA[$N=2$]]></tex-math></inline-formula>.</p>
<p>According to the current prescription, the two-point function of <inline-formula><tex-math notation="LaTeX" id="ImEquation241"><![CDATA[$\mathcal{O}_{h_+}$]]></tex-math></inline-formula> in Eq. (<xref ref-type="disp-formula" rid="ptx154-M3">3</xref>) should be computed as
<disp-formula id="ptx154-M49"><label>(49)</label><tex-math notation="LaTeX" id="Equation49"><![CDATA[
\begin{align}
\langle \mathcal{O}_{h_+} (z) \bar{\mathcal{O}}_{h_+} (0) \rangle = \langle W_{h_0} (z) \rangle \, ,
\label{2ptWilson}
\end{align}
]]></tex-math></disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation242"><![CDATA[$\langle W_{h_0} (z) \rangle$]]></tex-math></inline-formula> is evaluated by the correlators of <inline-formula><tex-math notation="LaTeX" id="ImEquation243"><![CDATA[$J^{(s)}$]]></tex-math></inline-formula> in the W<inline-formula><tex-math notation="LaTeX" id="ImEquation244"><![CDATA[$_N$]]></tex-math></inline-formula> theory. The leading-order expansion in <inline-formula><tex-math notation="LaTeX" id="ImEquation245"><![CDATA[$1/\hat k$]]></tex-math></inline-formula> leads to
<disp-formula id="ptx154-M50"><label>(50)</label><tex-math notation="LaTeX" id="Equation50"><![CDATA[
\begin{align}
\left. \langle \mathcal{O}_{h_+} (z) \bar{\mathcal{O}}_{h_+} (0) \rangle \right|_{\mathcal{O} (c^0) }= \left. \langle W_{h_0} (z) \rangle \right|_{\mathcal{O} (c^0) }=
\frac{1}{z^{2h_0}}
\end{align}
]]></tex-math></disp-formula>
as expected.</p>
<p>We are also interested in the three-point functions in Eq. (<xref ref-type="disp-formula" rid="ptx154-M3">3</xref>), which should be obtained as
<disp-formula id="ptx154-M51"><label>(51)</label><tex-math notation="LaTeX" id="Equation51"><![CDATA[
\begin{align}
\langle \mathcal{O}_{h_+} (z) \bar{\mathcal{O}}_{h_+} (0) J^{(s)} (y) \rangle =
\langle W_{h_0} (z) J^{(s)} (y) \rangle \, .
\label{3ptWilson}
\end{align}
]]></tex-math></disp-formula></p>
<p>The first nontrivial contributions come from the terms of order <inline-formula><tex-math notation="LaTeX" id="ImEquation246"><![CDATA[$1/\hat k$]]></tex-math></inline-formula>. At this order, we need to compute
<disp-formula id="ptx154-M52"><label>(52)</label><tex-math notation="LaTeX" id="Equation52"><![CDATA[
\begin{align}
\left. \langle W_{h_0} (z) J^{(s)} (y) \rangle \right|_{\mathcal{O} (c^{0}) } &= - \frac{1}{\hat k N_{s}}
\int_0^z dz_1 f^{(s)}_1 (z_1) \langle J^{(s)} (z_1) J^{(s)} (y) \rangle \\
& = - \frac{1}{\hat k N_{s}}
\int_0^z dz_1 \frac{\Gamma (2h _0+ s - 1)}{\Gamma (2 h_0)}\frac{ (z - z_1)^{s-1} z_1^{s-1}}{ z^{ s -1 + 2h_0}} \langle J^{(s)} (z_1) J^{(s)} (y) \rangle \, . \nonumber
\end{align}
]]></tex-math></disp-formula></p>
<p>The normalization of higher-spin currents in Eq. (<xref ref-type="disp-formula" rid="ptx154-M29">29</xref>) corresponds to (see, e.g., Ref. [<xref ref-type="bibr" rid="B40">40</xref>])
<disp-formula id="ptx154-M53"><label>(53)</label><tex-math notation="LaTeX" id="Equation53"><![CDATA[
\begin{align}
\left. \langle J^{(s)} (z_1) J^{(s)} (z_2) \rangle \right|_{\mathcal{O} (c) } = - (2 s -1) \hat k N_s \frac{1}{z_{12}^{2s}} \, .
\label{2ptnorm}
\end{align}
]]></tex-math></disp-formula></p>
<p>Using
<disp-formula id="ptx154-M54"><label>(54)</label><tex-math notation="LaTeX" id="Equation54"><![CDATA[
\begin{align}
\int_0^z dz_1 \frac{(z - z_1)^{s-1} z_1^{s-1}}{(z_1 - y)^{2s} }
= \frac{z^{2s -1}}{( y- z)^s y^s} \frac{(\Gamma(s))^2}{\Gamma (2s)} \, ,
\end{align}
]]></tex-math></disp-formula>
we find
<disp-formula id="ptx154-M55"><label>(55)</label><tex-math notation="LaTeX" id="Equation55"><![CDATA[
\begin{align}
\left. \langle W_{h_0} (z) J^{(s)} (y) \rangle \right|_{\mathcal{O} (c^{0}) } = \frac{\Gamma (2h_0 + s - 1)}{\Gamma (2 h_0)}
\frac{(\Gamma(s))^2}{\Gamma (2s - 1)}
\left( \frac{z}{(y-z) y} \right)^s \left. \langle W_{h_0} (z) \rangle \right|_{\mathcal{O} (c^0) } \, . \label{3pttree}
\end{align}
]]></tex-math></disp-formula></p>
<p>The result is consistent with Eq. (<xref ref-type="disp-formula" rid="ptx154-M22">22</xref>) in the convention of Eq. (<xref ref-type="disp-formula" rid="ptx154-M53">53</xref>). In fact, it is the same as Eq. (1.3) of Ref. [<xref ref-type="bibr" rid="B40">40</xref>] up to a factor if we set <inline-formula><tex-math notation="LaTeX" id="ImEquation247"><![CDATA[$h_0 = (1 + \lambda)/2$]]></tex-math></inline-formula> (or <inline-formula><tex-math notation="LaTeX" id="ImEquation248"><![CDATA[$N = - \lambda$]]></tex-math></inline-formula>), and this is related to the triality relation discussed in Ref. [<xref ref-type="bibr" rid="B14">14</xref>].</p>
</sec>
<sec id="SEC3.4"><title>3.4. Prescription for regularization</title>
<p>The <inline-formula><tex-math notation="LaTeX" id="ImEquation249"><![CDATA[$1/c$]]></tex-math></inline-formula> corrections of the two- and three-point functions in Eq. (<xref ref-type="disp-formula" rid="ptx154-M3">3</xref>) can be evaluated from higher-order contributions in Eq. (<xref ref-type="disp-formula" rid="ptx154-M47">47</xref>) using the Wilson line method. However, integrals over <inline-formula><tex-math notation="LaTeX" id="ImEquation250"><![CDATA[$z_j$]]></tex-math></inline-formula> diverge when two (or more) currents <inline-formula><tex-math notation="LaTeX" id="ImEquation251"><![CDATA[$J(z_i)$]]></tex-math></inline-formula> collide. Therefore, we need to decide how to deal with these divergences, and we explain our prescription in this subsection.</p>
<p>Let us start with the correlators of higher-spin currents, which are uniquely fixed by the W<inline-formula><tex-math notation="LaTeX" id="ImEquation252"><![CDATA[$_N$]]></tex-math></inline-formula> symmetry in terms of central charge <inline-formula><tex-math notation="LaTeX" id="ImEquation253"><![CDATA[$c$]]></tex-math></inline-formula>. In particular, we use the two-point functions
<disp-formula id="ptx154-M56"><label>(56)</label><tex-math notation="LaTeX" id="Equation56"><![CDATA[
\begin{align}
\langle J^{(s)} (z_2) J^{(s)} (z_1) \rangle = - \frac{ (2 s -1) c N_s}{6} \frac{1}{z_{21}^{2s}} \, ,
\label{2ptnormc}
\end{align}
]]></tex-math></disp-formula>
which reduce to Eq. (<xref ref-type="disp-formula" rid="ptx154-M53">53</xref>) if we use the relation <inline-formula><tex-math notation="LaTeX" id="ImEquation254"><![CDATA[$c=6 \hat k$]]></tex-math></inline-formula> in Eq. (<xref ref-type="disp-formula" rid="ptx154-M30">30</xref>). At finite <inline-formula><tex-math notation="LaTeX" id="ImEquation255"><![CDATA[$\hat k$]]></tex-math></inline-formula>, the relation of Eq. (<xref ref-type="disp-formula" rid="ptx154-M30">30</xref>) should be modified, and corrections to higher-spin propagators are automatically included by expanding in <inline-formula><tex-math notation="LaTeX" id="ImEquation256"><![CDATA[$1/c$]]></tex-math></inline-formula> instead of <inline-formula><tex-math notation="LaTeX" id="ImEquation257"><![CDATA[$1/\hat k$]]></tex-math></inline-formula>; see Ref. [<xref ref-type="bibr" rid="B24">24</xref>] for some arguments. Divergence would arise at the coincident point <inline-formula><tex-math notation="LaTeX" id="ImEquation258"><![CDATA[$z_2 = z_1$]]></tex-math></inline-formula>, and we need to decide how to regularize it. We introduce a regulator as
<disp-formula id="ptx154-M57"><label>(57)</label><tex-math notation="LaTeX" id="Equation57"><![CDATA[
\begin{align}
\langle J^{(s)} (z_2) J^{(s)} (z_1) \rangle = - \frac{ (2 s -1) c N_s}{6} \frac{1}{z_{21}^{2s - 2 \epsilon}}
\label{2ptnormreg}
\end{align}
]]></tex-math></disp-formula>
by shifting the conformal weight of the higher-spin current as <inline-formula><tex-math notation="LaTeX" id="ImEquation259"><![CDATA[$s \to s - \epsilon$]]></tex-math></inline-formula>. This choice is reasonable since it does not break the scaling symmetry. Analogously, we introduce the regulator <inline-formula><tex-math notation="LaTeX" id="ImEquation260"><![CDATA[$\epsilon$]]></tex-math></inline-formula> to other correlators of higher-spin currents <inline-formula><tex-math notation="LaTeX" id="ImEquation261"><![CDATA[$J^{(s)}$]]></tex-math></inline-formula> by shifting the conformal wights of the current.</p>
<p>Introducing the regulator <inline-formula><tex-math notation="LaTeX" id="ImEquation262"><![CDATA[$\epsilon$]]></tex-math></inline-formula>, integrals over <inline-formula><tex-math notation="LaTeX" id="ImEquation263"><![CDATA[$z_j$]]></tex-math></inline-formula> become finite but have terms diverging at <inline-formula><tex-math notation="LaTeX" id="ImEquation264"><![CDATA[$\epsilon \to 0$]]></tex-math></inline-formula>. In the usual quantum field theory with a renormalizable Lagrangian, we can remove divergences by renormalizing the overall normalization of quantum fields and the parameters of interactions. In the current case, we offer to remove divergences in a similar manner. We first use the fact that the normalization of a two-point function can be chosen arbitrarily by the redefinition of the operator. We remove a kind of divergence by changing the overall factor of the open Wilson line such that the corresponding two-point function becomes the normalized one as in Eq. (<xref ref-type="disp-formula" rid="ptx154-M6">6</xref>). We then notice that the three-point interactions between two scalars and a higher-spin field are governed by the coefficients in front of <inline-formula><tex-math notation="LaTeX" id="ImEquation265"><![CDATA[$J^{(s)} (z)$]]></tex-math></inline-formula> in Eq. (<xref ref-type="disp-formula" rid="ptx154-M45">45</xref>). We introduce parameters <inline-formula><tex-math notation="LaTeX" id="ImEquation266"><![CDATA[$c_s$]]></tex-math></inline-formula> such that Eq. (<xref ref-type="disp-formula" rid="ptx154-M45">45</xref>) becomes
<disp-formula id="ptx154-M58"><label>(58)</label><tex-math notation="LaTeX" id="Equation58"><![CDATA[
\begin{align}
W_{h_0} (z) = \left. P \exp \left[ \int^{z}_{0} d z ' ( V_1^{2} - \frac{6}{c} \sum_{s =2}^N \frac{c_s}{N_s} J^{(s)} (z ') V^s_{-s + 1} ) \right] \frac{1}{x^{2h_0}} \right |_{x=0} \, .
\label{Wilsonreg}
\end{align}
]]></tex-math></disp-formula></p>
<p>In terms of <inline-formula><tex-math notation="LaTeX" id="ImEquation267"><![CDATA[$1/c$]]></tex-math></inline-formula> expansion, Eq. (<xref ref-type="disp-formula" rid="ptx154-M47">47</xref>) is changed as
<disp-formula id="ptx154-M59"><label>(59)</label><tex-math notation="LaTeX" id="Equation59"><![CDATA[
\begin{align}
\label{Wilson1/creg}
W_{h_0} (z) & = \sum_{n=0}^\infty \left( - \frac{6}{c} \right )^n
\int_0^z dz_n \cdots \int_0^{z_2} dz_1 \sum_{s_j = 2}^N
\left[ \prod_{j=1}^n \frac{c_{s_j}}{N_{s_j}} J^{(s_j)} (z_j) \right]
f_n^{(s_n,\ldots , s_1)} (z_n ,\ldots , z_1) \, ,
\end{align}
]]></tex-math></disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation268"><![CDATA[$f_n^{(s_n,\ldots , s_1)} (z_n ,\ldots , z_1) $]]></tex-math></inline-formula> are given by Eq. (<xref ref-type="disp-formula" rid="ptx154-M48">48</xref>). At the leading order in <inline-formula><tex-math notation="LaTeX" id="ImEquation269"><![CDATA[$1/c$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation270"><![CDATA[$c = 6 \hat k$]]></tex-math></inline-formula> as in Eq. (<xref ref-type="disp-formula" rid="ptx154-M30">30</xref>) and <inline-formula><tex-math notation="LaTeX" id="ImEquation271"><![CDATA[$c_s = 1$]]></tex-math></inline-formula>. From the next order in <inline-formula><tex-math notation="LaTeX" id="ImEquation272"><![CDATA[$1/c$]]></tex-math></inline-formula>, we shift the values of <inline-formula><tex-math notation="LaTeX" id="ImEquation273"><![CDATA[$c_s$]]></tex-math></inline-formula> to remove divergences. Namely, we expand <inline-formula><tex-math notation="LaTeX" id="ImEquation274"><![CDATA[$c_s$]]></tex-math></inline-formula> in <inline-formula><tex-math notation="LaTeX" id="ImEquation275"><![CDATA[$1/c$]]></tex-math></inline-formula> as
<disp-formula id="ptx154-M60"><label>(60)</label><tex-math notation="LaTeX" id="Equation60"><![CDATA[
\begin{align}
c_s = 1 + \frac{1}{c} c_s^{(1)} + \frac{1}{c^2} c_s^{(2)} + \mathcal{O} (c^{-2}) \, ,
\label{csexp}
\end{align}
]]></tex-math></disp-formula>
and absorb divergences in <inline-formula><tex-math notation="LaTeX" id="ImEquation276"><![CDATA[$c_s^{(i)}$]]></tex-math></inline-formula> <inline-formula><tex-math notation="LaTeX" id="ImEquation277"><![CDATA[$(i=1,2,\ldots)$]]></tex-math></inline-formula> order by order. We conjecture that all divergences can be removed by these two methods of renormalization.</p>
<p>As explained above, we decide to remove divergences by properly choosing the &#x201C;bare&#x201D; values of parameters <inline-formula><tex-math notation="LaTeX" id="ImEquation278"><![CDATA[$c_s$]]></tex-math></inline-formula>. However, we have still freedom to choose the terms independent of <inline-formula><tex-math notation="LaTeX" id="ImEquation279"><![CDATA[$\epsilon$]]></tex-math></inline-formula>. Here we fix them such that the three-point functions <inline-formula><tex-math notation="LaTeX" id="ImEquation280"><![CDATA[$\langle \mathcal{O}_{h_+} \bar{\mathcal{O}}_{h_+} J^{(s)} \rangle$]]></tex-math></inline-formula> in Eq. (<xref ref-type="disp-formula" rid="ptx154-M3">3</xref>) are reproduced from the Wilson line method as in Eq. (<xref ref-type="disp-formula" rid="ptx154-M51">51</xref>). Since the three-point functions can be fixed by the W<inline-formula><tex-math notation="LaTeX" id="ImEquation281"><![CDATA[$_N$]]></tex-math></inline-formula> symmetry as shown in the previous section, we would say that the regularization scheme is determined by making use of the boundary symmetry. This is expected to fix all the ambiguities left, and the other physical quantities should be predictable. In the following two sections, we examine concrete examples with <inline-formula><tex-math notation="LaTeX" id="ImEquation282"><![CDATA[$N=2,3$]]></tex-math></inline-formula> and show that the <inline-formula><tex-math notation="LaTeX" id="ImEquation283"><![CDATA[$1/c$]]></tex-math></inline-formula> corrections in the conformal dimensions of scalar operators can be reproduced from the bulk viewpoint up to the two-loop level applying the prescription described above.</p>
</sec>
</sec>
<sec id="SEC4"><title>4. Correlators for <inline-formula><tex-math notation="LaTeX" id="ImEquation284"><![CDATA[$\boldsymbol{N=2}$]]></tex-math></inline-formula></title>
<p>In this and the next section, we explicitly evaluate the loop corrections of the correlators in terms of open Wilson lines. We start with the simpler case with <inline-formula><tex-math notation="LaTeX" id="ImEquation285"><![CDATA[$N=2$]]></tex-math></inline-formula> and then move to a more involved one with <inline-formula><tex-math notation="LaTeX" id="ImEquation286"><![CDATA[$N=3$]]></tex-math></inline-formula>. For <inline-formula><tex-math notation="LaTeX" id="ImEquation287"><![CDATA[$N=2$]]></tex-math></inline-formula>, we can work with generic <inline-formula><tex-math notation="LaTeX" id="ImEquation288"><![CDATA[$h_0 = -j$]]></tex-math></inline-formula>, because the sl(2) generators in terms of <inline-formula><tex-math notation="LaTeX" id="ImEquation289"><![CDATA[$x$]]></tex-math></inline-formula>-derivatives as in Eq. (<xref ref-type="disp-formula" rid="ptx154-M35">35</xref>) are available for the generic case as argued in <xref ref-type="sec" rid="SEC3.2">Sect. 3.2</xref>.</p>
<p>Two- and three-point functions with generic <inline-formula><tex-math notation="LaTeX" id="ImEquation290"><![CDATA[$h_0 $]]></tex-math></inline-formula> are obtained from analysis of conformal field theory as follows. For <inline-formula><tex-math notation="LaTeX" id="ImEquation291"><![CDATA[$h_0 = - j$]]></tex-math></inline-formula>, the <inline-formula><tex-math notation="LaTeX" id="ImEquation292"><![CDATA[$1/c$]]></tex-math></inline-formula> correction of conformal weight is given as Eq. (<xref ref-type="disp-formula" rid="ptx154-M9">9</xref>) with
<disp-formula id="ptx154-M61"><label>(61)</label><tex-math notation="LaTeX" id="Equation61"><![CDATA[
\begin{align}
h_1 = - 6 h_0 (h_0-1) \, , \quad h_2 = - 78 h_0 (h_0-1) \, ;
\label{dimcorr}
\end{align}
]]></tex-math></disp-formula>
see, e.g., Ref. [<xref ref-type="bibr" rid="B24">24</xref>]. The <inline-formula><tex-math notation="LaTeX" id="ImEquation293"><![CDATA[$1/c$]]></tex-math></inline-formula> expansion of the two-point function is then Eq. (<xref ref-type="disp-formula" rid="ptx154-M10">10</xref>). In the next subsection, we examine the two-point function at the next leading order in <inline-formula><tex-math notation="LaTeX" id="ImEquation294"><![CDATA[$1/c$]]></tex-math></inline-formula>. We reproduce the order-<inline-formula><tex-math notation="LaTeX" id="ImEquation295"><![CDATA[$1/c$]]></tex-math></inline-formula> result as <inline-formula><tex-math notation="LaTeX" id="ImEquation296"><![CDATA[$h_1$]]></tex-math></inline-formula> in Eq. (<xref ref-type="disp-formula" rid="ptx154-M61">61</xref>), and remove a divergence by renormalizing the overall factor of the open Wilson line. The three-point function is fixed by the conformal Ward identity as
<disp-formula id="ptx154-M62"><label>(62)</label><tex-math notation="LaTeX" id="Equation62"><![CDATA[
\begin{align}
\langle \mathcal{O}_h (z) \bar{\mathcal{O}}_h (0) J^{(2)} (y) \rangle =\left[ h_0 + \frac1c h_1 \right] \left( \frac{z}{(y - z) y} \right)^2 \langle \mathcal{O}_{h} (z) \bar{\mathcal{O}}_{h} (0) \rangle + \mathcal{O}(c^{-2})
\label{Ward}
\end{align}
]]></tex-math></disp-formula>
in the current convention of <inline-formula><tex-math notation="LaTeX" id="ImEquation297"><![CDATA[$J^{(2)}$]]></tex-math></inline-formula> given by Eq. (<xref ref-type="disp-formula" rid="ptx154-M56">56</xref>). The <inline-formula><tex-math notation="LaTeX" id="ImEquation298"><![CDATA[$c^0$]]></tex-math></inline-formula>-order term follows from Eq. (<xref ref-type="disp-formula" rid="ptx154-M55">55</xref>). In <xref ref-type="sec" rid="SEC4.2">Sect. 4.2</xref>, we fix the parameter <inline-formula><tex-math notation="LaTeX" id="ImEquation299"><![CDATA[$c_2$]]></tex-math></inline-formula> introduced in Eq. (<xref ref-type="disp-formula" rid="ptx154-M58">58</xref>) such that the <inline-formula><tex-math notation="LaTeX" id="ImEquation300"><![CDATA[$1/c$]]></tex-math></inline-formula>-order term is reproduced. In particular, this removes another type of divergence. With the regularization scheme, we reproduce the order-<inline-formula><tex-math notation="LaTeX" id="ImEquation301"><![CDATA[$1/c^2$]]></tex-math></inline-formula> term as <inline-formula><tex-math notation="LaTeX" id="ImEquation302"><![CDATA[$h_2$]]></tex-math></inline-formula> in Eq. (<xref ref-type="disp-formula" rid="ptx154-M61">61</xref>) from the two-point function at two-loop order in <xref ref-type="sec" rid="SEC4.3">Sect. 4.3</xref>.</p>
<sec id="SEC4.1"><title>4.1. Two-point function at <inline-formula><tex-math notation="LaTeX" id="ImEquation303"><![CDATA[$1/c$]]></tex-math></inline-formula> order</title>
<p>For the two-point function of <inline-formula><tex-math notation="LaTeX" id="ImEquation304"><![CDATA[$\mathcal{O}_h$]]></tex-math></inline-formula>, we need to evaluate the expectation value of the open Wilson line <inline-formula><tex-math notation="LaTeX" id="ImEquation305"><![CDATA[$W_{h_0} (z)$]]></tex-math></inline-formula> as in Eq. (<xref ref-type="disp-formula" rid="ptx154-M49">49</xref>). With <inline-formula><tex-math notation="LaTeX" id="ImEquation306"><![CDATA[$N=2$]]></tex-math></inline-formula>, the <inline-formula><tex-math notation="LaTeX" id="ImEquation307"><![CDATA[$1/c$]]></tex-math></inline-formula> expansion of the open Wilson line in Eq. (<xref ref-type="disp-formula" rid="ptx154-M59">59</xref>) becomes
<disp-formula id="ptx154-M63"><label>(63)</label><tex-math notation="LaTeX" id="Equation63"><![CDATA[
\begin{align}
W_{h_0} (z) = \frac{1}{z^{2h_0}} + \sum_{n =1} \left( \frac{6 c_2}{c} \right)^n W^{(n)}_{h_0} (z)
\label{Wexp}
\end{align}
]]></tex-math></disp-formula>
with
<disp-formula id="ptx154-M64"><label>(64)</label><tex-math notation="LaTeX" id="Equation64"><![CDATA[
\begin{align}
W^{(1)}_{h_0} (z) &= \int_0^z d z_1 f_1^{(2)} ( z_1) J^{(2)} (z_1) \, , \nonumber \\
W^{(2)}_{h_0} (z) &= \int_0^z d z_2 \int_0^{z_2} dz_1 f_2^{(2,2)} (z_2,z_1)
J^{(2)} (z_2) J^{(2)} (z_1) \, , \label{Wexpe} \nonumber\\
W^{(3)}_{h_0} (z) &= \int_0^z d z_3 \int_0^{z_3} d z_2 \int_0^{z_2} dz_1 f_3^{(2,2,2)} ( z_3,z_2 ,z_1) J^{(2)} (z_3)J^{(2)} (z_2)J^{(2)} (z_1) \, , \nonumber \\
W^{(4)}_{h_0} (z) &= \int_0^z d z_4 \cdots \int_0^{z_2} dz_1 f_4^{(2,2,2,2)} ( z_4,z_3 ,z_2,z_1) J^{(2)} (z_4)J^{(2)} (z_3) J^{(2)} (z_2) J^{(2)} (z_1) \, ,
\end{align}
]]></tex-math></disp-formula>
and so on. Here <inline-formula><tex-math notation="LaTeX" id="ImEquation308"><![CDATA[$f_n^{(2,\ldots,2)} (z_n , \ldots , z_1)$]]></tex-math></inline-formula> are defined in Eq. (<xref ref-type="disp-formula" rid="ptx154-M48">48</xref>). Since the one-point function vanishes as <inline-formula><tex-math notation="LaTeX" id="ImEquation309"><![CDATA[$\langle J^{(2)} (z) \rangle = 0$]]></tex-math></inline-formula>, the nontrivial contribution starts from <inline-formula><tex-math notation="LaTeX" id="ImEquation310"><![CDATA[$\langle W^{(2)}_{h_0} (z) \rangle$]]></tex-math></inline-formula>. The contribution corresponds to the one-loop correction in the two-point function of <inline-formula><tex-math notation="LaTeX" id="ImEquation311"><![CDATA[$\mathcal{O}_h$]]></tex-math></inline-formula> as in <xref ref-type="fig" rid="F1">Fig. 1</xref>.</p>
<fig id="F1" orientation="portrait" position="float"><label>Fig. 1.</label><caption><p>Diagram contributing to the <inline-formula><tex-math notation="LaTeX" id="ImEquation312"><![CDATA[$1/c$]]></tex-math></inline-formula>-order correction of <inline-formula><tex-math notation="LaTeX" id="ImEquation313"><![CDATA[$\langle \mathcal{O}_h \bar{\mathcal{O}}_h \rangle$]]></tex-math></inline-formula> for <inline-formula><tex-math notation="LaTeX" id="ImEquation314"><![CDATA[$N=2$]]></tex-math></inline-formula>. The straight line and the wavy line represent the open Wilson line and the propagator of spin-two current.</p></caption>
<graphic xmlns:xlink="http://www.w3.org/1999/xlink" orientation="portrait" position="float" xlink:href="ptx154F1.tif"/></fig>
<p>The integrals in <inline-formula><tex-math notation="LaTeX" id="ImEquation315"><![CDATA[$\langle W^{(2)}_{h_0} (z) \rangle$]]></tex-math></inline-formula> over <inline-formula><tex-math notation="LaTeX" id="ImEquation316"><![CDATA[$z_1,z_2$]]></tex-math></inline-formula> diverge, and we introduce a regulator <inline-formula><tex-math notation="LaTeX" id="ImEquation317"><![CDATA[$\epsilon$]]></tex-math></inline-formula> as in Eq. (<xref ref-type="disp-formula" rid="ptx154-M57">57</xref>), i.e.,
<disp-formula id="ptx154-M65"><label>(65)</label><tex-math notation="LaTeX" id="Equation65"><![CDATA[
\begin{align}
\langle J^{(2)} (z_2) J^{(2)} (z_1) \rangle = \frac{c/2}{z_{21}^{4 - 2 \epsilon}}
\end{align}
]]></tex-math></disp-formula>
for spin-two current. With the regulator, we obtain a finite result after the integration over <inline-formula><tex-math notation="LaTeX" id="ImEquation318"><![CDATA[$z_1,z_2$]]></tex-math></inline-formula> as
<disp-formula id="ptx154-M66"><label>(66)</label><tex-math notation="LaTeX" id="Equation66"><![CDATA[
\begin{align}
\langle W^{(2)}_{h_0} (z) \rangle &= \int_0^z d z_2 \int_0^{z_2} dz_1 f_2 ^{(2,2)} (z_2,z_1)
\langle J^{(2)} (z_2) J^{(2)} (z_1) \rangle \nonumber \\
& = \frac{c}{2 z^{2h_0}} \left[ \frac{(h_0-1) h_0 }{3 \epsilon}+\frac{1}{9} h_0 \left(6 (h_0-1) \log \left(z\right)+5 h_0-2\right) \right] + \mathcal{O} (\epsilon) \, .
\label{W2}
\end{align}
]]></tex-math></disp-formula></p>
<p>Using Eq. (<xref ref-type="disp-formula" rid="ptx154-M63">63</xref>) and <inline-formula><tex-math notation="LaTeX" id="ImEquation319"><![CDATA[$c_2 = 1 + \mathcal{O}(c^{-1})$]]></tex-math></inline-formula>, the above expression leads to
<disp-formula id="ptx154-M67"><label>(67)</label><tex-math notation="LaTeX" id="Equation67"><![CDATA[
\begin{align}
\langle W_{h_0} (z) \rangle = \frac{1}{z^{2h_0}} \left[ 1 + \frac{1}{c}\left(\frac{6(h_0-1) h_0 }{ \epsilon} + \left(12 h_0 (h_0 -1) \log \left(z\right)+2 h_0 (5 h_0 -2 ) \right) \right)\right]
\label{2pt1}
\end{align}
]]></tex-math></disp-formula>
up to the terms of order <inline-formula><tex-math notation="LaTeX" id="ImEquation320"><![CDATA[$\epsilon^0$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation321"><![CDATA[$1/c$]]></tex-math></inline-formula>.</p>
<p>We compare the above expression in Eq. (<xref ref-type="disp-formula" rid="ptx154-M67">67</xref>) with the <inline-formula><tex-math notation="LaTeX" id="ImEquation322"><![CDATA[$1/c$]]></tex-math></inline-formula> expansion of the two-point function in Eq. (<xref ref-type="disp-formula" rid="ptx154-M10">10</xref>). We can see that the <inline-formula><tex-math notation="LaTeX" id="ImEquation323"><![CDATA[$\log (z)$]]></tex-math></inline-formula> term correctly explains <inline-formula><tex-math notation="LaTeX" id="ImEquation324"><![CDATA[$h_1 = - 6 h_0 (h_0-1)$]]></tex-math></inline-formula> in Eq. (<xref ref-type="disp-formula" rid="ptx154-M61">61</xref>), as shown in Ref. [<xref ref-type="bibr" rid="B24">24</xref>]. The expression in Eq. (<xref ref-type="disp-formula" rid="ptx154-M67">67</xref>) has a term proportional to <inline-formula><tex-math notation="LaTeX" id="ImEquation325"><![CDATA[$1/\epsilon$]]></tex-math></inline-formula>, which diverges for <inline-formula><tex-math notation="LaTeX" id="ImEquation326"><![CDATA[$\epsilon \to 0$]]></tex-math></inline-formula>. We can remove the divergence by changing the overall factor of the open Wilson line as
<disp-formula id="ptx154-M68"><label>(68)</label><tex-math notation="LaTeX" id="Equation68"><![CDATA[
\begin{align}
\tilde W_{h_0} (z) = \left[ 1 - \frac{1}{c}\left(\frac{6(h_0-1) h_0 }{ \epsilon} + 2 h_0 (5 h_0 -2 ) \right)\right] W_{h_0} (z) \, .
\label{overall}
\end{align}
]]></tex-math></disp-formula></p>
<p>With the normalization, we have
<disp-formula id="ptx154-M69"><label>(69)</label><tex-math notation="LaTeX" id="Equation69"><![CDATA[
\begin{align}
\langle \tilde W_{h_0} (z) \rangle = \frac{1}{z^{2 (h_0 + h_1/c)}} + \mathcal{O} (c^{-2})
\end{align}
]]></tex-math></disp-formula>
for <inline-formula><tex-math notation="LaTeX" id="ImEquation327"><![CDATA[$\epsilon \to 0$]]></tex-math></inline-formula>. In other words, we choose the <inline-formula><tex-math notation="LaTeX" id="ImEquation328"><![CDATA[$\epsilon$]]></tex-math></inline-formula>-independent part such that the corresponding two-point function has unit normalization as in Eq. (<xref ref-type="disp-formula" rid="ptx154-M6">6</xref>).</p>
</sec>
<sec id="SEC4.2"><title>4.2. Three-point function</title>
<p>We have proposed that three-point functions can be computed with open Wilson lines as in Eq. (<xref ref-type="disp-formula" rid="ptx154-M51">51</xref>) and reproduced the tree-level results as in Eq. (<xref ref-type="disp-formula" rid="ptx154-M55">55</xref>). In this subsection, we examine the next leading order in <inline-formula><tex-math notation="LaTeX" id="ImEquation329"><![CDATA[$1/c$]]></tex-math></inline-formula>. There are two types of contribution at the order as in <xref ref-type="fig" rid="F2">Fig. 2</xref> and we would like to examine them in turn.</p>
<fig id="F2" orientation="portrait" position="float"><label>Fig. 2.</label><caption><p>Diagrams contributing to the <inline-formula><tex-math notation="LaTeX" id="ImEquation330"><![CDATA[$1/c$]]></tex-math></inline-formula>-order correction of <inline-formula><tex-math notation="LaTeX" id="ImEquation331"><![CDATA[$\langle \mathcal{O}_h \bar{\mathcal{O}}_h J^{(2)} \rangle$]]></tex-math></inline-formula> for <inline-formula><tex-math notation="LaTeX" id="ImEquation332"><![CDATA[$N=2$]]></tex-math></inline-formula>.</p></caption>
<graphic xmlns:xlink="http://www.w3.org/1999/xlink" orientation="portrait" position="float" xlink:href="ptx154F2.tif"/></fig>
<p>The first one is from
<disp-formula id="ptx154-M70"><label>(70)</label><tex-math notation="LaTeX" id="Equation70"><![CDATA[
\begin{align}
\langle W_{h_0}^{(2)} (z) J^{(2)} (y) \rangle = \int_0^z d z_2 \int_0^{z_2} dz_1 f_2^{(2,2)} (z_2,z_1)
\langle J^{(2)} (z_2) J^{(2)} (z_1) J^{(2)} (y) \rangle \, ,
\end{align}
]]></tex-math></disp-formula>
which is represented as diagram (a) in <xref ref-type="fig" rid="F2">Fig. 2</xref>. Here we need to introduce the regulator <inline-formula><tex-math notation="LaTeX" id="ImEquation333"><![CDATA[$\epsilon$]]></tex-math></inline-formula> to the three-point function of spin-two current. Our prescription is to shift the conformal weight from <inline-formula><tex-math notation="LaTeX" id="ImEquation334"><![CDATA[$2$]]></tex-math></inline-formula> to <inline-formula><tex-math notation="LaTeX" id="ImEquation335"><![CDATA[$2 - \epsilon$]]></tex-math></inline-formula>, so we use
<disp-formula id="ptx154-M71"><label>(71)</label><tex-math notation="LaTeX" id="Equation71"><![CDATA[
\begin{align}
\langle J^{(2)} (z_2) J^{(2)} (z_1) J^{(2)} (y) \rangle =
\frac{c}{z_{21}^{2- \epsilon}(z_2 - y )^{2- \epsilon}(z_1 - y )^{2- \epsilon} } \, .
\end{align}
]]></tex-math></disp-formula></p>
<p>The integral becomes simpler by taking <inline-formula><tex-math notation="LaTeX" id="ImEquation336"><![CDATA[$y \to - \infty$]]></tex-math></inline-formula> as
<disp-formula id="ptx154-M72"><label>(72)</label><tex-math notation="LaTeX" id="Equation72"><![CDATA[
\begin{align}
\lim_{y \to - \infty} |y|^{4 -2 \epsilon } \langle W_{h_0}^{(2)} (z) J^{(2)} (y) \rangle
= - \frac{c h_0}{z^{2h_0 - 2}} \left[ \frac{1 }{3 \epsilon} + \frac{1}{36} (18 h_0 +12 \log (z)-13) \right]
\label{spin2first}
\end{align}
]]></tex-math></disp-formula>
up to the term of order <inline-formula><tex-math notation="LaTeX" id="ImEquation337"><![CDATA[$\epsilon^0$]]></tex-math></inline-formula>.</p>
<p>The second one is from
<disp-formula id="ptx154-M73"><label>(73)</label><tex-math notation="LaTeX" id="Equation73"><![CDATA[
\begin{align}
&\langle W^{(3)}_{h_0} (z) J^{(2)} (y) \rangle \nonumber\\
&\quad = \int_0^z d z_3 \int_0^{z_3} d z_2 \int_0^{z_2} dz_1 f_3 ^{(2,2,2)} ( z_3,z_2 ,z_1) \langle J^{(2)} (z_3)J^{(2)} (z_2)J^{(2)} (z_1) J^{(2)} (y) \rangle \, .
\end{align}
]]></tex-math></disp-formula></p>
<p>At the leading order in <inline-formula><tex-math notation="LaTeX" id="ImEquation338"><![CDATA[$1/c$]]></tex-math></inline-formula>, the four-point function is given by a sum over the products of the two-point function as
<disp-formula id="ptx154-M74"><label>(74)</label><tex-math notation="LaTeX" id="Equation74"><![CDATA[
\begin{align}
& \langle J^{(2)} (z_3)J^{(2)} (z_2)J^{(2)} (z_1) J^{(2)} (y) \rangle \nonumber \\
&\quad= \frac{c^2/4}{z_{32}^{4 -2 \epsilon}(z_1 - y )^{4- 2 \epsilon }} +\frac{c^2/4}{z_{31} ^{4 - 2 \epsilon} (z_2 - y )^{4- 2 \epsilon } } + \frac{c^2/4}{z_{21}^{4- 2\epsilon} (z_3 - y )^{4- 2 \epsilon} }
+ \mathcal{O}(c)\, .
\end{align}
]]></tex-math></disp-formula></p>
<p>Denoting
<disp-formula id="ptx154-M75"><label>(75)</label><tex-math notation="LaTeX" id="Equation75"><![CDATA[
\begin{align}
H^{(3)}_{ij} (z) =z^{2h_0 - 2}
\int_0^z d z_3 \int_0^{z_3} d z_2 \int_0^{z_2} dz_1 f_3 ^{(2,2,2)} ( z_3,z_2 ,z_1)
\frac{1}{z_{ji} ^{4 - 2 \epsilon}} \, ,
\end{align}
]]></tex-math></disp-formula>
we find
<disp-formula id="ptx154-M76"><label>(76)</label><tex-math notation="LaTeX" id="Equation76"><![CDATA[
\begin{align}
H^{(3)}_{12} (z)& =H^{(3)}_{23} (z)= \frac{(h_0-1) h_0^2 }{9 \epsilon}+\frac{2}{45} h_0 (5 (h_0-1) h_0 \log (z)+(h_0-2) (h_0+1)) \, , \nonumber\\
H^{(3)}_{13} (z)& = -\frac{h_0 ((h_0-1) h_0-1) }{9 \epsilon}-\frac{1}{135} h_0 (30 ((h_0-1) h_0-1) \log (z)-h_0 (13 h_0+32)+1)
\end{align}
]]></tex-math></disp-formula>
up to the terms of <inline-formula><tex-math notation="LaTeX" id="ImEquation339"><![CDATA[$\mathcal{O} (\epsilon^0)$]]></tex-math></inline-formula>. The integrals <inline-formula><tex-math notation="LaTeX" id="ImEquation340"><![CDATA[$H^{(3)}_{12}(z)$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation341"><![CDATA[$H^{(3)}_{13}(z)$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation342"><![CDATA[$H^{(3)}_{23}(z)$]]></tex-math></inline-formula> correspond to the diagrams (b), (c), (d) in <xref ref-type="fig" rid="F2">Fig. 2</xref>, respectively.</p>
<p>Combining the results so far, we find
<disp-formula id="ptx154-M77"><label>(77)</label><tex-math notation="LaTeX" id="Equation77"><![CDATA[
\begin{align}
&\lim_{y \to - \infty} |y|^{4 - 2 \epsilon } \langle W_{h_0} (z) J^{(2)} (y)\rangle
\nonumber \\
&\quad= \frac{1}{z^{2h_0-2}} \left[
h_0 + \frac{h_0}{c} \left(\frac{6 (h_0(h_0-1)-1) }{\epsilon} + 10 h_0 (h_0-1) + 3 + 12 (h_0-1) h_0 \log ( z) \right) \right] + \cdots \nonumber \\
&\quad= z^2 \left[ h_0 - \frac{6 h_0}{c} \left( \frac{1}{\epsilon} + h_0 - \frac12 \right) \right] \langle W_{h_0} (z) \rangle + \cdots \, .
\end{align}
]]></tex-math></disp-formula></p>
<p>The expression diverges for <inline-formula><tex-math notation="LaTeX" id="ImEquation343"><![CDATA[$\epsilon \to 0$]]></tex-math></inline-formula>, and we remove the divergence by properly choosing <inline-formula><tex-math notation="LaTeX" id="ImEquation344"><![CDATA[$c_2^{(1)}$]]></tex-math></inline-formula> in Eq. (<xref ref-type="disp-formula" rid="ptx154-M60">60</xref>) as
<disp-formula id="ptx154-M78"><label>(78)</label><tex-math notation="LaTeX" id="Equation78"><![CDATA[
\begin{align}
c_2 = 1 + \frac{6}{c} \left( \frac{1}{\epsilon} + a \right) + \mathcal{O} (c^{-2}) \, .
\end{align}
]]></tex-math></disp-formula></p>
<p>Here <inline-formula><tex-math notation="LaTeX" id="ImEquation345"><![CDATA[$a$]]></tex-math></inline-formula> is an arbitrary constant, which shall be fixed shortly. With this choice of the parameter <inline-formula><tex-math notation="LaTeX" id="ImEquation346"><![CDATA[$c_2$]]></tex-math></inline-formula>, there arises a contribution of order <inline-formula><tex-math notation="LaTeX" id="ImEquation347"><![CDATA[$1/c$]]></tex-math></inline-formula> from the following term as
<disp-formula id="ptx154-M79"><label>(79)</label><tex-math notation="LaTeX" id="Equation79"><![CDATA[
\begin{align}
\left. \frac{6 c_2}{c} \lim_{y \to - \infty} |y|^{4 - 2 \epsilon } \langle W_{h_0}^{(1)} (z) J^{(2)} (y)\rangle
\right|_{\mathcal{O}(c^{-1})} = \frac{ h_0 }{z^{2h_0 -2}}\frac{6}{c} \left( \frac{1}{\epsilon} + a \right)
\end{align}
]]></tex-math></disp-formula>
up to the terms of order <inline-formula><tex-math notation="LaTeX" id="ImEquation348"><![CDATA[$\epsilon^0$]]></tex-math></inline-formula>. Here <inline-formula><tex-math notation="LaTeX" id="ImEquation349"><![CDATA[$W_{h_0}^{(1)} (z)$]]></tex-math></inline-formula> is given in Eq. (<xref ref-type="disp-formula" rid="ptx154-M64">64</xref>). With this prescription, we have
<disp-formula id="ptx154-M80"><label>(80)</label><tex-math notation="LaTeX" id="Equation80"><![CDATA[
\begin{align}
&\lim_{y \to - \infty} |y|^{4 - 2 \epsilon} \langle W_{h_0} (z) J^{(2)} (y)\rangle \nonumber \\
& \quad = z^2 \left[ h_0 - \frac{6 h_0}{c} \left( h_0 - \frac12 - a \right) \right] \langle W_{h_0} (z) \rangle
+ \mathcal{O}(c^{-2})
\end{align}
]]></tex-math></disp-formula>
for <inline-formula><tex-math notation="LaTeX" id="ImEquation350"><![CDATA[$\epsilon \to 0$]]></tex-math></inline-formula>. Therefore, setting <inline-formula><tex-math notation="LaTeX" id="ImEquation351"><![CDATA[$a = 1/2$]]></tex-math></inline-formula>, we reproduce the expected result as Eq. (<xref ref-type="disp-formula" rid="ptx154-M62">62</xref>) with <inline-formula><tex-math notation="LaTeX" id="ImEquation352"><![CDATA[$h_1 = - 6 h_0 (h_0 -1)$]]></tex-math></inline-formula> in Eq. (<xref ref-type="disp-formula" rid="ptx154-M61">61</xref>). In summary, we choose the parameter <inline-formula><tex-math notation="LaTeX" id="ImEquation353"><![CDATA[$c_2$]]></tex-math></inline-formula> in Eq. (<xref ref-type="disp-formula" rid="ptx154-M58">58</xref>) as
<disp-formula id="ptx154-M81"><label>(81)</label><tex-math notation="LaTeX" id="Equation81"><![CDATA[
\begin{align}
c_2 = 1 + \frac{1}{c} \left( \frac{6}{\epsilon} + 3 \right) + \mathcal{O} (c^{-2})
\label{level2c}
\end{align}
]]></tex-math></disp-formula>
in order to absorb a divergence from the one-loop diagram and also reproduce the result from the conformal Ward identity.</p>
</sec>
<sec id="SEC4.3"><title>4.3. Two-point function at <inline-formula><tex-math notation="LaTeX" id="ImEquation354"><![CDATA[$1/c^2$]]></tex-math></inline-formula> order</title>
<p>In the previous subsections we have regularized divergences arising up to the one-loop order. Our claim is that other quantities are predictable after the renormalization. Here we would like to examine the two-point function at two-loop order. Generically, two-loop diagrams have one-loop sub-diagrams, and there would appear non-local divergences from the sub-diagrams. After all one-loop divergences are removed by the renormalization procedure, we should have no non-local divergences at the two-loop order. There would be local divergences remaining, which can be renormalized as for the one-loop computations. As discussed in Ref. [<xref ref-type="bibr" rid="B24">24</xref>], a two-point function without proper renormalization does not reproduce the correct dependence on <inline-formula><tex-math notation="LaTeX" id="ImEquation355"><![CDATA[$\log (z)$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation356"><![CDATA[$\log^2 (z)$]]></tex-math></inline-formula> at the two-loop order because of non-local divergences as <inline-formula><tex-math notation="LaTeX" id="ImEquation357"><![CDATA[$1/\epsilon \log (z)$]]></tex-math></inline-formula>.</p>
<p>Since now it is not expected to have such divergences after the renormalization, it should be possible to reproduce the correct shift of conformal weight even at the <inline-formula><tex-math notation="LaTeX" id="ImEquation358"><![CDATA[$1/c^2$]]></tex-math></inline-formula> order. We shall show that this is indeed the case in this subsection.</p>
<p>We first evaluate the expectation value of the open Wilson line at the <inline-formula><tex-math notation="LaTeX" id="ImEquation359"><![CDATA[$1/c^2$]]></tex-math></inline-formula> order without renormalization, then we consider its effects. A contribution comes from <inline-formula><tex-math notation="LaTeX" id="ImEquation360"><![CDATA[$ \langle W_{h_0}^{(3)} (z) \rangle$]]></tex-math></inline-formula> in Eq. (<xref ref-type="disp-formula" rid="ptx154-M64">64</xref>) as
<disp-formula id="ptx154-M82"><label>(82)</label><tex-math notation="LaTeX" id="Equation82"><![CDATA[
\begin{align}
G^{(2)}_{123} (z) = & \left( \frac{6}{c}\right)^3 \int_0^z d z_3 \int_0^{z_3} d z_2 \int_0^{z_2} dz_1 f_3^{(2,2,2)} ( z_3,z_2 ,z_1) \frac{c}{z_{32}^{2- \epsilon}z_{31}^{2-\epsilon} z_{21}^{2- \epsilon} } \, ,
\end{align}
]]></tex-math></disp-formula>
which is expressed as diagram (a) in <xref ref-type="fig" rid="F3">Fig. 3</xref>. The integral is computed as</p>
<fig id="F3" orientation="portrait" position="float"><label>Fig. 3.</label><caption><p>Diagrams contributing to the <inline-formula><tex-math notation="LaTeX" id="ImEquation361"><![CDATA[$1/c^2$]]></tex-math></inline-formula>-order correction of <inline-formula><tex-math notation="LaTeX" id="ImEquation362"><![CDATA[$\langle \mathcal{O}_h \bar{\mathcal{O}}_h \rangle$]]></tex-math></inline-formula> for <inline-formula><tex-math notation="LaTeX" id="ImEquation363"><![CDATA[$N=2$]]></tex-math></inline-formula>.</p></caption>
<graphic xmlns:xlink="http://www.w3.org/1999/xlink" orientation="portrait" position="float" xlink:href="ptx154F3.tif"/></fig>
<p><disp-formula id="ptx154-M83"><label>(83)</label><tex-math notation="LaTeX" id="Equation83"><![CDATA[
\begin{align}
c^2 z^{2h_0}G^{(2)}_{123} (z) & = -\frac{ 288 h_0 (h_0-1) \log (z)}{\epsilon} \nonumber \\
&\quad +2 h_0 \left(36 \log (z) \left(-6 (h_0-1) \log (z)-2 h_0^2-9 h_0+5\right)\right) \, .
\end{align}
]]></tex-math></disp-formula></p>
<p>Here we neglect the terms of <inline-formula><tex-math notation="LaTeX" id="ImEquation364"><![CDATA[$\mathcal{O}(\epsilon)$]]></tex-math></inline-formula> and write down only the terms depending on <inline-formula><tex-math notation="LaTeX" id="ImEquation365"><![CDATA[$\log (z)$]]></tex-math></inline-formula> or <inline-formula><tex-math notation="LaTeX" id="ImEquation366"><![CDATA[$\log ^2 (z)$]]></tex-math></inline-formula>. In the rest of this subsection, we include only such terms. Another type of contribution arises from <inline-formula><tex-math notation="LaTeX" id="ImEquation367"><![CDATA[$ \langle W_{h_0}^{(4)} (z) \rangle$]]></tex-math></inline-formula> in Eq. (<xref ref-type="disp-formula" rid="ptx154-M64">64</xref>). Defining
<disp-formula id="ptx154-M84"><label>(84)</label><tex-math notation="LaTeX" id="Equation84"><![CDATA[
\begin{align}
&G^{(2)}_{ij;kl} (z) = \left( \frac{6}{c}\right)^4 \int_0^z d z_4 \int_0^{z_4} d z_3 \int_0^{z_3} d z_2 \int_0^{z_2} dz_1 f_4^{(2,2,2,2)} ( z_4,z_3,z_2,z_1) \frac{c^{2/4}}{z_{lk} ^{4- 2 \epsilon} z_{ji}^{4- 2 \epsilon}} \, ,
\end{align}
]]></tex-math></disp-formula>
we find
<disp-formula id="ptx154-M85"><label>(85)</label><tex-math notation="LaTeX" id="Equation85"><![CDATA[
\begin{align}
c^2 z^{ 2 h_0} G^{(2)}_{12;34} (z) &=\frac{144 h_0^2 (h_0-1)^2 \log (z)}{\epsilon} \nonumber \\
& \quad - 96 (h_0-1) h_0 ^2 \log (z) (-3 (h_0-1) \log (z)-5 h_0+2) \, , \nonumber \\
c^2 z^{2 h_0} G^{(2)}_{14;23} (z) &= \frac{ 360 (h_0-1)^2 h_0^2 \log (z)}{5 \epsilon} \nonumber \\ & \quad +\frac{72}{5} h_0 (h_0-1) \log (z) (10 (h_0-1) h_0 \log (z)+h_0 (23 h_0-43)-16) \, , \\
c^2 z^{2 h_0} G^{(2)}_{13;24} (z) &= - \frac{ 720 h_0 \left((h_0-2) h_0^2+1\right) \log (z)}{5 \epsilon} \nonumber \\
& \quad +\frac{12}{5} h_0 \log (z) \left(-120 \left((h_0-2) h^2_0 +1\right) \log (z)+h_0 \left(-238 h_0^2+596 h_0+3\right)-241\right) \, . \nonumber
\end{align}
]]></tex-math></disp-formula></p>
<p>These integrals correspond to diagrams (b), (c), (d) in <xref ref-type="fig" rid="F3">Fig. 3</xref>, respectively. Summing over all contributions we find
<disp-formula id="ptx154-M86"><label>(86)</label><tex-math notation="LaTeX" id="Equation86"><![CDATA[
\begin{align}
\label{G2z}
c^2 z^{2h_0} G^{(2)}_{h_0} (z) &= \frac{ 72 h_0 (h_0-2) (h_0-1) (h_0+1) \log (z) }{\epsilon} \nonumber \\ & \quad +12 h_0 \log (z) \left(12 \left((h_0-2) h_0^2+1\right) \log (z) +h_0 (4 h_0 (5 h_0-7)-5)+1\right) \, .
\end{align}
]]></tex-math></disp-formula></p>
<p>Therefore, a non-locally divergent term as <inline-formula><tex-math notation="LaTeX" id="ImEquation368"><![CDATA[$1/\epsilon \log (z)$]]></tex-math></inline-formula> remains, and the expression cannot be compared with Eq. (<xref ref-type="disp-formula" rid="ptx154-M10">10</xref>).</p>
<p>Now we include the effects of renormalization, namely, the change of overall factor as in Eq. (<xref ref-type="disp-formula" rid="ptx154-M68">68</xref>) and the shift of parameter <inline-formula><tex-math notation="LaTeX" id="ImEquation369"><![CDATA[$c_2$]]></tex-math></inline-formula> as in Eq. (<xref ref-type="disp-formula" rid="ptx154-M81">81</xref>). These effects lead to an extra contribution as
<disp-formula id="ptx154-M87"><label>(87)</label><tex-math notation="LaTeX" id="Equation87"><![CDATA[
\begin{align}
\langle \tilde W_{h_0} (z) \rangle
&= \left[ 1 - \frac{1}{c}\left(\frac{6(h_0-1) h_0 }{ \epsilon} + 2 h_0 (5 h_0 -2 ) \right) \right] \nonumber \\
&\quad\times
\left[ \frac{1}{z^{2h_0}} + \left(\frac{6 }{c} \right)^2 \left( 1 + \frac{1}{c} \left( \frac{6}{\epsilon} + 3 \right) \right)^2
\langle W^{(2)}_{h_0} (z) \rangle + G^{(2)}_{h_0} (z) \right] + \cdots \nonumber \\
&= \frac{1}{z^{2h_0}} + \left(\frac{6 }{c} \right)^2\langle W^{(2)}_{h_0} (z) \rangle + G^{(2)}_{h_0} (z) + \tilde G^{(2)}_{h_0} (z) + \cdots \, ,
\end{align}
]]></tex-math></disp-formula>
where
<disp-formula id="ptx154-M88"><label>(88)</label><tex-math notation="LaTeX" id="Equation88"><![CDATA[
\begin{align}
\tilde G^{(2)}_{h_0} (z) = \frac{1}{c}\left[ 2 \left( \frac{6}{\epsilon} + 3 \right) - \frac{6 h_0 (h_0 -1)}{\epsilon} - 2 h_0 (5h_0 -2) \right] \left( \frac{6}{c} \right)^2 \langle W^{(2)}_{h_0} (z) \rangle \, .
\label{extra}
\end{align}
]]></tex-math></disp-formula></p>
<p>The extra contribution can be evaluated as
<disp-formula id="ptx154-M89"><label>(89)</label><tex-math notation="LaTeX" id="Equation89"><![CDATA[
\begin{align}
c^2 z^{2h_0} \tilde G^{(2)}_{h_0} (z) &=
\frac{- 72 h_0 (h_0-2) (h_0-1) (h_0+1) \log \left(z\right)}{\epsilon} \\
& \quad - 72 h_0 (h_0-2) (h_0-1) (h_0+1) \log ^2\left(z\right)
+24 h_0 (h_0 (2 h_0 (7-5 h_0)+9)-7) \log \left(z\right) \nonumber \, .
\end{align}
]]></tex-math></disp-formula></p>
<p>Thus in total we arrive at
<disp-formula id="ptx154-M90"><label>(90)</label><tex-math notation="LaTeX" id="Equation90"><![CDATA[
\begin{align}
c^2 z^{2 h_0} \left. \langle \tilde W_{h_0} (z) \rangle \right|_{\mathcal{O}(c^{0})} =
72 h_0^2 (h_0-1)^2 \log ^2 (z)+156 h_0 (h_0-1) \log (z) \, ,
\end{align}
]]></tex-math></disp-formula>
which does not have any non-local divergence. Compared with the <inline-formula><tex-math notation="LaTeX" id="ImEquation370"><![CDATA[$1/c$]]></tex-math></inline-formula> expansion of the two-point function in Eq. (<xref ref-type="disp-formula" rid="ptx154-M10">10</xref>), the coefficients in front of <inline-formula><tex-math notation="LaTeX" id="ImEquation371"><![CDATA[$\log (z)$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation372"><![CDATA[$\log^2 (z)$]]></tex-math></inline-formula> at the <inline-formula><tex-math notation="LaTeX" id="ImEquation373"><![CDATA[$1/c^2$]]></tex-math></inline-formula> order are correctly reproduced with <inline-formula><tex-math notation="LaTeX" id="ImEquation374"><![CDATA[$h_1,h_2$]]></tex-math></inline-formula> in Eq. (<xref ref-type="disp-formula" rid="ptx154-M61">61</xref>).</p>
</sec>
</sec>
<sec id="SEC5"><title>5. Correlators for <inline-formula><tex-math notation="LaTeX" id="ImEquation375"><![CDATA[$\boldsymbol{N=3}$]]></tex-math></inline-formula></title>
<p>In the previous section, we have illustrated our prescription by examining a simple example of sl<inline-formula><tex-math notation="LaTeX" id="ImEquation376"><![CDATA[$(N)$]]></tex-math></inline-formula> Chern&#x2013;Simons theory with <inline-formula><tex-math notation="LaTeX" id="ImEquation377"><![CDATA[$N=2$]]></tex-math></inline-formula>. In this section, we extend the analysis to a more involved case with <inline-formula><tex-math notation="LaTeX" id="ImEquation378"><![CDATA[$N=3$]]></tex-math></inline-formula>. It is a rather straightforward generalization even though computations become complicated due to the existence of spin-three current <inline-formula><tex-math notation="LaTeX" id="ImEquation379"><![CDATA[$J^{(3)}$]]></tex-math></inline-formula>. In this paper, we adopt the representation of sl<inline-formula><tex-math notation="LaTeX" id="ImEquation380"><![CDATA[$(N)$]]></tex-math></inline-formula> generators with <inline-formula><tex-math notation="LaTeX" id="ImEquation381"><![CDATA[$x$]]></tex-math></inline-formula>-derivatives as in Eq. (<xref ref-type="disp-formula" rid="ptx154-M42">42</xref>), which is valid for arbitrary representation with <inline-formula><tex-math notation="LaTeX" id="ImEquation382"><![CDATA[$h_0 = - j$]]></tex-math></inline-formula> for <inline-formula><tex-math notation="LaTeX" id="ImEquation383"><![CDATA[$N=2$]]></tex-math></inline-formula> but only for the fundamental representation with <inline-formula><tex-math notation="LaTeX" id="ImEquation384"><![CDATA[$h_0 = (1 - N)/2$]]></tex-math></inline-formula> for <inline-formula><tex-math notation="LaTeX" id="ImEquation385"><![CDATA[$N \geq 3$]]></tex-math></inline-formula>.<xref ref-type="fn" rid="FN4"><sup>4</sup></xref> With <inline-formula><tex-math notation="LaTeX" id="ImEquation386"><![CDATA[$N=3$]]></tex-math></inline-formula>, the <inline-formula><tex-math notation="LaTeX" id="ImEquation387"><![CDATA[$1/c$]]></tex-math></inline-formula> expansion of conformal weight is given by Eq. (<xref ref-type="disp-formula" rid="ptx154-M9">9</xref>) with Eq. (<xref ref-type="disp-formula" rid="ptx154-M11">11</xref>) as
<disp-formula id="ptx154-M91"><label>(91)</label><tex-math notation="LaTeX" id="Equation91"><![CDATA[
\begin{align}
h_0 = - 1 \, , \quad h_1 = - 32 \, , \quad h_2 = - 1600 \, .
\label{dimshift3}
\end{align}
]]></tex-math></disp-formula></p>
<p>In the next subsection, we reproduce the conformal weight at the <inline-formula><tex-math notation="LaTeX" id="ImEquation388"><![CDATA[$1/c$]]></tex-math></inline-formula> order as in <inline-formula><tex-math notation="LaTeX" id="ImEquation389"><![CDATA[$h_1$]]></tex-math></inline-formula> above from the bulk viewpoint and renormalize the open Wilson line. In <xref ref-type="sec" rid="SEC5.2">Sect. 5.2</xref>, we examine three-point functions and fix the two parameters <inline-formula><tex-math notation="LaTeX" id="ImEquation390"><![CDATA[$c_2$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation391"><![CDATA[$c_3$]]></tex-math></inline-formula> in Eq. (<xref ref-type="disp-formula" rid="ptx154-M58">58</xref>) to be consistent with symmetry. In <xref ref-type="sec" rid="SEC5.3">Sect. 5.3</xref>, we show that our prescription correctly reproduces the conformal weight at the <inline-formula><tex-math notation="LaTeX" id="ImEquation392"><![CDATA[$1/c^2$]]></tex-math></inline-formula> order as <inline-formula><tex-math notation="LaTeX" id="ImEquation393"><![CDATA[$h_2$]]></tex-math></inline-formula> in Eq. (<xref ref-type="disp-formula" rid="ptx154-M91">91</xref>).</p>
<sec id="SEC5.1"><title>5.1. Two-point function at <inline-formula><tex-math notation="LaTeX" id="ImEquation394"><![CDATA[$1/c$]]></tex-math></inline-formula> order</title>
<p>As for <inline-formula><tex-math notation="LaTeX" id="ImEquation395"><![CDATA[$N=2$]]></tex-math></inline-formula>, we start by examining the two-point function at the <inline-formula><tex-math notation="LaTeX" id="ImEquation396"><![CDATA[$1/c$]]></tex-math></inline-formula> order. Since spin-three current <inline-formula><tex-math notation="LaTeX" id="ImEquation397"><![CDATA[$J^{(3)}$]]></tex-math></inline-formula> is involved along with spin-two current <inline-formula><tex-math notation="LaTeX" id="ImEquation398"><![CDATA[$J^{(2)}$]]></tex-math></inline-formula>, there are two types of corrections as
<disp-formula id="ptx154-M92"><label>(92)</label><tex-math notation="LaTeX" id="Equation92"><![CDATA[
\begin{align}
\left( \frac{6}{c}\right)^2 \left[ \langle W^{(2)}_{h_0} (z) \rangle + \langle W^{(2)'}_{h_0 } (z) \rangle \right]
\label{W2h}
\end{align}
]]></tex-math></disp-formula>
at this order. They are represented in <xref ref-type="fig" rid="F1">Figs. 1</xref> and <xref ref-type="fig" rid="F4">4</xref>, respectively. Here <inline-formula><tex-math notation="LaTeX" id="ImEquation399"><![CDATA[$W^{(2)}_{h_0} (z) $]]></tex-math></inline-formula> is defined in Eq. (<xref ref-type="disp-formula" rid="ptx154-M64">64</xref>) and</p>
<fig id="F4" orientation="portrait" position="float"><label>Fig. 4.</label><caption><p>Diagram contributing to the <inline-formula><tex-math notation="LaTeX" id="ImEquation400"><![CDATA[$1/c$]]></tex-math></inline-formula>-order correction of <inline-formula><tex-math notation="LaTeX" id="ImEquation401"><![CDATA[$\langle \mathcal{O}_{h_+} \bar{\mathcal{O}}_{h_+} \rangle$]]></tex-math></inline-formula> for <inline-formula><tex-math notation="LaTeX" id="ImEquation402"><![CDATA[$N=3$]]></tex-math></inline-formula> in addition to the one in <xref ref-type="fig" rid="F1">Fig. 1</xref>. The thick wavy line represents the propagator of spin-three current.</p></caption>
<graphic xmlns:xlink="http://www.w3.org/1999/xlink" orientation="portrait" position="float" xlink:href="ptx154F4.tif"/></fig>
<p><disp-formula id="ptx154-M93"><label>(93)</label><tex-math notation="LaTeX" id="Equation93"><![CDATA[
\begin{align}
W^{(2) '}_{h_0} (z) = \int_0^z d z_2 \int_0^{z_2} dz_1 f^{(3,3)}_2 (z_2,z_1)
J^{(3)} (z_2) J^{(3)} (z_1) \, .
\label{W2p}
\end{align}
]]></tex-math></disp-formula></p>
<p>Since we have already computed <inline-formula><tex-math notation="LaTeX" id="ImEquation403"><![CDATA[$\langle W^{(2)}_{h_0} (z) \rangle$]]></tex-math></inline-formula> as in Eq. (<xref ref-type="disp-formula" rid="ptx154-M66">66</xref>), we just need to evaluate <inline-formula><tex-math notation="LaTeX" id="ImEquation404"><![CDATA[$\langle W^{(2)'}_{h_0} (z) \rangle$]]></tex-math></inline-formula>. The prescription in Eq. (<xref ref-type="disp-formula" rid="ptx154-M57">57</xref>) leads us to adopt
<disp-formula id="ptx154-M94"><label>(94)</label><tex-math notation="LaTeX" id="Equation94"><![CDATA[
\begin{align}
\langle J^{(3)} (z_2) J^{(3)} (z_1) \rangle = - \frac{5c}{6} \frac{1}{z_{21}^{6 -2 \epsilon} }
\end{align}
]]></tex-math></disp-formula>
with the shift of conformal dimension of <inline-formula><tex-math notation="LaTeX" id="ImEquation405"><![CDATA[$J^{(3)}$]]></tex-math></inline-formula> from <inline-formula><tex-math notation="LaTeX" id="ImEquation406"><![CDATA[$3$]]></tex-math></inline-formula> to <inline-formula><tex-math notation="LaTeX" id="ImEquation407"><![CDATA[$3 - \epsilon$]]></tex-math></inline-formula>. Using this expression, we find
<disp-formula id="ptx154-M95"><label>(95)</label><tex-math notation="LaTeX" id="Equation95"><![CDATA[
\begin{align}
\langle W^{(2)'}_{h_0} (z) \rangle &= - \frac{5 c}{6}\left[
-\frac{h_0 (h_0 (4 (h_0-2) h_0+1)+3) z^{-2 h_0}}{15 \epsilon} \right. \\
&\quad \left. -\frac{1}{450} h_0 (2 h_0+1) z^{-2 h_0} (60 (h_0-1) (2 h_0-3) \log (z)+h_0 (94 h_0-115)-9) \right] \nonumber
\end{align}
]]></tex-math></disp-formula>
up to the term of order <inline-formula><tex-math notation="LaTeX" id="ImEquation408"><![CDATA[$\epsilon^0$]]></tex-math></inline-formula>. Inserting <inline-formula><tex-math notation="LaTeX" id="ImEquation409"><![CDATA[$h_0 = -1$]]></tex-math></inline-formula>, we obtain
<disp-formula id="ptx154-M96"><label>(96)</label><tex-math notation="LaTeX" id="Equation96"><![CDATA[
\begin{align}
z^{-2} \langle W_{-1} (z) \rangle&= 1 + \left( \frac{6}{c} \right)^2 \frac{c}{2} \left(\frac{2 }{3 \epsilon} + \frac{1}{9} \left(12 \log \left(z\right) + 7\right) \right)
\nonumber \\
&\quad + \left( \frac{6}{c} \right)^2 \left(- \frac{5c}{6} \right) \left(-\frac{2 }{3 \epsilon}-\frac{1}{450} (600 \log (z)+200) \right) \nonumber \\
&= 1 + \frac{1}{c} \left(\frac{32 }{\epsilon }+ 64 \log (z)+\frac{82}{3} \right)
\end{align}
]]></tex-math></disp-formula>
up to the terms of orders <inline-formula><tex-math notation="LaTeX" id="ImEquation410"><![CDATA[$\epsilon^0$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation411"><![CDATA[$1/c$]]></tex-math></inline-formula>. In particular, the <inline-formula><tex-math notation="LaTeX" id="ImEquation412"><![CDATA[$1/c$]]></tex-math></inline-formula>-order correction of conformal weight is read off as <inline-formula><tex-math notation="LaTeX" id="ImEquation413"><![CDATA[$h_1 = - 32$]]></tex-math></inline-formula>, which is consistent with Eq. (<xref ref-type="disp-formula" rid="ptx154-M91">91</xref>). In order to remove the divergence at <inline-formula><tex-math notation="LaTeX" id="ImEquation414"><![CDATA[$\epsilon \to 0$]]></tex-math></inline-formula> up to the <inline-formula><tex-math notation="LaTeX" id="ImEquation415"><![CDATA[$1/c$]]></tex-math></inline-formula> order, we renormalize the Wilson line operator as
<disp-formula id="ptx154-M97"><label>(97)</label><tex-math notation="LaTeX" id="Equation97"><![CDATA[
\begin{align}
\tilde W_{-1} (z) = \left[ 1 - \frac{1}{c} \left(\frac{32}{ \epsilon} + \frac{82}{3} \right) \right]W_{-1} (z) \, , \label{wfren3}
\end{align}
]]></tex-math></disp-formula>
which leads to the corresponding two-point function of canonical form as in Eq. (<xref ref-type="disp-formula" rid="ptx154-M6">6</xref>).</p>
</sec>
<sec id="SEC5.2"><title>5.2. Three-point functions</title>
<p>We move to three-point functions with one conserved current. For <inline-formula><tex-math notation="LaTeX" id="ImEquation416"><![CDATA[$N=3$]]></tex-math></inline-formula>, there are two choices of currents, i.e., spin-two current <inline-formula><tex-math notation="LaTeX" id="ImEquation417"><![CDATA[$J^{(2)}$]]></tex-math></inline-formula> and spin-three current <inline-formula><tex-math notation="LaTeX" id="ImEquation418"><![CDATA[$J^{(3)}$]]></tex-math></inline-formula>. We start by computing <inline-formula><tex-math notation="LaTeX" id="ImEquation419"><![CDATA[$ \langle W_{-1} (z) J^{(2)}(y) \rangle $]]></tex-math></inline-formula> up to the <inline-formula><tex-math notation="LaTeX" id="ImEquation420"><![CDATA[$1/c$]]></tex-math></inline-formula> order by following the previous analysis for <inline-formula><tex-math notation="LaTeX" id="ImEquation421"><![CDATA[$N=2$]]></tex-math></inline-formula>. With the convention of <inline-formula><tex-math notation="LaTeX" id="ImEquation422"><![CDATA[$J^{(2)}$]]></tex-math></inline-formula> in Eq. (<xref ref-type="disp-formula" rid="ptx154-M56">56</xref>), the corresponding three-point function is given by Eq. (<xref ref-type="disp-formula" rid="ptx154-M62">62</xref>) with Eq. (<xref ref-type="disp-formula" rid="ptx154-M91">91</xref>). At the leading order in <inline-formula><tex-math notation="LaTeX" id="ImEquation423"><![CDATA[$1/c$]]></tex-math></inline-formula>, we have already computed as in Eq. (<xref ref-type="disp-formula" rid="ptx154-M55">55</xref>) with <inline-formula><tex-math notation="LaTeX" id="ImEquation424"><![CDATA[$s=2$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation425"><![CDATA[$h_0=-1$]]></tex-math></inline-formula>. In the following we shall examine the next nontrivial order in <inline-formula><tex-math notation="LaTeX" id="ImEquation426"><![CDATA[$1/c$]]></tex-math></inline-formula>.</p>
<p>At the order in <inline-formula><tex-math notation="LaTeX" id="ImEquation427"><![CDATA[$1/c$]]></tex-math></inline-formula>, there are several types of contribution as in <xref ref-type="fig" rid="F2">Fig. 2</xref> and <xref ref-type="fig" rid="F5">Fig. 5</xref>.</p>
<fig id="F5" orientation="portrait" position="float"><label>Fig. 5.</label><caption><p>Diagrams contributing to the <inline-formula><tex-math notation="LaTeX" id="ImEquation428"><![CDATA[$1/c$]]></tex-math></inline-formula>-order correction of <inline-formula><tex-math notation="LaTeX" id="ImEquation429"><![CDATA[$\langle \mathcal{O}_{h_+} \bar{\mathcal{O}}_{h_+} J^{(2)} \rangle $]]></tex-math></inline-formula> for <inline-formula><tex-math notation="LaTeX" id="ImEquation430"><![CDATA[$N=3$]]></tex-math></inline-formula> in addition to the ones in <xref ref-type="fig" rid="F2">Fig. 2</xref>.</p></caption>
<graphic xmlns:xlink="http://www.w3.org/1999/xlink" orientation="portrait" position="float" xlink:href="ptx154F5.tif"/></fig>
<p>One comes from
<disp-formula id="ptx154-M98"><label>(98)</label><tex-math notation="LaTeX" id="Equation98"><![CDATA[
\begin{align}
\langle W_{-1}^{(2)} (z) J^{(2)}(y) \rangle &= \int_0^z dz_2 \int_0^{z_2} dz_1 f^{(2,2)}_2 (z_2 , z_1) \langle J^{(2)} (z_2) J^{(2)} (z_1) J^{(2)} (y) \rangle \, , \nonumber \\
\langle W_{-1}^{(2)'} (z) J^{(2)}(y) \rangle &=
\int_0^z dz_2 \int_0^{z_2} dz_1 f^{(3,3)}_2 (z_2 , z_1) \langle J^{(3)} (z_2) J^{(3)} (z_1) J^{(2)} (y) \rangle\, ,
\end{align}
]]></tex-math></disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation431"><![CDATA[$W_{-1}^{(2)} (z)$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation432"><![CDATA[$W_{-1}^{(2)'} (z)$]]></tex-math></inline-formula> were introduced in Eqs. (<xref ref-type="disp-formula" rid="ptx154-M64">64</xref>) and (<xref ref-type="disp-formula" rid="ptx154-M93">93</xref>), respectively. The first contribution corresponds to the diagram (a) in <xref ref-type="fig" rid="F2">Fig. 2</xref> and it has been computed as in Eq. (<xref ref-type="disp-formula" rid="ptx154-M72">72</xref>) with <inline-formula><tex-math notation="LaTeX" id="ImEquation433"><![CDATA[$h_0=-1$]]></tex-math></inline-formula>. For the second one corresponding to the diagram (a) in <xref ref-type="fig" rid="F5">Fig. 5</xref>, we find
<disp-formula id="ptx154-M99"><label>(99)</label><tex-math notation="LaTeX" id="Equation99"><![CDATA[
\begin{align}
\lim_{y \to - \infty} |y|^{4 - 2 \epsilon} \langle W_{-1}^{(2)'} (z) J^{(2)}(y) \rangle = - \frac{5 c}{2} \left[ -\frac{2 z^4}{3 \epsilon} +
\frac{1}{18} z^4 (13- 12 \log (z)) \right] + \mathcal{O}(\epsilon) \, ,
\end{align}
]]></tex-math></disp-formula>
where we have used
<disp-formula id="ptx154-M100"><label>(100)</label><tex-math notation="LaTeX" id="Equation100"><![CDATA[
\begin{align}
\langle J^{(3)} (z_2) J^{(3)} (z_1) J^{(2)}(y) \rangle = \frac{- 5 c/2}{z_{21}^{4 - \epsilon} (z_2 - y )^{2 - \epsilon} (z_1 - y )^{2 - \epsilon} }
\label{j3j3j2}
\end{align}
]]></tex-math></disp-formula>
with the shifts of conformal weight both for <inline-formula><tex-math notation="LaTeX" id="ImEquation434"><![CDATA[$J^{(2)}$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation435"><![CDATA[$J^{(3)}$]]></tex-math></inline-formula>.</p>
<p>Other types of contribution include four conserved currents. One of them involves four spin-two currents as
<disp-formula id="ptx154-M101"><label>(101)</label><tex-math notation="LaTeX" id="Equation101"><![CDATA[
\begin{align}
\int_0^{z} dz_3 \int_0^{z_3} dz_2 \int_0^{z_2} dz_1
f^{(2,2,2)}_3 (z_3 , z_2 , z_1 ) \langle J^{(2)} (z_3) J^{(2)} (z_2) J^{(2)} (z_1) J^{(2)} (y) \rangle \, .
\end{align}
]]></tex-math></disp-formula></p>
<p>They are represented in <xref ref-type="fig" rid="F2">Fig. 2</xref> and have already been evaluated in <xref ref-type="sec" rid="SEC4.2">Sect. 4.2</xref>. Others involve two spin-two and two spin-three currents, and the correlator of them is factorized at the leading order in <inline-formula><tex-math notation="LaTeX" id="ImEquation436"><![CDATA[$1/c$]]></tex-math></inline-formula> as
<disp-formula id="ptx154-M102"><label>(102)</label><tex-math notation="LaTeX" id="Equation102"><![CDATA[
\begin{align}
\langle J^{(3)} (z_3) J^{(3)} (z_2)J^{(2)} (z_1) J^{(2)} (y) \rangle
= \frac{- 5c^2/12}{z_{32}^{6 -2 \epsilon} ( z_1 - y )^{4 - 2 \epsilon} } + \mathcal{O} (c) \, . \label{j2j3j3j2}
\end{align}
]]></tex-math></disp-formula></p>
<p>Therefore, we need to evaluate
<disp-formula id="ptx154-M103"><label>(103)</label><tex-math notation="LaTeX" id="Equation103"><![CDATA[
\begin{align}
H^{(3,2)}_{1}(z) &= - \frac{5 c^2}{12} z^{-4} \int_0^{z} dz_3 \int_0^{z_3} dz_2 \int_0^{z_2} dz_1
f^{(2,3,3)}_3 (z_3 , z_2 , z_1 ) \frac{1}{z_{21}^{6 - 2\epsilon} } \, ,\nonumber \\
H^{(3,2)}_{2} (z) &= - \frac{5 c^2}{12} z^{-4}\int_0^{z} dz_3 \int_0^{z_3} dz_2 \int_0^{z_2} dz_1
f^{(3,2,3)}_3 (z_3 , z_2 , z_1 ) \frac{1}{z_{31}^{6 - 2\epsilon} } \, , \nonumber \\
H^{(3,2)}_{3} (z) &= - \frac{5 c^2}{12} z^{-4} \int_0^{z} dz_3 \int_0^{z_3} dz_2 \int_0^{z_2} dz_1
f^{(3,3,2)}_3 (z_3 , z_2 , z_1 ) \frac{1}{z_{32}^{6 - 2\epsilon} } \, ,
\end{align}
]]></tex-math></disp-formula>
which correspond to diagrams (b), (c), (d) in <xref ref-type="fig" rid="F5">Fig. 5</xref>, respectively. Explicitly performing the integrals, we find
<disp-formula id="ptx154-M104"><label>(104)</label><tex-math notation="LaTeX" id="Equation104"><![CDATA[
\begin{align}
& H^{(3,2)}_{1} (z)= H^{(3,2)}_3 (z) = - \frac{5c^2}{12} \left[\frac{2 }{9 \epsilon}+\frac{1}{9} (4 \log (z)-1) \right] \, , \nonumber \\
&H^{(3,2)}_{2} (z)= - \frac{5c^2}{12} \left[\frac{1}{9 \epsilon}+\frac{1}{54} (12 \log (z)-13) \right] \, .
\end{align}
]]></tex-math></disp-formula></p>
<p>Combining all contributions so far, we have
<disp-formula id="ptx154-M105"><label>(105)</label><tex-math notation="LaTeX" id="Equation105"><![CDATA[
\begin{align}
&z^{-4} \lim_{y \to - \infty} |y|^{4 - 2 \epsilon} \langle W_{-1} (z) J^{(2)} (y)\rangle \nonumber \\
&\quad= -1- \frac{1}{c} \left[ \frac{6}{\epsilon}+24 \log (z)+23 \right] \nonumber \\
&\qquad+ \left(\frac{6}{c} \right)^2
\frac{-5 c }{2} \cdot \left[ -\frac{2 }{3 \epsilon} +
\frac{1}{18} (13- 12 \log (z)) \right] + \left(\frac{6}{c}\right)^3 [2 H^{(3,2)}_1 (z)+ H^{(3,2)}_2 (z)] + \cdots \, .\nonumber \\
\end{align}
]]></tex-math></disp-formula></p>
<p>The above expression reduces to
<disp-formula id="ptx154-M106"><label>(106)</label><tex-math notation="LaTeX" id="Equation106"><![CDATA[
\begin{align}
- 1 + \frac{1}{c} \left( \frac{4}{\epsilon} - 64 \log (z) - \frac{139}{3} \right)
=z^{-2} \left[ -1 + \frac{1}{c} \left( \frac{36}{\epsilon} - 19 \right) \right] \langle W_{-1} (z) \rangle \, .
\label{wj2}
\end{align}
]]></tex-math></disp-formula></p>
<p>As before, we choose the parameter <inline-formula><tex-math notation="LaTeX" id="ImEquation437"><![CDATA[$c_2$]]></tex-math></inline-formula> in Eq. (<xref ref-type="disp-formula" rid="ptx154-M58">58</xref>) as
<disp-formula id="ptx154-M107"><label>(107)</label><tex-math notation="LaTeX" id="Equation107"><![CDATA[
\begin{align}
c_2 = 1 + \frac{1}{c} \left( \frac{36}{\epsilon} + 13 \right) + \mathcal{O}(c^{-2}) \, .
\label{level2c32}
\end{align}
]]></tex-math></disp-formula></p>
<p>This leads to an extra contribution up to the <inline-formula><tex-math notation="LaTeX" id="ImEquation438"><![CDATA[$1/c$]]></tex-math></inline-formula> order from
<disp-formula id="ptx154-M108"><label>(108)</label><tex-math notation="LaTeX" id="Equation108"><![CDATA[
\begin{align}
\left.
z^{-4} \lim_{y \to - \infty} |y|^{4 - 2 \epsilon} \frac{6c_2}{c} \langle W^{(1)}_{-1} (z) J^{(2)} (y) \rangle
\right|_{\mathcal{O}(c^{-1})} = - \frac{1}{c} \left( \frac{36}{\epsilon} + 13 \right)
\end{align}
]]></tex-math></disp-formula>
with <inline-formula><tex-math notation="LaTeX" id="ImEquation439"><![CDATA[$W^{(1)}_{h_0}$]]></tex-math></inline-formula> in Eq. (<xref ref-type="disp-formula" rid="ptx154-M64">64</xref>). We can see that this contribution cancels the divergence in Eq. (<xref ref-type="disp-formula" rid="ptx154-M106">106</xref>) as
<disp-formula id="ptx154-M109"><label>(109)</label><tex-math notation="LaTeX" id="Equation109"><![CDATA[
\begin{align}
&z^{-4} \lim_{y \to - \infty} |y|^{4 - 2 \epsilon } \langle W_{-1} (z) J^{(2)} (y)\rangle
=z^{-2} \left[ -1 - \frac{32}{c} \right] \langle W_{-1} (z) \rangle + \mathcal{O}(c^{-2})
\end{align}
]]></tex-math></disp-formula>
for <inline-formula><tex-math notation="LaTeX" id="ImEquation440"><![CDATA[$\epsilon \to 0$]]></tex-math></inline-formula>. The constant term in Eq. (<xref ref-type="disp-formula" rid="ptx154-M107">107</xref>) is chosen in order to reproduce Eq. (<xref ref-type="disp-formula" rid="ptx154-M62">62</xref>) with <inline-formula><tex-math notation="LaTeX" id="ImEquation441"><![CDATA[$h_1 = - 32$]]></tex-math></inline-formula> as in Eq. (<xref ref-type="disp-formula" rid="ptx154-M91">91</xref>).</p>
<p>We would like to compute another correlator as <inline-formula><tex-math notation="LaTeX" id="ImEquation442"><![CDATA[$ \langle W_{-1} (z) J^{(3)}(y) \rangle $]]></tex-math></inline-formula> with spin-three current at the <inline-formula><tex-math notation="LaTeX" id="ImEquation443"><![CDATA[$1/c$]]></tex-math></inline-formula> order. Using the leading-order result in Eq. (<xref ref-type="disp-formula" rid="ptx154-M55">55</xref>) with <inline-formula><tex-math notation="LaTeX" id="ImEquation444"><![CDATA[$h_0 = -1$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation445"><![CDATA[$s=3$]]></tex-math></inline-formula>, and the <inline-formula><tex-math notation="LaTeX" id="ImEquation446"><![CDATA[$1/c$]]></tex-math></inline-formula> correction as <inline-formula><tex-math notation="LaTeX" id="ImEquation447"><![CDATA[$C_{1}^{(3)}/C_{0}^{(3)} = 224/5$]]></tex-math></inline-formula> obtained in <xref ref-type="sec" rid="SEC2">Sect. 2</xref>, the corresponding three-point function is given by
<disp-formula id="ptx154-M110"><label>(110)</label><tex-math notation="LaTeX" id="Equation110"><![CDATA[
\begin{align}
\langle \mathcal{O}_{h_+} (z) \bar{\mathcal{O}}_{h_+} (0) J^{(3)} (y) \rangle = \frac{1}{3}\left[ 1 + \frac1c \frac{224}{5} \right] \left( \frac{z}{(y - z) y} \right)^3 \langle \mathcal{O}_{h_+} (z) \bar{\mathcal{O}}_{h_+} (0) \rangle + \mathcal{O}(c^{-2}) \, .
\label{3pts3N3}
\end{align}
]]></tex-math></disp-formula></p>
<p>Following the prescription discussed in <xref ref-type="sec" rid="SEC3.4">Sect. 3.4</xref>, we choose the parameter <inline-formula><tex-math notation="LaTeX" id="ImEquation448"><![CDATA[$c_3$]]></tex-math></inline-formula> in Eq. (<xref ref-type="disp-formula" rid="ptx154-M58">58</xref>) such that the Wilson line computation reproduces this expression.</p>
<p>With two current insertions from an open Wilson line, we have the following type of contribution as
<disp-formula id="ptx154-M111"><label>(111)</label><tex-math notation="LaTeX" id="Equation111"><![CDATA[
\begin{align}
H^{(2,3)} (z)& = \lim_{y \to - \infty} |y|^{6 -2 \epsilon} z^{-5} \int_0^z dz_2 \int_0^{z_2} dz_1 \left[ f^{(3,2)}_2 (z_2 , z_1) \right . \langle J^{(3)} (z_2) J^{(2)} (z_1) J^{(3)} (y) \rangle \nonumber \\
& \qquad \qquad \qquad \qquad + \left. f^{(2,3)}_2 (z_2 , z_1) \langle J^{(2)} (z_2) J^{(3)} (z_1)J^{(3)} (y) \rangle \right] \nonumber \\
& =- \frac{5 c}{2} \left[ -\frac{4 }{15 \epsilon} + \frac{1 }{225} (107-60 \log (z)) \right] \, ,
\end{align}
]]></tex-math></disp-formula>
which come from diagrams (a), (b) in <xref ref-type="fig" rid="F6">Fig. 6</xref>. For the correlator of the three currents, we have used Eq. (<xref ref-type="disp-formula" rid="ptx154-M100">100</xref>). There are contributions with two spin-two and two spin-three currents. With the correlator in Eq. (<xref ref-type="disp-formula" rid="ptx154-M102">102</xref>), they are given by</p>
<fig id="F6" orientation="portrait" position="float"><label>Fig. 6.</label><caption><p>Diagrams contributing to the <inline-formula><tex-math notation="LaTeX" id="ImEquation449"><![CDATA[$1/c$]]></tex-math></inline-formula>-order correction of <inline-formula><tex-math notation="LaTeX" id="ImEquation450"><![CDATA[$\langle \mathcal{O}_{h_+} \bar{\mathcal{O}}_{h_+} J^{(3)} \rangle $]]></tex-math></inline-formula> for <inline-formula><tex-math notation="LaTeX" id="ImEquation451"><![CDATA[$N=3$]]></tex-math></inline-formula>.</p></caption>
<graphic xmlns:xlink="http://www.w3.org/1999/xlink" orientation="portrait" position="float" xlink:href="ptx154F6.tif"/></fig>
<p><disp-formula id="ptx154-M112"><label>(112)</label><tex-math notation="LaTeX" id="Equation112"><![CDATA[
\begin{align}
H^{(3,3)}_{1} (z)= - \frac{5 c^2 }{12} z^{-5} \int_0^{z} dz_3 \int_0^{z_3} dz_2 \int_0^{z_2} dz_1
f^{(3,2,2)}_3 (z_3 , z_2 , z_1 ) \frac{1}{z_{21}^{4 -2 \epsilon}} \, , \nonumber \\
H^{(3,3)}_{2} (z)= - \frac{5 c^2 }{12} z^{-5} \int_0^{z} dz_3 \int_0^{z_3} dz_2 \int_0^{z_2} dz_1
f^{(2,3,2)}_3 (z_3 , z_2 , z_1 ) \frac{1}{z_{31}^{4 -2 \epsilon}} \, , \nonumber \\
H^{(3,3)}_{3} (z)= - \frac{5 c^2 }{12} z^{-5} \int_0^{z} dz_3 \int_0^{z_3} dz_2 \int_0^{z_2} dz_1
f^{(2,2,3)}_3 (z_3 , z_2 , z_1 ) \frac{1}{z_{32}^{4 - 2 \epsilon}} \, ,
\end{align}
]]></tex-math></disp-formula>
which correspond to diagrams (c), (d), (e) in <xref ref-type="fig" rid="F6">Fig. 6</xref>. Integrating over the variables <inline-formula><tex-math notation="LaTeX" id="ImEquation452"><![CDATA[$z_1,z_2,z_3$]]></tex-math></inline-formula>, we find
<disp-formula id="ptx154-M113"><label>(113)</label><tex-math notation="LaTeX" id="Equation113"><![CDATA[
\begin{align}
&H^{(3,3)}_{1} (z)= H^{(3,3)}_{3} (z)= - \frac{5 c^2 }{12} \cdot \left[\frac{2 }{45 \epsilon}+\frac{4}{225} (5 \log (z)-1)\right] \, , \nonumber \\
&H^{(3,3)}_{2} (z)=- \frac{5 c^2 }{12} \cdot \left[ \frac{1}{45 \epsilon}+\frac{2}{675} (15 \log (z)-26) \right] \, .
\end{align}
]]></tex-math></disp-formula></p>
<p>Furthermore, we need to consider a contribution of the form as
<disp-formula id="ptx154-M114"><label>(114)</label><tex-math notation="LaTeX" id="Equation114"><![CDATA[
\begin{align}
\int_0^z d z_3 \int_0^{z_3} d z_2 \int_0^{z_2} dz_1 f_3 ^{(3,3,3)} ( z_3,z_2 ,z_1) \langle J^{(3)} (z_3) J^{(3)} (z_2) J^{(3)} (z_1) J^{(3)} (y) \rangle
\end{align}
]]></tex-math></disp-formula>
with
<disp-formula id="ptx154-M115"><label>(115)</label><tex-math notation="LaTeX" id="Equation115"><![CDATA[
\begin{align}
&\langle J^{(3)} (z_3)J^{(3)} (z_2)J^{(3)} (z_1) J^{(3)} (y) \rangle \nonumber \\
&\quad = \frac{(5c/6)^2}{z_{32}^{6 - 2 \epsilon} (z_1 - y )^{6 - 2 \epsilon} } +
\frac{(5c/6)^2}{ z_{31}^{6 - 2 \epsilon } ( z_2 - y )^{ 6 - 2 \epsilon }} + \frac{(5c/6)^2}{z_{21}^{6 - 2 \epsilon} (z_3 - y)^{ 6 - 2 \epsilon} } + \mathcal{O}(c)\, .
\end{align}
]]></tex-math></disp-formula></p>
<p>Denoting
<disp-formula id="ptx154-M116"><label>(116)</label><tex-math notation="LaTeX" id="Equation116"><![CDATA[
\begin{align}
H^{(3,3)}_{ij} (z) = \left(\frac{5c}{6} \right)^2 z^{-5}
\int_0^z d z_3 \int_0^{z_3} d z_2 \int_0^{z_2} dz_1 f_3 ^{(3,3,3)} ( z_3,z_2 ,z_1)
\frac{1}{z_{ji}^{6 - 2\epsilon} } \, ,
\end{align}
]]></tex-math></disp-formula>
we find
<disp-formula id="ptx154-M117"><label>(117)</label><tex-math notation="LaTeX" id="Equation117"><![CDATA[
\begin{align}
H^{(3,3)}_{12} (z)& =H^{(3,3)}_{23} (z) = \left(\frac{5c}{6} \right)^2 \left[-\frac{2 }{45 \epsilon} + \frac{1}{225} (9-20 \log (z)) \right] \, ,\nonumber \\
H^{(3,3)}_{13} (z)& = \left(\frac{5c}{6} \right)^2 \left[ \frac{1}{225 \epsilon} + \frac{1}{6750}(60 \log (z)-137) \right] \, .
\end{align}
]]></tex-math></disp-formula></p>
<p>Here <inline-formula><tex-math notation="LaTeX" id="ImEquation453"><![CDATA[$H^{(3,3)}_{12} (z)$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation454"><![CDATA[$H^{(3,3)}_{13} (z)$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation455"><![CDATA[$H^{(3,3)}_{23} (z)$]]></tex-math></inline-formula> correspond to diagrams (f), (g), (h) in <xref ref-type="fig" rid="F6">Fig. 6</xref>.</p>
<p>Combining the results so far as
<disp-formula id="ptx154-M118"><label>(118)</label><tex-math notation="LaTeX" id="Equation118"><![CDATA[
\begin{align}
& z^{ - 5} \lim_{y \to - \infty} |y|^{6 - 2 \epsilon } \langle W_{-1} (z) J^{(3)}(y) \rangle \nonumber\\
& \quad = \frac{1}{3} - \left( \frac{6}{c} \right)^2 H^{(2,3)} - \left( \frac{6}{c} \right)^3
\left[2 H^{(3,3)}_1 (z) +H^{(3,3)}_2 (z) + 2 H^{(3,3)}_{21} (z)+ H^{(3,3)}_{31} (z) \right] + \cdots \, ,
\end{align}
]]></tex-math></disp-formula>
we find
<disp-formula id="ptx154-M119"><label>(119)</label><tex-math notation="LaTeX" id="Equation119"><![CDATA[
\begin{align}
z^{-5 } \lim_{y \to - \infty} |y|^{6 - 2 \epsilon } \langle W_{-1} (z) J^{(3)}(y) \rangle &= \frac{1}{3} +
\frac{1}{c} \left( -\frac{4}{3 \epsilon}+\frac{64 \log (z)}{3}+\frac{1067}{45} \right) + \cdots
\nonumber \\ &= z^{-2} \left[ \frac{1}{3} +
\frac{1}{ c} \left( - \frac{12}{\epsilon} + \frac{657}{45} \right) \right] \langle W_{-1} (z) \rangle + \cdots \, .
\end{align}
]]></tex-math></disp-formula></p>
<p>We remove the divergent term by properly choosing the parameter <inline-formula><tex-math notation="LaTeX" id="ImEquation456"><![CDATA[$c_3$]]></tex-math></inline-formula> in Eq. (<xref ref-type="disp-formula" rid="ptx154-M58">58</xref>) as before. We propose to use
<disp-formula id="ptx154-M120"><label>(120)</label><tex-math notation="LaTeX" id="Equation120"><![CDATA[
\begin{align}
c_3 = 1 + \frac{1}{c} \left( \frac{36}{\epsilon} + 1 \right) + \mathcal{O} (c^{-2}) \, ,
\label{level2c33}
\end{align}
]]></tex-math></disp-formula>
which leads to an extra contribution at the <inline-formula><tex-math notation="LaTeX" id="ImEquation457"><![CDATA[$1/c$]]></tex-math></inline-formula> order as
<disp-formula id="ptx154-M121"><label>(121)</label><tex-math notation="LaTeX" id="Equation121"><![CDATA[
\begin{align}
\left. z^{-5} \lim_{y \to - \infty} |y|^{6 - 2\epsilon } \frac{6 c_3}{c} \langle W^{(1)'}_{-1} (z) J^{(3)} (y) \rangle \right|_{\mathcal{O} (c^{-1})} = \frac{1}{c} \frac{1}{3} \left( \frac{36}{\epsilon} + 1 \right) \, .
\end{align}
]]></tex-math></disp-formula></p>
<p>Here <inline-formula><tex-math notation="LaTeX" id="ImEquation458"><![CDATA[$W^{(1)'}_{-1} (z)$]]></tex-math></inline-formula> is defined as
<disp-formula id="ptx154-M122"><label>(122)</label><tex-math notation="LaTeX" id="Equation122"><![CDATA[
\begin{align}
W^{(1)'}_{h_0} = \int_0^z d z_1 f^{(3)}_1 (z_1) J^{(3)} (z_1) \, .
\label{W1p}
\end{align}
]]></tex-math></disp-formula></p>
<p>Including the effect, we obtain
<disp-formula id="ptx154-M123"><label>(123)</label><tex-math notation="LaTeX" id="Equation123"><![CDATA[
\begin{align}
\lim_{y \to - \infty} |y|^{6 - 2 \epsilon } \langle W_{-1} (z) J^{(3)}(y) \rangle = \frac{1}{3} z^3 \left[ 1 +
\frac{1}{ c} \frac{224}{5} \right] \langle W_{-1} (z) \rangle + \mathcal{O} (c^{-2})
\end{align}
]]></tex-math></disp-formula>
for <inline-formula><tex-math notation="LaTeX" id="ImEquation459"><![CDATA[$\epsilon \to 0$]]></tex-math></inline-formula> as in Eq. (<xref ref-type="disp-formula" rid="ptx154-M110">110</xref>).</p>
</sec>
<sec id="SEC5.3"><title>5.3. Two-point function at <inline-formula><tex-math notation="LaTeX" id="ImEquation460"><![CDATA[$1/c^2$]]></tex-math></inline-formula> order</title>
<p>As for <inline-formula><tex-math notation="LaTeX" id="ImEquation461"><![CDATA[$N=2$]]></tex-math></inline-formula>, we examine the two-point function up to the <inline-formula><tex-math notation="LaTeX" id="ImEquation462"><![CDATA[$1/c^2$]]></tex-math></inline-formula> order and see whether we can reproduce the <inline-formula><tex-math notation="LaTeX" id="ImEquation463"><![CDATA[$1/c$]]></tex-math></inline-formula> correction of conformal weight as in Eq. (<xref ref-type="disp-formula" rid="ptx154-M91">91</xref>) after adopting the regularization. As before, we first evaluate the <inline-formula><tex-math notation="LaTeX" id="ImEquation464"><![CDATA[$1/c$]]></tex-math></inline-formula> correction without renormalization and then include its effects.</p>
<p>There are contributions involving only spin-two currents, which were already evaluated in Eq. (<xref ref-type="disp-formula" rid="ptx154-M86">86</xref>). We find
<disp-formula id="ptx154-M124"><label>(124)</label><tex-math notation="LaTeX" id="Equation124"><![CDATA[
\begin{align}
c^2 z^{-2} G^{(2)}_\text{spin 2} (z) = 72 \log (z) (4 \log (z)+7)
\end{align}
]]></tex-math></disp-formula>
by setting <inline-formula><tex-math notation="LaTeX" id="ImEquation465"><![CDATA[$h_0 = -1$]]></tex-math></inline-formula>. In this subsection, we only keep the terms involving <inline-formula><tex-math notation="LaTeX" id="ImEquation466"><![CDATA[$\log (z)$]]></tex-math></inline-formula> or <inline-formula><tex-math notation="LaTeX" id="ImEquation467"><![CDATA[$\log ^2 (z)$]]></tex-math></inline-formula> and not vanishing at <inline-formula><tex-math notation="LaTeX" id="ImEquation468"><![CDATA[$\epsilon \to 0$]]></tex-math></inline-formula>.</p>
<p>Furthermore, we include the effects of spin-three current <inline-formula><tex-math notation="LaTeX" id="ImEquation469"><![CDATA[$J^{(3)}$]]></tex-math></inline-formula>. In order to make our notation simpler, we adopt the following rule. If <inline-formula><tex-math notation="LaTeX" id="ImEquation470"><![CDATA[$J^{(2)} (z_i)$]]></tex-math></inline-formula> comes from the open Wilson line, then we use index <inline-formula><tex-math notation="LaTeX" id="ImEquation471"><![CDATA[$i$]]></tex-math></inline-formula>. If <inline-formula><tex-math notation="LaTeX" id="ImEquation472"><![CDATA[$J^{(3)} (z_i)$]]></tex-math></inline-formula> enters instead of <inline-formula><tex-math notation="LaTeX" id="ImEquation473"><![CDATA[$J^{(2)} (z_i)$]]></tex-math></inline-formula>, then we replace the index <inline-formula><tex-math notation="LaTeX" id="ImEquation474"><![CDATA[$i$]]></tex-math></inline-formula> by <inline-formula><tex-math notation="LaTeX" id="ImEquation475"><![CDATA[${\boldsymbol{i}}$]]></tex-math></inline-formula>. We first compute those with three currents as
<disp-formula id="ptx154-M125"><label>(125)</label><tex-math notation="LaTeX" id="Equation125"><![CDATA[
\begin{align}
G^{(2)}_{1{\boldsymbol{23}}} (z) = & \left( \frac{6}{c}\right)^3 \int_0^z d z_3 \int_0^{z_3} d z_2 \int_0^{z_2} dz_1 f_3^{(3,3,2)} ( z_3,z_2 ,z_1) \frac{- 5 c/2}{ z_{32}^{4- \epsilon} z_{31}^{2-\epsilon} z_{21}^{2- \epsilon} } \, ,
\end{align}
]]></tex-math></disp-formula>
and <inline-formula><tex-math notation="LaTeX" id="ImEquation476"><![CDATA[$G_{{\boldsymbol 1}2{\boldsymbol 3}}^{(2)} (z)$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation477"><![CDATA[$G_{{\boldsymbol 12}3}^{(2)} (z)$]]></tex-math></inline-formula>, which are represented by diagrams (a), (b), (c) in <xref ref-type="fig" rid="F7">Fig. 7</xref>, respectively. Integrations over <inline-formula><tex-math notation="LaTeX" id="ImEquation478"><![CDATA[$z_i$]]></tex-math></inline-formula> yield</p>
<fig id="F7" orientation="portrait" position="float"><label>Fig. 7.</label><caption><p>Diagrams contributing to the <inline-formula><tex-math notation="LaTeX" id="ImEquation479"><![CDATA[$1/c^2$]]></tex-math></inline-formula>-order correction of <inline-formula><tex-math notation="LaTeX" id="ImEquation480"><![CDATA[$\langle \mathcal{O}_{h_+} \bar{\mathcal{O}}_{h_+} \rangle $]]></tex-math></inline-formula> for <inline-formula><tex-math notation="LaTeX" id="ImEquation481"><![CDATA[$N=3$]]></tex-math></inline-formula> in addition to the ones in <xref ref-type="fig" rid="F3">Fig. 3</xref>.</p></caption>
<graphic xmlns:xlink="http://www.w3.org/1999/xlink" orientation="portrait" position="float" xlink:href="ptx154F7.tif"/></fig>
<p><disp-formula id="ptx154-M126"><label>(126)</label><tex-math notation="LaTeX" id="Equation126"><![CDATA[
\begin{align}
&c^2 z^{-2} G_{1{\boldsymbol{23}}}^{(2)} (z) = c^2 z^{-2} G_{{\boldsymbol{12}}3}^{(2)} (z) = -\frac{ 2880 \log (z) }{\epsilon} - 4320 \log (z) (\log (z)+1) \, , \nonumber \\
&c^2 z^{-2}G_{{\boldsymbol{1}}2{\boldsymbol{3}}}^{(2)} (z) =-\frac{ 2880 \log (z)}{\epsilon}- 1440 \log (z) (3 \log (z)+2) \, .
\end{align}
]]></tex-math></disp-formula></p>
<p>There are also contributions with two spin-two and two spin-three currents such as
<disp-formula id="ptx154-M127"><label>(127)</label><tex-math notation="LaTeX" id="Equation127"><![CDATA[
\begin{align}
G^{(2)}_{12;{\boldsymbol{34}}} (z) = & \left( \frac{6}{c}\right)^4 \int_0^z d z_3 \int_0^{z_3} d z_2 \int_0^{z_2} dz_1 f_4^{(3,3,2,2)} ( z_4,z_3 ,z_2,z_1) \frac{- 5 c^2 /12}{z_{43}^{6- 2\epsilon} z_{21}^{4- 2\epsilon} } \, ,
\end{align}
]]></tex-math></disp-formula>
and so on. They are computed as
<disp-formula id="ptx154-M128"><label>(128)</label><tex-math notation="LaTeX" id="Equation128"><![CDATA[
\begin{align}
&c^2 z^{-2} G_{12;{\boldsymbol{34}}}^{(2)} (z) =c^2 z^{-2} G_{{\boldsymbol{12};34}}^{(2)} (z) = \frac{ 960 \log (z)}{\epsilon} + 160 \log (z) (12 \log (z)+11) \, , \nonumber \\
&c^2 z^{-2} G_{14;{\boldsymbol{23}}}^{(2)} (z) = \frac{480 \log (z)}{\epsilon} + 240 \log (z) \left( 4 \log (z)+ 9\right)\, ,\nonumber \\
&c^2 z^{-2} G_{{\boldsymbol{14}};23}^{(2)} (z) = \frac{480 \log (z)}{\epsilon}+ 240 \log (z) \left( 4 \log (z)+ 5 \right) \, , \nonumber \\
&c^2 z^{-2} G_{13;{\boldsymbol{24}}}^{(2)} (z) = c^2 G_{{\boldsymbol 13;24}}^{(2)} (z) = \frac{480 \log (z)}{\epsilon} + 350 \log (z) \left( \log (z)+ 4 \right) \, ,
\end{align}
]]></tex-math></disp-formula>
which correspond to diagrams (d)&#x2013;(i) in <xref ref-type="fig" rid="F7">Fig. 7</xref>. Finally, those with four spin-three currents are
<disp-formula id="ptx154-M129"><label>(129)</label><tex-math notation="LaTeX" id="Equation129"><![CDATA[
\begin{align}
G^{(2)}_{{\boldsymbol 12;34}} (z) = & \left( \frac{6}{c}\right)^4 \int_0^z d z_3 \int_0^{z_3} d z_2 \int_0^{z_2} dz_1 f_4^{(3,3,3,3)} (z_4, z_3,z_2 ,z_1) \frac{(5 c/6)^2}{z_{43}^{6- 2 \epsilon} z_{21}^{6- 2\epsilon} }
\end{align}
]]></tex-math></disp-formula>
and others with different products of the two-point function. They are obtained as
<disp-formula id="ptx154-M130"><label>(130)</label><tex-math notation="LaTeX" id="Equation130"><![CDATA[
\begin{align}
&c^2 z^{-2} G_{{\boldsymbol 12;34}}^{(2)} (z) = \frac{1600 \log (z)}{ \epsilon} + \frac{3200}{3} \left( \log (z) (3 \log (z)+2) \right) \, , \nonumber \\
&c^2 z^{-2} G_{{\boldsymbol 14;23}}^{(2)} (z) = \frac{800 \log (z)}{\epsilon}+1600 \log (z) (\log (z)+1)\, , \nonumber \\
&c^2 z^{-2} G_{{\boldsymbol 13;24}}^{(2)} (z) = -\frac{160 \log (z) }{ \epsilon} - \frac{8}{3} \log (z) (120 \log (z)+127) \, ,
\end{align}
]]></tex-math></disp-formula>
which are represented in diagrams (j), (k), (l) in <xref ref-type="fig" rid="F7">Fig. 7</xref>, respectively. Summing up all contributions we have
<disp-formula id="ptx154-M131"><label>(131)</label><tex-math notation="LaTeX" id="Equation131"><![CDATA[
\begin{align}
c^2 z^{-2} G^{(2)} (z) = &
-\frac{2560 \log (z) }{\epsilon} -\frac{32}{3} \log (z) (48 \log (z)-193) \, ,
\end{align}
]]></tex-math></disp-formula>
which includes a non-locally divergent term.</p>
<p>Let us then examine the effects of renormalization. There are two types of <inline-formula><tex-math notation="LaTeX" id="ImEquation482"><![CDATA[$1/c$]]></tex-math></inline-formula>-order corrections as in Eq. (<xref ref-type="disp-formula" rid="ptx154-M92">92</xref>) before the renormalization. Multiplying the <inline-formula><tex-math notation="LaTeX" id="ImEquation483"><![CDATA[$1/c$]]></tex-math></inline-formula> terms due to renormalization, some contributions at the <inline-formula><tex-math notation="LaTeX" id="ImEquation484"><![CDATA[$1/c^2$]]></tex-math></inline-formula> order arise. With Eqs. (<xref ref-type="disp-formula" rid="ptx154-M107">107</xref>) and (<xref ref-type="disp-formula" rid="ptx154-M97">97</xref>), the contribution with spin-two current becomes
<disp-formula id="ptx154-M132"><label>(132)</label><tex-math notation="LaTeX" id="Equation132"><![CDATA[
\begin{align}
&\frac{1}{c}\left[ 2 \left( \frac{36}{ \epsilon} + 13 \right) - \frac{32}{\epsilon} - \frac{82}{3} \right] \left(\frac{6}{c} \right)^2 \langle W^{(2)}_{-1} (z) \rangle \nonumber \\
& \quad = \frac{1}{c} \left[\frac{960 z^2 \log (z)}{\epsilon} + 64 z^2 \log (z) (15 \log (z)+17) \right] \, ;
\end{align}
]]></tex-math></disp-formula>
see Eq. (<xref ref-type="disp-formula" rid="ptx154-M88">88</xref>) for the previous case with <inline-formula><tex-math notation="LaTeX" id="ImEquation485"><![CDATA[$N=2$]]></tex-math></inline-formula>. The contribution with spin-three current is
<disp-formula id="ptx154-M133"><label>(133)</label><tex-math notation="LaTeX" id="Equation133"><![CDATA[
\begin{align}
&\frac{1}{c} \left[ 2 \left( \frac{36}{ \epsilon} + 1 \right) - \frac{32}{ \epsilon} - \frac{82}{3} \right] \left(\frac{6}{c} \right)^2 \langle W^{(2)'}_{-1} (z) \rangle \nonumber \\
& \quad = \frac{1}{c} \left[ \frac{1600 z^2 \log (z)}{ \epsilon} +\frac{160}{3} z^2 \log (z) \left(30 \log (z)+ 1 \right) \right] \, ,
\end{align}
]]></tex-math></disp-formula>
where we have used Eqs. (<xref ref-type="disp-formula" rid="ptx154-M120">120</xref>) and (<xref ref-type="disp-formula" rid="ptx154-M97">97</xref>). Thus the <inline-formula><tex-math notation="LaTeX" id="ImEquation486"><![CDATA[$\log(z)$]]></tex-math></inline-formula>- and <inline-formula><tex-math notation="LaTeX" id="ImEquation487"><![CDATA[$\log ^2 (z)$]]></tex-math></inline-formula>-dependent terms in the total contribution are
<disp-formula id="ptx154-M134"><label>(134)</label><tex-math notation="LaTeX" id="Equation134"><![CDATA[
\begin{align}
& c^2 z^{-2} \left. \langle \tilde W_{h_0} (z) \rangle \right|_{\mathcal{O}(c^{0})} = 3200 \log (z) + 2048 \log ^2 (z) \, .
\end{align}
]]></tex-math></disp-formula></p>
<p>The coefficients in front of <inline-formula><tex-math notation="LaTeX" id="ImEquation488"><![CDATA[$\log (z)$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation489"><![CDATA[$\log ^2 ( z)$]]></tex-math></inline-formula> are precisely those in Eq. (<xref ref-type="disp-formula" rid="ptx154-M10">10</xref>) with Eq. (<xref ref-type="disp-formula" rid="ptx154-M91">91</xref>). We would like to emphasize again that there is cancellation among non-local divergences.</p>
</sec>
</sec>
<sec sec-type="conclusion|discussions" id="SEC6"><title>6. Conclusion and discussions</title>
<p>We have examined the two- and three-point functions (<xref ref-type="disp-formula" rid="ptx154-M3">3</xref>) of the 2D W<inline-formula><tex-math notation="LaTeX" id="ImEquation490"><![CDATA[$_N$]]></tex-math></inline-formula> minimal model in <inline-formula><tex-math notation="LaTeX" id="ImEquation491"><![CDATA[$1/c$]]></tex-math></inline-formula> expansion from the bulk viewpoint. Extending a previous work of Ref. [<xref ref-type="bibr" rid="B16">16</xref>] at the leading order in <inline-formula><tex-math notation="LaTeX" id="ImEquation492"><![CDATA[$1/c$]]></tex-math></inline-formula>, we claim that these correlators can be computed with open Wilson lines in sl<inline-formula><tex-math notation="LaTeX" id="ImEquation493"><![CDATA[$(N)$]]></tex-math></inline-formula> Chern&#x2013;Simons gauge theory as in Eqs. (<xref ref-type="disp-formula" rid="ptx154-M49">49</xref>) and (<xref ref-type="disp-formula" rid="ptx154-M51">51</xref>) even at higher orders in <inline-formula><tex-math notation="LaTeX" id="ImEquation494"><![CDATA[$1/c$]]></tex-math></inline-formula>. There are divergences associated with loop diagrams in the Wilson line computations, and we have to decide how to deal with them. We offer to regularize the divergences by renormalizing the overall factor of the open Wilson line and parameters <inline-formula><tex-math notation="LaTeX" id="ImEquation495"><![CDATA[$c_s$]]></tex-math></inline-formula> introduced in Eq. (<xref ref-type="disp-formula" rid="ptx154-M58">58</xref>). The finite parts of <inline-formula><tex-math notation="LaTeX" id="ImEquation496"><![CDATA[$c_s$]]></tex-math></inline-formula> are fixed such that three-point functions from Eq. (<xref ref-type="disp-formula" rid="ptx154-M51">51</xref>) are consistent with the boundary W<inline-formula><tex-math notation="LaTeX" id="ImEquation497"><![CDATA[$_N$]]></tex-math></inline-formula> symmetry. We confirm the validity of our prescription by reproducing the <inline-formula><tex-math notation="LaTeX" id="ImEquation498"><![CDATA[$1/c$]]></tex-math></inline-formula> corrections of scalar conformal weight from Eq. (<xref ref-type="disp-formula" rid="ptx154-M49">49</xref>) including <inline-formula><tex-math notation="LaTeX" id="ImEquation499"><![CDATA[$1/c^2$]]></tex-math></inline-formula>-order terms.</p>
<p>As concrete examples, we have only examined Chern&#x2013;Simons gauge theories based on sl<inline-formula><tex-math notation="LaTeX" id="ImEquation500"><![CDATA[$(N)$]]></tex-math></inline-formula> with <inline-formula><tex-math notation="LaTeX" id="ImEquation501"><![CDATA[$N=2,3$]]></tex-math></inline-formula>. For <inline-formula><tex-math notation="LaTeX" id="ImEquation502"><![CDATA[$N \geq 4$]]></tex-math></inline-formula> we see no major difference even though computations would be quite complicated. For instance, we can reproduce <inline-formula><tex-math notation="LaTeX" id="ImEquation503"><![CDATA[$h_1$]]></tex-math></inline-formula> in Eq. (<xref ref-type="disp-formula" rid="ptx154-M11">11</xref>) by evaluating integrals in Eq. (<xref ref-type="disp-formula" rid="ptx154-M49">49</xref>) up to the <inline-formula><tex-math notation="LaTeX" id="ImEquation504"><![CDATA[$1/c$]]></tex-math></inline-formula> order and comparing the <inline-formula><tex-math notation="LaTeX" id="ImEquation505"><![CDATA[$1/c$]]></tex-math></inline-formula> expansion of the two-point function in Eq. (<xref ref-type="disp-formula" rid="ptx154-M10">10</xref>). We consider the following integral as
<disp-formula id="ptx154-M135"><label>(135)</label><tex-math notation="LaTeX" id="Equation135"><![CDATA[
\begin{align}
\langle W_{(1 - N)/2}^{(1,s)} (z) \rangle \equiv - \frac{ (2 s -1) N_s}{6}
\int_0^z d z_2 \int_0^{z_2} dz_1 f^{(s,s)}_2 (z_2,z_1) \frac{1}{z_{21}^{2 s- 2 \epsilon }}
\end{align}
]]></tex-math></disp-formula>
with conformal weight <inline-formula><tex-math notation="LaTeX" id="ImEquation506"><![CDATA[$(1-N)/2$]]></tex-math></inline-formula>. The term including <inline-formula><tex-math notation="LaTeX" id="ImEquation507"><![CDATA[$\log(z)$]]></tex-math></inline-formula> at the order <inline-formula><tex-math notation="LaTeX" id="ImEquation508"><![CDATA[$\epsilon^0$]]></tex-math></inline-formula> is evaluated as
<disp-formula id="ptx154-M136"><label>(136)</label><tex-math notation="LaTeX" id="Equation136"><![CDATA[
\begin{align}
\langle W_{(1-N)/2}^{(1,s)} (z) \rangle |_{\log , \epsilon^0}
= (2 s -1) (N^2-1) \left(- \frac{N_s}{6} \right) ^2 z^{N-1} \log(z)
\end{align}
]]></tex-math></disp-formula>
for <inline-formula><tex-math notation="LaTeX" id="ImEquation509"><![CDATA[$s=2,3, \ldots ,10$]]></tex-math></inline-formula>. We conjecture that the above equality also holds for <inline-formula><tex-math notation="LaTeX" id="ImEquation510"><![CDATA[$s > 10$]]></tex-math></inline-formula>. Then, the <inline-formula><tex-math notation="LaTeX" id="ImEquation511"><![CDATA[$1/c$]]></tex-math></inline-formula>-order correction of scalar conformal weight for generic <inline-formula><tex-math notation="LaTeX" id="ImEquation512"><![CDATA[$N$]]></tex-math></inline-formula> can be read off as
<disp-formula id="ptx154-M137"><label>(137)</label><tex-math notation="LaTeX" id="Equation137"><![CDATA[
\begin{align}
- \frac{1}{2} \sum_{s = 2}^N \left(- \frac{6}{N_s} \right) ^2 (2 s -1) (N^2-1) \left(- \frac{N_s}{6} \right) ^2 = - \frac{(N^2 - 1)^2}{2} \, ,
\end{align}
]]></tex-math></disp-formula>
which matches <inline-formula><tex-math notation="LaTeX" id="ImEquation513"><![CDATA[$h_1$]]></tex-math></inline-formula> in Eq. (<xref ref-type="disp-formula" rid="ptx154-M11">11</xref>). For our purpose it is enough to work with the non-unitary duality, but other problems may require a unitary one, i.e., the &#x2019;t Hooft limit of Ref. [<xref ref-type="bibr" rid="B11">11</xref>]; see footnote 2. For the unitary duality, we should extend the analysis to the case with a higher-spin algebra hs<inline-formula><tex-math notation="LaTeX" id="ImEquation514"><![CDATA[$[\lambda]$]]></tex-math></inline-formula>, which is a gauge algebra of 3D Prokushkin&#x2013;Vasiliev theory [<xref ref-type="bibr" rid="B12">12</xref>]. In particular, we would like to understand the precise relation between open Wilson lines and particles traveling in the bulk.</p>
<p>An important open problem is to confirm our proposal that correlators in the 2D W<inline-formula><tex-math notation="LaTeX" id="ImEquation515"><![CDATA[$_N$]]></tex-math></inline-formula> minimal model can be computed with open Wilson lines in sl<inline-formula><tex-math notation="LaTeX" id="ImEquation516"><![CDATA[$(N)$]]></tex-math></inline-formula> Chern&#x2013;Simons gauge theory including <inline-formula><tex-math notation="LaTeX" id="ImEquation517"><![CDATA[$1/c$]]></tex-math></inline-formula> corrections. In particular, we have to extend the checks to higher orders in <inline-formula><tex-math notation="LaTeX" id="ImEquation518"><![CDATA[$1/c$]]></tex-math></inline-formula>. We have conjectured that all divergences are removed by renormalizing the overall factor of the open Wilson line and the parameters <inline-formula><tex-math notation="LaTeX" id="ImEquation519"><![CDATA[$c_s$]]></tex-math></inline-formula> in Eq. (<xref ref-type="disp-formula" rid="ptx154-M58">58</xref>), but it is desirable to prove this claim. A different regulator was introduced in Ref. [<xref ref-type="bibr" rid="B24">24</xref>] by shifting <inline-formula><tex-math notation="LaTeX" id="ImEquation520"><![CDATA[$1/(z_{21}^2)^a \to 1/(z_{21}^2 + \epsilon^2)^a$]]></tex-math></inline-formula>, but it breaks conformal symmetry. We can see that divergences from loop computations with this regulator cannot be absorbed by these changes; thus conformal symmetry in the regularization procedure should play an important role.</p>
<p>We have proposed our regularization prescription so as to be analogous to that for the usual quantum field theory even though the precise relation is yet to be clarified. We offer to fix the interaction parameters by comparing them to &#x201C;experimental data&#x201D; that are obtained from dual conformal field theory in the current situation. Once they are fixed, then other quantities like the self-energy of the scalar propagator are claimed to be predictable. A particularly nice thing happens for <inline-formula><tex-math notation="LaTeX" id="ImEquation521"><![CDATA[$N=2$]]></tex-math></inline-formula>. In this case, the <inline-formula><tex-math notation="LaTeX" id="ImEquation522"><![CDATA[$1/c$]]></tex-math></inline-formula> order of the interaction parameter <inline-formula><tex-math notation="LaTeX" id="ImEquation523"><![CDATA[$c^{(1)}_2$]]></tex-math></inline-formula> was determined by using the information on <inline-formula><tex-math notation="LaTeX" id="ImEquation524"><![CDATA[$h_1$]]></tex-math></inline-formula> in Eq. (<xref ref-type="disp-formula" rid="ptx154-M61">61</xref>) through Eq. (<xref ref-type="disp-formula" rid="ptx154-M62">62</xref>). Fortunately, <inline-formula><tex-math notation="LaTeX" id="ImEquation525"><![CDATA[$h_1$]]></tex-math></inline-formula> can be obtained from the expectation value of the open Wilson line as in Eq. (<xref ref-type="disp-formula" rid="ptx154-M67">67</xref>); therefore we do not need to refer to explicit boundary data and everything is computable in terms of bulk theory. Here we have only considered to the next leading order in <inline-formula><tex-math notation="LaTeX" id="ImEquation526"><![CDATA[$1/c$]]></tex-math></inline-formula>, but it is natural to expect that the same is true for higher orders in <inline-formula><tex-math notation="LaTeX" id="ImEquation527"><![CDATA[$1/c$]]></tex-math></inline-formula> as well. For <inline-formula><tex-math notation="LaTeX" id="ImEquation528"><![CDATA[$N=3$]]></tex-math></inline-formula>, we fixed the <inline-formula><tex-math notation="LaTeX" id="ImEquation529"><![CDATA[$1/c$]]></tex-math></inline-formula> order of the other interaction parameter <inline-formula><tex-math notation="LaTeX" id="ImEquation530"><![CDATA[$c_3^{(1)}$]]></tex-math></inline-formula> such that the equality in Eq. (<xref ref-type="disp-formula" rid="ptx154-M110">110</xref>) is satisfied. Here the number <inline-formula><tex-math notation="LaTeX" id="ImEquation531"><![CDATA[$224/5$]]></tex-math></inline-formula> was borrowed from the W<inline-formula><tex-math notation="LaTeX" id="ImEquation532"><![CDATA[$_N$]]></tex-math></inline-formula> minimal model. However, we believe that there should be a way to determine <inline-formula><tex-math notation="LaTeX" id="ImEquation533"><![CDATA[$c_3$]]></tex-math></inline-formula> without referring to explicit boundary data, and it is an important open problem to find this out. We do not claim that our prescription is unique, and in fact a different one was adopted in Ref. [<xref ref-type="bibr" rid="B23">23</xref>] for <inline-formula><tex-math notation="LaTeX" id="ImEquation534"><![CDATA[$N=2$]]></tex-math></inline-formula>. It is easier to see the physical meaning in our regularization procedure, but their prescription seems to be convenient for actual computations of conformal blocks. In any case, it should be useful to understand the relation between different prescriptions.</p>
<p>In this paper, we have examined the duality of Ref. [<xref ref-type="bibr" rid="B11">11</xref>] in the semiclassical limit discussed in Refs. [<xref ref-type="bibr" rid="B13">13</xref>&#x2013;<xref ref-type="bibr" rid="B15">15</xref>] with <inline-formula><tex-math notation="LaTeX" id="ImEquation535"><![CDATA[$1/c$]]></tex-math></inline-formula> corrections, but it is also possible to extend the analysis to other examples. In particular, an <inline-formula><tex-math notation="LaTeX" id="ImEquation536"><![CDATA[$\mathcal{N}=2$]]></tex-math></inline-formula> supersymmetric version of duality was proposed in Ref. [<xref ref-type="bibr" rid="B42">42</xref>], and the bulk description of its semiclassical limit was argued to be given by sl<inline-formula><tex-math notation="LaTeX" id="ImEquation537"><![CDATA[$(N+1|N)$]]></tex-math></inline-formula> Chern&#x2013;Simons gauge theory [<xref ref-type="bibr" rid="B43">43</xref>]. See Refs. [<xref ref-type="bibr" rid="B44">44</xref>&#x2013;<xref ref-type="bibr" rid="B48">48</xref>] for conical defect or black hole solutions in higher-spin supergravity. We think that supersymmetric extension is important for the following two reasons. Firstly, it is usually expected that supersymmetry suppresses quantum effects, and it would enable us to examine higher-order corrections in <inline-formula><tex-math notation="LaTeX" id="ImEquation538"><![CDATA[$1/c$]]></tex-math></inline-formula> systematically. Secondly, supersymmetry helps us to study relations between higher-spin gauge theory and superstring theory, and concrete examples have been discussed in Refs. [<xref ref-type="bibr" rid="B4">4</xref>,<xref ref-type="bibr" rid="B49">49</xref>,<xref ref-type="bibr" rid="B50">50</xref>] with <inline-formula><tex-math notation="LaTeX" id="ImEquation539"><![CDATA[$\mathcal{N}=3$]]></tex-math></inline-formula> supersymmetry and in Refs. [<xref ref-type="bibr" rid="B51">51</xref>,<xref ref-type="bibr" rid="B52">52</xref>] with <inline-formula><tex-math notation="LaTeX" id="ImEquation540"><![CDATA[$\mathcal{N}=4$]]></tex-math></inline-formula> supersymmetry. We would like to report on this extension in the near future.</p>
</sec>
</body>
<back>
<ack>
<title>Acknowledgments</title>
<p>We are grateful to Andrea Campoleoni, Pawel Caputa, Nilay Kundu, Takahiro Nishinaka, Volker Schomerus, Yuji Sugawara, Tadashi Takayanagi, and J&#x00F6;rg Teschner for useful discussions. Y.H. would like to thank the organizers of the &#x201C;Universit&#x00E4;t Hamburg&#x2013;Kyoto University Symposium&#x201D; and the workshop &#x201C;New ideas on higher spin gravity and holography&#x201D; at Kyung Hee University, Seoul for their hospitality. The work of Y.H. is supported by JSPS KAKENHI Grant Number 16H02182.</p>
</ack>
<sec><title>Funding</title>
<p>Open Access funding: SCOAP<inline-formula><tex-math notation="LaTeX" id="ImEquation541"><![CDATA[$^3$]]></tex-math></inline-formula>.</p>
</sec>
<fn-group>
<title>Footnotes</title>
<fn id="FN1"><p><sup>1</sup> After completing this paper, we become aware of an interesting paper [<xref ref-type="bibr" rid="B2">2</xref>] appearing in the arXiv. The paper deals with loop corrections in two-point Witten diagrams for higher-spin theories on AdS<inline-formula><tex-math notation="LaTeX" id="ImEquation542"><![CDATA[$_d$]]></tex-math></inline-formula>. Related previous works may be found in Refs. [<xref ref-type="bibr" rid="B3">3</xref>&#x2013;<xref ref-type="bibr" rid="B10">10</xref>].</p></fn>
<fn id="FN2"><p><sup>2</sup> The analysis of this paper will not rely on unitarity, so we can safely work in the non-unitary regime. However, we may have to make use of unitarity for other purposes, and in that case we should come back to the &#x2019;t Hooft limit, for instance, by utilizing the analytic continuation discussed in Ref. [<xref ref-type="bibr" rid="B14">14</xref>].</p></fn>
<fn id="FN3"><p><sup>3</sup> Previously, Wilson lines in <inline-formula><tex-math notation="LaTeX" id="ImEquation543"><![CDATA[$\text{sl}(N) $]]></tex-math></inline-formula> Chern&#x2013;Simons gauge theory were utilized to compute entanglement entropy in a holographic way [<xref ref-type="bibr" rid="B17">17</xref>,<xref ref-type="bibr" rid="B18">18</xref>]. For the case with <inline-formula><tex-math notation="LaTeX" id="ImEquation544"><![CDATA[$N=2$]]></tex-math></inline-formula>, the proposal reduces to that in Refs. [<xref ref-type="bibr" rid="B19">19</xref>,<xref ref-type="bibr" rid="B20">20</xref>].</p></fn>
<fn id="FN4"><p><sup>4</sup> One may find the expression of sl<inline-formula><tex-math notation="LaTeX" id="ImEquation545"><![CDATA[$(3)$]]></tex-math></inline-formula> generators for generic representation in terms of three parameters <inline-formula><tex-math notation="LaTeX" id="ImEquation546"><![CDATA[$x_1,x_2,x_3$]]></tex-math></inline-formula>, e.g., in Sect. 15.7.4 of Ref. [<xref ref-type="bibr" rid="B41">41</xref>].</p></fn>
</fn-group>
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