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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/pty025</article-id>
<article-id pub-id-type="publisher-id">pty025</article-id>
<article-id pub-id-type="arxiv">arXiv:1710.08853</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/B10</subject>
<subject>PTEP/B16</subject>
</subj-group>
</article-categories>
<title-group>
<article-title>Orbifold Schur index and IR formula</article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author" corresp="yes">
<name><surname>Imamura</surname><given-names>Yosuke</given-names></name>
<xref ref-type="aff" rid="AFF1"/>
<xref ref-type="corresp" rid="COR1"/>
<email xlink:type="simple">imamura@phys.titech.ac.jp</email>
</contrib>
</contrib-group>
<aff id="AFF1"><italic>Department of Physics, Tokyo Institute of Technology, Tokyo 152-8551, Japan</italic></aff>
<author-notes>
<corresp id="COR1">E-mail: <email>imamura@phys.titech.ac.jp</email></corresp>
</author-notes>
<pub-date pub-type="cover">
<month>04</month>
<year>2018</year>
</pub-date>
<pub-date pub-type="collection">
<day>01</day>
<month>04</month>
<year>2018</year>
</pub-date>
<pub-date pub-type="epub" iso-8601-date="2018-04-10">
<day>10</day>
<month>04</month>
<year>2018</year>
</pub-date>
<volume>2018</volume>
<issue>4</issue>
<elocation-id>043B01</elocation-id>
<history>
<date date-type="received">
<day>21</day>
<month>11</month>
<year>2017</year>
</date>
<date date-type="rev-recd">
<day>05</day>
<month>02</month>
<year>2018</year>
</date>
<date date-type="accepted">
<day>09</day>
<month>02</month>
<year>2018</year>
</date>
</history>
<permissions>
<copyright-statement>&#x000A9; The Author 2018. Published by Oxford University Press on behalf of the Physical Society of Japan.</copyright-statement>
<copyright-year>2018</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="pty025.pdf"/>
<abstract abstract-type="abstract"><title>Abstract</title>
<p>We discuss an orbifold version of the Schur index defined as the supersymmetric partition function in <inline-formula><tex-math notation="LaTeX" id="ImEquation1"><![CDATA[$\boldsymbol{S}^3/{\mathbb{Z}}_n\times\boldsymbol{S}^1$]]></tex-math></inline-formula>. We first give a general formula for Lagrangian theories obtained by the localization technique, and then suggest a generalization of the Cordova and Shao IR formula. We confirm that the generalized IR formula gives the correct answer for systems with free hypermultiplets if we tune the background fields so that they are invariant under the orbifold action. Unfortunately, we find disagreement for theories with dynamical vector multiplets.</p>
</abstract>
<kwd-group kwd-group-type="jel">
<kwd>B10</kwd>
<kwd>B16</kwd>
</kwd-group>
<counts>
<page-count count="12"/>
</counts>
</article-meta>
</front>
<body>
<sec sec-type="intro" id="SEC1"><title>1. Introduction</title>
<p>Exactly calculable quantities in supersymmetric field theories play important roles in recent progress in quantum field theories. The Schur index of <inline-formula><tex-math notation="LaTeX" id="ImEquation2"><![CDATA[${\cal N}=2$]]></tex-math></inline-formula> superconformal field theories is one such quantity. There are different ways to calculate the index.</p>
<p>The Schur index is a specialization of the superconformal index of <inline-formula><tex-math notation="LaTeX" id="ImEquation3"><![CDATA[${\cal N}=1$]]></tex-math></inline-formula> superconformal field theories [<xref ref-type="bibr" rid="B1">1</xref>,<xref ref-type="bibr" rid="B2">2</xref>]. (See Ref. [<xref ref-type="bibr" rid="B3">3</xref>] for various limits of the superconformal index.) The superconformal index can be regarded as the supersymmetric partition function in <inline-formula><tex-math notation="LaTeX" id="ImEquation4"><![CDATA[$\boldsymbol{S}^3\times\boldsymbol{S}^1$]]></tex-math></inline-formula>. For Lagrangian theories it is defined as the path integral in the background, and we can reduce it as a finite-dimensional integral by using the localization method. This is also available for a non-Lagrangian theory if we know a UV Lagrangian theory that flows to the theory.</p>
<p>Cordova and Shao [<xref ref-type="bibr" rid="B4">4</xref>] proposed an interesting formula for the Schur index which gives the index as the trace of a so-called quantum monodromy operator. With this formula we can calculate the index from the information of the BPS spectrum of the theory in the Coulomb branch. Although the BPS spectrum depends on the Coulomb moduli parameters and jumps on walls of marginal stability the quantum monodromy operator is wall-crossing invariant, and so is the index. The formula is generalized to decorated indices by introducing defect operators [<xref ref-type="bibr" rid="B5">5</xref>&#x2013;<xref ref-type="bibr" rid="B7">7</xref>].</p>
<p>For class S theories, which are realized on M5-branes wrapped on Riemann surfaces, the Schur index is expressed as a correlation function of a two-dimensional topological field theory on the associated Riemann surface [<xref ref-type="bibr" rid="B8">8</xref>&#x2013;<xref ref-type="bibr" rid="B14">14</xref>].</p>
<p>The Schur index receives contributions of a special class of gauge-invariant operators, which are called Schur operators. Beem et al. [<xref ref-type="bibr" rid="B15">15</xref>] show that the set of Schur operators form a chiral algebra of two-dimensional conformal field theory (CFT). Once we identify the chiral algebra associated with a four-dimensional theory the Schur index is obtained as the vacuum character of the chiral algebra. The characters of other modules are also important and are related to line and surface operator insertions [<xref ref-type="bibr" rid="B7">7</xref>,<xref ref-type="bibr" rid="B16">16</xref>]. For theories of class S there is a prescription to obtain the corresponding chiral algebra [<xref ref-type="bibr" rid="B17">17</xref>].</p>
<p>The purpose of this paper is investigate a generalization of the Schur index defined by replacing the background manifold <inline-formula><tex-math notation="LaTeX" id="ImEquation5"><![CDATA[$\boldsymbol{S}^3\times\boldsymbol{S}^1$]]></tex-math></inline-formula> with its orbifold <inline-formula><tex-math notation="LaTeX" id="ImEquation6"><![CDATA[$\boldsymbol{S}^3/{\mathbb{Z}}_n\times\boldsymbol{S}^1$]]></tex-math></inline-formula>. Such an orbifold generalization for the superconformal index of <inline-formula><tex-math notation="LaTeX" id="ImEquation7"><![CDATA[${\cal N}=1$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation8"><![CDATA[${\cal N}=2$]]></tex-math></inline-formula> theories has already been investigated in Refs. [<xref ref-type="bibr" rid="B18">18</xref>&#x2013;<xref ref-type="bibr" rid="B22">22</xref>]. The index is defined in Ref. [<xref ref-type="bibr" rid="B18">18</xref>] by using <inline-formula><tex-math notation="LaTeX" id="ImEquation9"><![CDATA[${\mathbb{Z}}_n$]]></tex-math></inline-formula>, which preserves a supercharge of a specific chirality. Because we need only one supercharge (and its Hermitian conjugate) for the definition of the superconformal index, this orbifolding is consistent with the definition of the index. However, in the case of the Schur index, we need to preserve two supercharges with opposite chirality (and their Hermitian conjugates). Therefore, we need to modify the definition of the orbifold index by introducing an extra <inline-formula><tex-math notation="LaTeX" id="ImEquation10"><![CDATA[$SU(2)_R\times U(1)_r$]]></tex-math></inline-formula> twist. The application of the localization technique for the orbifold Schur index is straightforward and will be shown in <xref ref-type="sec" rid="SEC2">Sect. 2</xref>. Then, we discuss a generalization of the IR formula to the orbifold case. We suggest a natural generalization of Cordova and Shao&#x2019;s formula based on a physical interpretation of the formula, and apply it to some simple examples. For systems consisting of free hypermultiplets we find agreement of the UV and IR formulae. Unfortunately, however, for more general systems including dynamical vector multiplets the suggested formula does not give the desired results.</p>
</sec>
<sec id="SEC2"><title>2. UV formula</title>
<p>Let us consider an <inline-formula><tex-math notation="LaTeX" id="ImEquation11"><![CDATA[${\cal N}=2$]]></tex-math></inline-formula> superconformal field theory defined in <inline-formula><tex-math notation="LaTeX" id="ImEquation12"><![CDATA[$\boldsymbol{S}^3\times{\mathbb{R}}_t$]]></tex-math></inline-formula>. Let <inline-formula><tex-math notation="LaTeX" id="ImEquation13"><![CDATA[$H$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation14"><![CDATA[$J$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation15"><![CDATA[$\overline J$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation16"><![CDATA[$R$]]></tex-math></inline-formula>, and <inline-formula><tex-math notation="LaTeX" id="ImEquation17"><![CDATA[$r$]]></tex-math></inline-formula> be the Hamiltonian, the third component of the left-handed spin, that of the right-handed spin, the <inline-formula><tex-math notation="LaTeX" id="ImEquation18"><![CDATA[$SU(2)_R$]]></tex-math></inline-formula> Cartan generator, and the <inline-formula><tex-math notation="LaTeX" id="ImEquation19"><![CDATA[$U(1)_r$]]></tex-math></inline-formula> charge, respectively. The superconformal index is defined by
<disp-formula id="pty025-M1"><label>(1)</label><tex-math notation="LaTeX" id="Equation1"><![CDATA[
\begin{align}
I(p,q,t,\vec z_F)={\rm Tr}\left[e^{2\pi i(J+\overline J)}
x^{\mu_x}
p^{\mu_p}
q^{\mu_q}
t^{\mu_t}
\vec z_F^{\vec T_F}
\right]\!,
\label{defsci}
\end{align}
]]></tex-math></disp-formula>
where the trace is taken over all gauge-invariant states in <inline-formula><tex-math notation="LaTeX" id="ImEquation20"><![CDATA[$\boldsymbol{S}^3$]]></tex-math></inline-formula>. We denote the set of Cartan generators of the flavor group <inline-formula><tex-math notation="LaTeX" id="ImEquation21"><![CDATA[$F$]]></tex-math></inline-formula> by <inline-formula><tex-math notation="LaTeX" id="ImEquation22"><![CDATA[$\vec T_F=(T_{F,1},\ldots,T_{F,r_F})$]]></tex-math></inline-formula>. Other Cartan generators are defined by
<disp-formula id="pty025-M2"><label>(2)</label><tex-math notation="LaTeX" id="Equation2"><![CDATA[
\begin{align}
\mu_x&
=\frac{1}{2}H-J-R+\frac{1}{4}r
=\{Q,Q^\dagger\}
,\\
\end{align}
]]></tex-math></disp-formula>
<disp-formula id="pty025-M3"><label>(3)</label><tex-math notation="LaTeX" id="Equation3"><![CDATA[
\begin{align}
\mu_p&
=\frac{1}{2}H-\overline J-R-\frac{1}{4}r
=\{\overline Q,\overline Q^\dagger\}
,\\
\end{align}
]]></tex-math></disp-formula>
<disp-formula id="pty025-M4"><label>(4)</label><tex-math notation="LaTeX" id="Equation4"><![CDATA[
\begin{align}
\mu_q&=J+\overline J+R,\\
\end{align}
]]></tex-math></disp-formula>
<disp-formula id="pty025-M5"><label>(5)</label><tex-math notation="LaTeX" id="Equation5"><![CDATA[
\begin{align}
\mu_t&=R+\frac{1}{2}r,
\label{danddbar}
\end{align}
]]></tex-math></disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation23"><![CDATA[$Q$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation24"><![CDATA[$\overline Q$]]></tex-math></inline-formula> are supercharges with the following quantum numbers:
<disp-formula id="pty025-M6"><label>(6)</label><tex-math notation="LaTeX" id="Equation6"><![CDATA[
\begin{align}
Q:(H,J,\overline J,R,r)&=(\tfrac{1}{2},-\tfrac{1}{2},0,+\tfrac{1}{2},-1),\nonumber\\
\overline Q:(H,J,\overline J,R,r)&=(\tfrac{1}{2},0,-\tfrac{1}{2},+\tfrac{1}{2},+1).
\end{align}
]]></tex-math></disp-formula></p>
<p>The definition in Eq. (<xref ref-type="disp-formula" rid="pty025-M1">1</xref>) respects <inline-formula><tex-math notation="LaTeX" id="ImEquation25"><![CDATA[$Q$]]></tex-math></inline-formula>. Namely, all the Cartan generators used in Eq. (<xref ref-type="disp-formula" rid="pty025-M1">1</xref>) commute with <inline-formula><tex-math notation="LaTeX" id="ImEquation26"><![CDATA[$Q$]]></tex-math></inline-formula>. Because <inline-formula><tex-math notation="LaTeX" id="ImEquation27"><![CDATA[$\mu_x$]]></tex-math></inline-formula> is <inline-formula><tex-math notation="LaTeX" id="ImEquation28"><![CDATA[$Q$]]></tex-math></inline-formula>-exact, the index in Eq. (<xref ref-type="disp-formula" rid="pty025-M1">1</xref>) is independent of <inline-formula><tex-math notation="LaTeX" id="ImEquation29"><![CDATA[$x$]]></tex-math></inline-formula>.<xref ref-type="fn" rid="FN1"><sup>1</sup></xref></p>
<p>The superconformal index can be regarded as the supersymmetric partition function in <inline-formula><tex-math notation="LaTeX" id="ImEquation30"><![CDATA[$\boldsymbol{S}^3\times\boldsymbol{S}^1$]]></tex-math></inline-formula>. If the theory has a Lagrangian description with gauge group <inline-formula><tex-math notation="LaTeX" id="ImEquation31"><![CDATA[$G$]]></tex-math></inline-formula> we can define the index as the path integral. By using the localization technique we can reduce the path integral to the finite-dimensional integral
<disp-formula id="pty025-M7"><label>(7)</label><tex-math notation="LaTeX" id="Equation7"><![CDATA[
\begin{align}
I=\int d\mu \,{\rm Pexp}\,i, \label{ioint}
\end{align}
]]></tex-math></disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation32"><![CDATA[${\rm Pexp}$]]></tex-math></inline-formula> is the plethystic exponential defined by
<disp-formula id="pty025-M8"><label>(8)</label><tex-math notation="LaTeX" id="Equation8"><![CDATA[
\begin{align}
{\rm Pexp} f(x_1,x_2,\ldots,x_k)
=\exp\sum_{m=1}^\infty\frac{1}{m} f(x_1^m,x_2^m,\ldots,x_k^m).
\end{align}
]]></tex-math></disp-formula></p>
<p><inline-formula><tex-math notation="LaTeX" id="ImEquation33"><![CDATA[$i$]]></tex-math></inline-formula> is the one-particle index defined by
<disp-formula id="pty025-M9"><label>(9)</label><tex-math notation="LaTeX" id="Equation9"><![CDATA[
\begin{align}
i(p,q,t,\vec z)={\rm tr}\left[e^{2\pi i(J+\overline J)}
x^{\mu_x}
p^{\mu_p}
q^{\mu_q}
t^{\mu_t}
\vec z^{\vec T}
\right]\!,
\label{defopi}
\end{align}
]]></tex-math></disp-formula>
where the trace is taken over all one-particle states including gauge-non-invariant states. <inline-formula><tex-math notation="LaTeX" id="ImEquation34"><![CDATA[$\vec T$]]></tex-math></inline-formula> includes both flavor and gauge Cartan generators, and <inline-formula><tex-math notation="LaTeX" id="ImEquation35"><![CDATA[$\vec z$]]></tex-math></inline-formula> is the set of the corresponding fugacities. Namely, <inline-formula><tex-math notation="LaTeX" id="ImEquation36"><![CDATA[$\vec z^{\vec T}=\vec z_F^{\vec T_F}\vec z_G^{\vec T_G}$]]></tex-math></inline-formula>. <inline-formula><tex-math notation="LaTeX" id="ImEquation37"><![CDATA[$\int d\mu$]]></tex-math></inline-formula> is the integral over the gauge fugacities,
<disp-formula id="pty025-M10"><label>(10)</label><tex-math notation="LaTeX" id="Equation10"><![CDATA[
\begin{align}
\int d\mu=\frac{1}{|W_G|}\prod_{i=1}^{r_G}\oint\frac{dz_{G,i}}{2\pi iz_{G,i}},
\end{align}
]]></tex-math></disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation38"><![CDATA[$|W_G|$]]></tex-math></inline-formula> is the size of the Weyl group of <inline-formula><tex-math notation="LaTeX" id="ImEquation39"><![CDATA[$G$]]></tex-math></inline-formula>.</p>
<p>The Schur index is obtained from the superconformal index by the specialization <inline-formula><tex-math notation="LaTeX" id="ImEquation40"><![CDATA[$t=1$]]></tex-math></inline-formula>. Then <inline-formula><tex-math notation="LaTeX" id="ImEquation41"><![CDATA[$\mu_t$]]></tex-math></inline-formula> disappears from Eq. (<xref ref-type="disp-formula" rid="pty025-M5">5</xref>), and all the remaining Cartan charges commute with not only <inline-formula><tex-math notation="LaTeX" id="ImEquation42"><![CDATA[$Q$]]></tex-math></inline-formula> but also <inline-formula><tex-math notation="LaTeX" id="ImEquation43"><![CDATA[$\overline Q$]]></tex-math></inline-formula>. Therefore, the Schur index receives contributions of operators that carry <inline-formula><tex-math notation="LaTeX" id="ImEquation44"><![CDATA[$\mu_x=\mu_p=0$]]></tex-math></inline-formula>. Such operators are called Schur operators. As a result, the Schur index is a function of the superconformal fugacity <inline-formula><tex-math notation="LaTeX" id="ImEquation45"><![CDATA[$q$]]></tex-math></inline-formula> and the flavor fugacities <inline-formula><tex-math notation="LaTeX" id="ImEquation46"><![CDATA[$\vec z_F$]]></tex-math></inline-formula>.</p>
<p>There is another index that receives from the same set of operators as the Schur index. It is the Macdonald index defined from the superconformal index by taking the limit <inline-formula><tex-math notation="LaTeX" id="ImEquation47"><![CDATA[$p\rightarrow0$]]></tex-math></inline-formula>. We do not consider the Macdonald index here because its definition does not respect the supercharges <inline-formula><tex-math notation="LaTeX" id="ImEquation48"><![CDATA[$Q$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation49"><![CDATA[$\overline Q$]]></tex-math></inline-formula> that are important when we discuss the BPS configuration associated with the IR formula. Even so, the Macdonald index is closely related to the Schur index, and can be reproduced from the chiral algebra up to some ambiguity that can be fixed by using information from four-dimensional SCFT [<xref ref-type="bibr" rid="B23">23</xref>]. In the recent paper [<xref ref-type="bibr" rid="B24">24</xref>] an orbifold version of the Macdonald index is studied, and a close relation to the chiral algebra is observed. It will be important to study the relation between the orbifold Schur index defined below and the orbifold Macdonald index in Ref. [<xref ref-type="bibr" rid="B24">24</xref>].</p>
<p>The one-particle Schur index is given by
<disp-formula id="pty025-M11"><label>(11)</label><tex-math notation="LaTeX" id="Equation11"><![CDATA[
\begin{align}
i=r_Gi_{U(1)}+i_V+i_H,
\end{align}
]]></tex-math></disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation50"><![CDATA[$i_{U(1)}$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation51"><![CDATA[$i_V$]]></tex-math></inline-formula>, and <inline-formula><tex-math notation="LaTeX" id="ImEquation52"><![CDATA[$i_H$]]></tex-math></inline-formula> represent the contributions of a single <inline-formula><tex-math notation="LaTeX" id="ImEquation53"><![CDATA[$U(1)$]]></tex-math></inline-formula> vector multiplet, charged vector multiplets, and half-hypermultiplets, respectively. They are explicitly given as
<disp-formula id="pty025-M12"><label>(12)</label><tex-math notation="LaTeX" id="Equation12"><![CDATA[
\begin{align}
i_{U(1)}=\frac{-2q}{1-q},\quad i_V=-\frac{1+q}{1-q}\chi'_{\rm adj}(\vec z_G),\quad i_H=\frac{q^{\frac{1}{2}}}{1-q}\chi_{R_H}(\vec z_F,\vec z_G),
\label{eq11}
\end{align}
]]></tex-math></disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation54"><![CDATA[$\chi_{\rm adj}'\equiv\chi_{\rm adj}-r_G$]]></tex-math></inline-formula> is the character of the adjoint representation of <inline-formula><tex-math notation="LaTeX" id="ImEquation55"><![CDATA[$G$]]></tex-math></inline-formula> with the Cartan contribution subtracted, and <inline-formula><tex-math notation="LaTeX" id="ImEquation56"><![CDATA[$\chi_{R_H}$]]></tex-math></inline-formula> is the character of the <inline-formula><tex-math notation="LaTeX" id="ImEquation57"><![CDATA[$G\times F$]]></tex-math></inline-formula> representation of the half-hypermultiplets.<xref ref-type="fn" rid="FN2"><sup>2</sup></xref> Because <inline-formula><tex-math notation="LaTeX" id="ImEquation58"><![CDATA[$i_{U(1)}$]]></tex-math></inline-formula> does not depend on the gauge fugacities <inline-formula><tex-math notation="LaTeX" id="ImEquation59"><![CDATA[$\vec z_G$]]></tex-math></inline-formula> we can factor out the Cartan contribution in Eq. (<xref ref-type="disp-formula" rid="pty025-M7">7</xref>) as <inline-formula><tex-math notation="LaTeX" id="ImEquation60"><![CDATA[$\lambda^{r_G}$]]></tex-math></inline-formula>, with <inline-formula><tex-math notation="LaTeX" id="ImEquation61"><![CDATA[$\lambda$]]></tex-math></inline-formula> defined by
<disp-formula id="pty025-M13"><label>(13)</label><tex-math notation="LaTeX" id="Equation13"><![CDATA[
\begin{align}
\lambda= \,{\rm Pexp}\,i_{U(1)}=(q;q)_\infty^2,
\label{u1shur}
\end{align}
]]></tex-math></disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation62"><![CDATA[$(z;q)_\infty$]]></tex-math></inline-formula> is the <inline-formula><tex-math notation="LaTeX" id="ImEquation63"><![CDATA[$q$]]></tex-math></inline-formula>-Pochhammer symbol defined by
<disp-formula id="pty025-M14"><label>(14)</label><tex-math notation="LaTeX" id="Equation14"><![CDATA[
\begin{align}
(z;q)_\infty=\prod_{k=0}^\infty(1-zq^k).
\end{align}
]]></tex-math></disp-formula></p>
<p>A generalization of the superconformal index to the orbifold background <inline-formula><tex-math notation="LaTeX" id="ImEquation64"><![CDATA[$\boldsymbol{S}^3/{\mathbb{Z}}_n\times\boldsymbol{S}^1$]]></tex-math></inline-formula> was first investigated in Ref. [<xref ref-type="bibr" rid="B18">18</xref>]. They defined the orbifold with the discrete group <inline-formula><tex-math notation="LaTeX" id="ImEquation65"><![CDATA[${\mathbb{Z}}_n$]]></tex-math></inline-formula> generated by
<disp-formula id="pty025-M15"><label>(15)</label><tex-math notation="LaTeX" id="Equation15"><![CDATA[
\begin{align}
\overline g_n=\omega_n^{2\overline J},\quad
\omega_n\equiv e^{\frac{2\pi i}{n}}\!.
\end{align}
]]></tex-math></disp-formula></p>
<p>This is consistent with the definition in Eq. (<xref ref-type="disp-formula" rid="pty025-M1">1</xref>) of the superconformal index in the sense that <inline-formula><tex-math notation="LaTeX" id="ImEquation66"><![CDATA[$\overline g_n$]]></tex-math></inline-formula> commutes with the supercharge <inline-formula><tex-math notation="LaTeX" id="ImEquation67"><![CDATA[$Q$]]></tex-math></inline-formula>. If the theory has gauge and/or flavor symmetry we can turn on holonomies <inline-formula><tex-math notation="LaTeX" id="ImEquation68"><![CDATA[$\vec h$]]></tex-math></inline-formula> by using <inline-formula><tex-math notation="LaTeX" id="ImEquation69"><![CDATA[$\overline g_n\omega_n^{\vec h\vec T}$]]></tex-math></inline-formula> instead of <inline-formula><tex-math notation="LaTeX" id="ImEquation70"><![CDATA[$\overline g_n$]]></tex-math></inline-formula> as the <inline-formula><tex-math notation="LaTeX" id="ImEquation71"><![CDATA[${\mathbb{Z}}_n$]]></tex-math></inline-formula> generator. Once we choose the <inline-formula><tex-math notation="LaTeX" id="ImEquation72"><![CDATA[${\mathbb{Z}}_n$]]></tex-math></inline-formula> generator, it is straightforward to generalize the formula in Eq. (<xref ref-type="disp-formula" rid="pty025-M7">7</xref>) to the orbifold case. What we have to do first is project away the contribution of <inline-formula><tex-math notation="LaTeX" id="ImEquation73"><![CDATA[${\mathbb{Z}}_n$]]></tex-math></inline-formula> non-invariant states from the one-particle index in Eq. (<xref ref-type="disp-formula" rid="pty025-M9">9</xref>). This projection is carried out by inserting the projection
<disp-formula id="pty025-M16"><label>(16)</label><tex-math notation="LaTeX" id="Equation16"><![CDATA[
\begin{align}
\frac{1}{n}\sum_{k=0}^{n-1}(\overline g_n\omega_n^{\vec h\vec T})^k
\end{align}
]]></tex-math></disp-formula>
into the trace in Eq. (<xref ref-type="disp-formula" rid="pty025-M9">9</xref>). Because <inline-formula><tex-math notation="LaTeX" id="ImEquation74"><![CDATA[$\overline g_n$]]></tex-math></inline-formula> can be expressed in terms of the Cartan generators appearing in Eq. (<xref ref-type="disp-formula" rid="pty025-M1">1</xref>) as <inline-formula><tex-math notation="LaTeX" id="ImEquation75"><![CDATA[$\overline g_n=\omega_n^{2\overline J}=\omega_n^{\mu_x-\mu_p+\mu_q-\mu_t}$]]></tex-math></inline-formula>, insertion of <inline-formula><tex-math notation="LaTeX" id="ImEquation76"><![CDATA[$(\overline g_n\omega_n^{\vec h\vec T})^k$]]></tex-math></inline-formula> is equivalent to the replacement of the fugacities
<disp-formula id="pty025-M17"><label>(17)</label><tex-math notation="LaTeX" id="Equation17"><![CDATA[
\begin{align}
(x,p,q,t,\vec z)\rightarrow
(\omega_n^kx,\omega_n^{-k}p,\omega_n^kq,\omega_n^{-k}t,\omega_n^{k\vec h}\vec z),
\label{vartor}
\end{align}
]]></tex-math></disp-formula>
and the one-particle index for the <inline-formula><tex-math notation="LaTeX" id="ImEquation77"><![CDATA[${\mathbb{Z}}_n$]]></tex-math></inline-formula> orbifold is
<disp-formula id="pty025-M18"><label>(18)</label><tex-math notation="LaTeX" id="Equation18"><![CDATA[
\begin{align}
i_n^{\vec h}(p,q,t,\vec z)=
\frac{1}{n}\sum_{k=0}^{n-1}
i(\omega_n^{-k}p,\omega_n^kq,\omega_n^{-k}t,\omega_n^{k\vec h}\vec z).
\end{align}
]]></tex-math></disp-formula></p>
<p>By using this orbifold one-particle index, the orbifold index is given by
<disp-formula id="pty025-M19"><label>(19)</label><tex-math notation="LaTeX" id="Equation19"><![CDATA[
\begin{align}
I_n^{\vec h_F}=\sum_{\vec h_G} e^{\varepsilon(\vec h)}\int d\mu\,{\rm Pexp}\,i_n^{\vec h},
\label{inh}
\end{align}
]]></tex-math></disp-formula>
where the factor <inline-formula><tex-math notation="LaTeX" id="ImEquation78"><![CDATA[$e^{\varepsilon(\vec h)}$]]></tex-math></inline-formula> is the contribution of the zero-point energy. For the ordinary index this factor just gives an overall factor and is usually neglected. However, in the orbifold case this factor is important because it depends on the gauge holonomy <inline-formula><tex-math notation="LaTeX" id="ImEquation79"><![CDATA[$\vec h_G$]]></tex-math></inline-formula>. The zero-point factor <inline-formula><tex-math notation="LaTeX" id="ImEquation80"><![CDATA[$e^{\varepsilon(\vec h)}$]]></tex-math></inline-formula> is easily obtained by taking the product of all contributions of one-particle states. For example, if the one-particle index is expanded as <inline-formula><tex-math notation="LaTeX" id="ImEquation81"><![CDATA[$i_n^{\vec h}=\sum_ic_ip^{a_i}q^{b_i}(\cdots)$]]></tex-math></inline-formula> (we explicitly show <inline-formula><tex-math notation="LaTeX" id="ImEquation82"><![CDATA[$p$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation83"><![CDATA[$q$]]></tex-math></inline-formula> dependence for simplicity, and the dots include other fugacities) then the corresponding zero-point factor is given by <inline-formula><tex-math notation="LaTeX" id="ImEquation84"><![CDATA[$e^{\varepsilon(\vec h)}=\prod_i(p^{\frac{a_i}{2}}q^{\frac{b_i}{2}}\cdots)^{c_i}$]]></tex-math></inline-formula>. Although this infinite product is usually divergent, we can obtain a finite result by using an appropriate regularization such as <inline-formula><tex-math notation="LaTeX" id="ImEquation85"><![CDATA[$\zeta$]]></tex-math></inline-formula>-function regularization.</p>
<p>Now, let us apply the same orbifolding prescription to the Schur index. We cannot obtain the orbifold Schur index by the specialization <inline-formula><tex-math notation="LaTeX" id="ImEquation86"><![CDATA[$t\rightarrow 1$]]></tex-math></inline-formula> from the orbifold superconformal index above because this contradicts the orbifold action in Eq. (<xref ref-type="disp-formula" rid="pty025-M17">17</xref>). For consistency with <inline-formula><tex-math notation="LaTeX" id="ImEquation87"><![CDATA[$t=1$]]></tex-math></inline-formula> we use
<disp-formula id="pty025-M20"><label>(20)</label><tex-math notation="LaTeX" id="Equation20"><![CDATA[
\begin{align}
g_n=
\overline g_n e^{\frac{2\pi i}{n}(R+\frac{1}{2}r)}
=e^{\frac{2\pi i}{n}(\mu_x-\mu_p+\mu_q)}
\label{gdef}
\end{align}
]]></tex-math></disp-formula>
instead of <inline-formula><tex-math notation="LaTeX" id="ImEquation88"><![CDATA[$\overline g_n$]]></tex-math></inline-formula>. Namely, we combine <inline-formula><tex-math notation="LaTeX" id="ImEquation89"><![CDATA[$\overline g_n$]]></tex-math></inline-formula> with the additional <inline-formula><tex-math notation="LaTeX" id="ImEquation90"><![CDATA[$SU(2)_R\times U(1)$]]></tex-math></inline-formula> twist to keep both <inline-formula><tex-math notation="LaTeX" id="ImEquation91"><![CDATA[$Q$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation92"><![CDATA[$\overline Q$]]></tex-math></inline-formula> invariant. Again, we can turn on holonomies <inline-formula><tex-math notation="LaTeX" id="ImEquation93"><![CDATA[$\vec h$]]></tex-math></inline-formula>, and the insertion of <inline-formula><tex-math notation="LaTeX" id="ImEquation94"><![CDATA[$(g_n\omega_n^{\vec h\vec T})^k$]]></tex-math></inline-formula> is equivalent to the replacement
<disp-formula id="pty025-M21"><label>(21)</label><tex-math notation="LaTeX" id="Equation21"><![CDATA[
\begin{align}
(x,p,q,\vec z)
\rightarrow(\omega_n^k x,\omega_n^{-k}p,\omega_n^k q,\omega_n^{k\vec h}\vec z).
\end{align}
]]></tex-math></disp-formula></p>
<p>Therefore, the orbifold one-particle index is
<disp-formula id="pty025-M22"><label>(22)</label><tex-math notation="LaTeX" id="Equation22"><![CDATA[
\begin{align}
i_n^{\vec h}(q,\vec z)=\frac{1}{n}\sum_{k=0}^{n-1}i(\omega^kq,\omega^{k\vec h}\vec z).
\end{align}
]]></tex-math></disp-formula></p>
<p>With this one-particle index we can calculate the orbifold Schur index of Lagrangian theories by using Eq. (<xref ref-type="disp-formula" rid="pty025-M19">19</xref>), which we call the UV formula in the following.</p>
<p>Before discussing the IR formula for the orbifold Schur index, let us apply the UV formula to some simple systems. In the following examples the zero-point factors give overall factors independent of the holonomies and we omit them.</p>
<sec id="SEC2.1"><title>2.1. <inline-formula><tex-math notation="LaTeX" id="ImEquation95"><![CDATA[$U(1)$]]></tex-math></inline-formula> vector multiplet</title>
<p>The <inline-formula><tex-math notation="LaTeX" id="ImEquation96"><![CDATA[$U(1)$]]></tex-math></inline-formula> contribution in <inline-formula><tex-math notation="LaTeX" id="ImEquation97"><![CDATA[$\boldsymbol{S}^3$]]></tex-math></inline-formula> is given by <inline-formula><tex-math notation="LaTeX" id="ImEquation98"><![CDATA[$\lambda$]]></tex-math></inline-formula> in Eq. (<xref ref-type="disp-formula" rid="pty025-M13">13</xref>). The <inline-formula><tex-math notation="LaTeX" id="ImEquation99"><![CDATA[${\mathbb{Z}}_n$]]></tex-math></inline-formula> action is simple phase rotation of variable <inline-formula><tex-math notation="LaTeX" id="ImEquation100"><![CDATA[$q$]]></tex-math></inline-formula>, and we obtain the orbifold one-particle index <inline-formula><tex-math notation="LaTeX" id="ImEquation101"><![CDATA[$i_n=-2q^n/(1-q^n)$]]></tex-math></inline-formula>. The orbifold Schur index is
<disp-formula id="pty025-M23"><label>(23)</label><tex-math notation="LaTeX" id="Equation23"><![CDATA[
\begin{align}
\lambda_n=
{\rm Pexp}\left(\frac{-2q^n}{1-q^n}\right)=(q^n;q^n)_\infty^2.
\label{lambdan}
\end{align}
]]></tex-math></disp-formula></p>
</sec>
<sec id="SEC2.2"><title>2.2. Free hypermultiplet</title>
<p>Let us consider the system of a single free hypermultiplet <inline-formula><tex-math notation="LaTeX" id="ImEquation102"><![CDATA[$(q,\widetilde q)$]]></tex-math></inline-formula>. This has <inline-formula><tex-math notation="LaTeX" id="ImEquation103"><![CDATA[$SU(2)_F$]]></tex-math></inline-formula> flavor symmetry. Let <inline-formula><tex-math notation="LaTeX" id="ImEquation104"><![CDATA[$z$]]></tex-math></inline-formula> be the fugacity for <inline-formula><tex-math notation="LaTeX" id="ImEquation105"><![CDATA[$U(1)_F\subset SU(2)_F$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation106"><![CDATA[$F$]]></tex-math></inline-formula> be the corresponding generator such that <inline-formula><tex-math notation="LaTeX" id="ImEquation107"><![CDATA[$q$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation108"><![CDATA[$\widetilde q$]]></tex-math></inline-formula> carry <inline-formula><tex-math notation="LaTeX" id="ImEquation109"><![CDATA[$F=+1$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation110"><![CDATA[$-1$]]></tex-math></inline-formula>, respectively. The one-particle index before <inline-formula><tex-math notation="LaTeX" id="ImEquation111"><![CDATA[${\mathbb{Z}}_n$]]></tex-math></inline-formula> projection is
<disp-formula id="pty025-M24"><label>(24)</label><tex-math notation="LaTeX" id="Equation24"><![CDATA[
\begin{align}
i(q,z)=\frac{q^{\frac{1}{2}}}{1-q}(z+z^{-1}).
\end{align}
]]></tex-math></disp-formula></p>
<p>The <inline-formula><tex-math notation="LaTeX" id="ImEquation112"><![CDATA[${\mathbb{Z}}_n$]]></tex-math></inline-formula> generator acts on the variables as
<disp-formula id="pty025-M25"><label>(25)</label><tex-math notation="LaTeX" id="Equation25"><![CDATA[
\begin{align}
g_n\omega_n^{hF}:(q,z)\rightarrow(\omega_n q,\omega_n^hz).
\end{align}
]]></tex-math></disp-formula></p>
<p>By definition, the generator <inline-formula><tex-math notation="LaTeX" id="ImEquation113"><![CDATA[$g_n\omega_n^{hF}$]]></tex-math></inline-formula> must satisfy <inline-formula><tex-math notation="LaTeX" id="ImEquation114"><![CDATA[$(g_n\omega_n^{hF})^n=1$]]></tex-math></inline-formula> (otherwise the fiber bundle associated with the fields is ill-defined). Due to the fractional <inline-formula><tex-math notation="LaTeX" id="ImEquation115"><![CDATA[$SU(2)_R$]]></tex-math></inline-formula> charge <inline-formula><tex-math notation="LaTeX" id="ImEquation116"><![CDATA[$R=-1/2$]]></tex-math></inline-formula> of <inline-formula><tex-math notation="LaTeX" id="ImEquation117"><![CDATA[$q$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation118"><![CDATA[$\widetilde q$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation119"><![CDATA[$g_n^n$]]></tex-math></inline-formula> acts on the hypermultiplet as <inline-formula><tex-math notation="LaTeX" id="ImEquation120"><![CDATA[$-1$]]></tex-math></inline-formula>. To compensate for this, we need to take the fractional holonomy <inline-formula><tex-math notation="LaTeX" id="ImEquation121"><![CDATA[$h\in{\mathbb{Z}}+\frac{1}{2}$]]></tex-math></inline-formula>. Then, after the projection we obtain
<disp-formula id="pty025-M26"><label>(26)</label><tex-math notation="LaTeX" id="Equation26"><![CDATA[
\begin{align}
i_n^h(q,z)=\frac{q^{\frac{1}{2}}}{1-q^n}
(q^{[-h-\frac{1}{2}]_n}z+q^{[h-\frac{1}{2}]_n}z^{-1}),\quad h=\frac{1}{2},\ldots,n-\frac{1}{2},
\label{hyperzn}
\end{align}
]]></tex-math></disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation122"><![CDATA[$[x]_n$]]></tex-math></inline-formula> for <inline-formula><tex-math notation="LaTeX" id="ImEquation123"><![CDATA[$x\in{\mathbb{Z}}$]]></tex-math></inline-formula> is the minimum non-negative integer satisfying <inline-formula><tex-math notation="LaTeX" id="ImEquation124"><![CDATA[$[x]_n\equiv x\mod n$]]></tex-math></inline-formula>. In the <inline-formula><tex-math notation="LaTeX" id="ImEquation125"><![CDATA[${\mathbb{Z}}_2$]]></tex-math></inline-formula> case, the one-particle indices for the two holonomies <inline-formula><tex-math notation="LaTeX" id="ImEquation126"><![CDATA[$h=\pm1/2$]]></tex-math></inline-formula> are
<disp-formula id="pty025-M27"><label>(27)</label><tex-math notation="LaTeX" id="Equation27"><![CDATA[
\begin{align}
i_2^{+\frac{1}{2}}=\frac{q^{\frac{1}{2}}}{1-q^2}(qz+z^{-1}),\quad i_2^{-\frac{1}{2}}=\frac{q^{\frac{1}{2}}}{1-q^2}(z+qz^{-1}).
\label{hyperz2}
\end{align}
]]></tex-math></disp-formula></p>
</sec>
<sec id="SEC2.3"><title>2.3. QED</title>
<p>Let us consider <inline-formula><tex-math notation="LaTeX" id="ImEquation127"><![CDATA[$U(1)$]]></tex-math></inline-formula> gauge theory with <inline-formula><tex-math notation="LaTeX" id="ImEquation128"><![CDATA[$N_f$]]></tex-math></inline-formula> hypermultiplets. This theory is not conformal, but we can obtain the index by applying the localization formula. When we consider the orbifold index, we should be careful about the fact that <inline-formula><tex-math notation="LaTeX" id="ImEquation129"><![CDATA[$U(1)_r$]]></tex-math></inline-formula> is broken to the subgroup <inline-formula><tex-math notation="LaTeX" id="ImEquation130"><![CDATA[${\mathbb{Z}}_{N_f}\subset U(1)_r$]]></tex-math></inline-formula> by an anomaly. The orbifold action must be consistent with this unbroken symmetry. For example, in the case of the <inline-formula><tex-math notation="LaTeX" id="ImEquation131"><![CDATA[${\mathbb{Z}}_2$]]></tex-math></inline-formula> orbifold, <inline-formula><tex-math notation="LaTeX" id="ImEquation132"><![CDATA[$N_f$]]></tex-math></inline-formula> must be even. For <inline-formula><tex-math notation="LaTeX" id="ImEquation133"><![CDATA[$N_f=2$]]></tex-math></inline-formula> the <inline-formula><tex-math notation="LaTeX" id="ImEquation134"><![CDATA[${\mathbb{Z}}_2$]]></tex-math></inline-formula> orbifold index is given by
<disp-formula id="pty025-M28"><label>(28)</label><tex-math notation="LaTeX" id="Equation28"><![CDATA[
\begin{align}
I^{\frac{1}{2}}_2
&=
\lambda_2
\sum_{h=\pm\frac{1}{2}}\oint\frac{dz}{2\pi iz}
{\rm Pexp}\left(2i_2^h\right)
=2(1+2q^2+8q^4+\cdots),
\label{qednf2}
\end{align}
]]></tex-math></disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation135"><![CDATA[$i_2^h$]]></tex-math></inline-formula> is the one-particle index of Eq. (<xref ref-type="disp-formula" rid="pty025-M27">27</xref>) for a single hypermultiplet. We did not turn on the <inline-formula><tex-math notation="LaTeX" id="ImEquation136"><![CDATA[$SU(N_F)$]]></tex-math></inline-formula> flavor symmetry for simplicity, and we omitted the zero-point factor which does not depend on <inline-formula><tex-math notation="LaTeX" id="ImEquation137"><![CDATA[$h=\pm1/2$]]></tex-math></inline-formula>.</p>
</sec>
</sec>
<sec id="SEC3"><title>3. IR formula</title>
<p>The IR formula proposed by Cordova and Shao [<xref ref-type="bibr" rid="B4">4</xref>] gives the Schur index by using the information of the BPS spectrum in the Coulomb branch.</p>
<p>Let <inline-formula><tex-math notation="LaTeX" id="ImEquation138"><![CDATA[$\Gamma$]]></tex-math></inline-formula> be the charge lattice of flavor and gauge charges, and <inline-formula><tex-math notation="LaTeX" id="ImEquation139"><![CDATA[$\langle\gamma,\gamma'\rangle$]]></tex-math></inline-formula> be the associated Dirac pairing. The central charge of a particle is determined by its charge <inline-formula><tex-math notation="LaTeX" id="ImEquation140"><![CDATA[$\gamma\in\Gamma$]]></tex-math></inline-formula>, and we denote it by <inline-formula><tex-math notation="LaTeX" id="ImEquation141"><![CDATA[$Z_\gamma$]]></tex-math></inline-formula>. The flavor sublattice <inline-formula><tex-math notation="LaTeX" id="ImEquation142"><![CDATA[$\Gamma_F\subset\Gamma$]]></tex-math></inline-formula> is defined as the set of charges <inline-formula><tex-math notation="LaTeX" id="ImEquation143"><![CDATA[$\gamma$]]></tex-math></inline-formula> which have vanishing pairing <inline-formula><tex-math notation="LaTeX" id="ImEquation144"><![CDATA[$\langle\gamma,\gamma'\rangle=0$]]></tex-math></inline-formula> with arbitrary <inline-formula><tex-math notation="LaTeX" id="ImEquation145"><![CDATA[$\gamma'\in\Gamma$]]></tex-math></inline-formula>.</p>
<p>Let <inline-formula><tex-math notation="LaTeX" id="ImEquation146"><![CDATA[$L$]]></tex-math></inline-formula> be the set of primitive charges such that the charge of an arbitrary BPS particle is given by <inline-formula><tex-math notation="LaTeX" id="ImEquation147"><![CDATA[$n\gamma$]]></tex-math></inline-formula> with <inline-formula><tex-math notation="LaTeX" id="ImEquation148"><![CDATA[$\gamma\in L$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation149"><![CDATA[$n\in{\mathbb{Z}}_+$]]></tex-math></inline-formula>. The BPS spectrum at a point of the Coulomb branch is encoded in a set of functions <inline-formula><tex-math notation="LaTeX" id="ImEquation150"><![CDATA[$K_\gamma(z)$]]></tex-math></inline-formula> defined for each <inline-formula><tex-math notation="LaTeX" id="ImEquation151"><![CDATA[$\gamma\in L$]]></tex-math></inline-formula>. These functions are called quantum Kontsevich&#x2013;Soibelman factors. The functional form of <inline-formula><tex-math notation="LaTeX" id="ImEquation152"><![CDATA[$K_\gamma(z)$]]></tex-math></inline-formula> depends on the helicity of the BPS particle <inline-formula><tex-math notation="LaTeX" id="ImEquation153"><![CDATA[$\gamma$]]></tex-math></inline-formula>. (By an abuse of notation we use <inline-formula><tex-math notation="LaTeX" id="ImEquation154"><![CDATA[$\gamma$]]></tex-math></inline-formula> as a label for sorts of particles.) In the following we deal with only BPS particles belonging to a half-hypermultiplet, and the function <inline-formula><tex-math notation="LaTeX" id="ImEquation155"><![CDATA[$K_\gamma$]]></tex-math></inline-formula> for such a particle is given by
<disp-formula id="pty025-M29"><label>(29)</label><tex-math notation="LaTeX" id="Equation29"><![CDATA[
\begin{align}
K_\gamma(z)=E_q(z)
={\rm Pexp}\frac{q^{\frac{1}{2}}z}{1-q}
=\prod_{k=0}^\infty
\frac{1}{1-q^{\frac{1}{2}+k}z}
=\sum_{k=0}^\infty
\frac{q^{\frac{k}{2}}}{(q)_k}z^k,
\end{align}
]]></tex-math></disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation156"><![CDATA[$(q)_k$]]></tex-math></inline-formula> is the <inline-formula><tex-math notation="LaTeX" id="ImEquation157"><![CDATA[$q$]]></tex-math></inline-formula>-factorial defined by <inline-formula><tex-math notation="LaTeX" id="ImEquation158"><![CDATA[$(q)_k=\prod_{i=1}^k(1-q^i)$]]></tex-math></inline-formula>.</p>
<p>Cordova and Shao&#x2019;s IR formula [<xref ref-type="bibr" rid="B4">4</xref>] is
<disp-formula id="pty025-M30"><label>(30)</label><tex-math notation="LaTeX" id="Equation30"><![CDATA[
\begin{align}
I
&=\lambda^r{\rm tr}\left(
\prod^\curvearrowleft_{\gamma\in L} K_\gamma(X_\gamma)\right)\!,
\end{align}
]]></tex-math></disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation159"><![CDATA[$\prod^\curvearrowleft_{\gamma\in L}$]]></tex-math></inline-formula> is the phase-ordered product according to <inline-formula><tex-math notation="LaTeX" id="ImEquation160"><![CDATA[$\arg Z_\gamma$]]></tex-math></inline-formula>; <inline-formula><tex-math notation="LaTeX" id="ImEquation161"><![CDATA[$r$]]></tex-math></inline-formula> is the rank of the theory, which is the number of massless <inline-formula><tex-math notation="LaTeX" id="ImEquation162"><![CDATA[$U(1)$]]></tex-math></inline-formula> gauge fields at a generic point of the Coulomb branch. <inline-formula><tex-math notation="LaTeX" id="ImEquation163"><![CDATA[$X_\gamma$]]></tex-math></inline-formula> are operators satisfying the quantum torus algebra<xref ref-type="fn" rid="FN3"><sup>3</sup></xref>
<disp-formula id="pty025-M31"><label>(31)</label><tex-math notation="LaTeX" id="Equation31"><![CDATA[
\begin{align}
X_\gamma X_{\gamma'}
=(-q^{\frac{1}{2}})^{\langle\gamma,\gamma'\rangle}
X_{\gamma+\gamma'}
=q^{\langle\gamma,\gamma'\rangle}
X_{\gamma'}X_\gamma.
\label{xxalgebra}
\end{align}
]]></tex-math></disp-formula></p>
<p>The trace <inline-formula><tex-math notation="LaTeX" id="ImEquation164"><![CDATA[${\rm tr} X_\gamma$]]></tex-math></inline-formula> is defined as an isomorphic map from <inline-formula><tex-math notation="LaTeX" id="ImEquation165"><![CDATA[$\Gamma_F$]]></tex-math></inline-formula> to <inline-formula><tex-math notation="LaTeX" id="ImEquation166"><![CDATA[${\mathbb{C}}^*$]]></tex-math></inline-formula>. If <inline-formula><tex-math notation="LaTeX" id="ImEquation167"><![CDATA[$\gamma\notin\Gamma_F$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation168"><![CDATA[${\rm tr} X_\gamma=0$]]></tex-math></inline-formula>.</p>
<p>To physically interpret this formula, we should understand the structure of BPS configurations in the Coulomb branch [<xref ref-type="bibr" rid="B5">5</xref>]. In general, a BPS configuration contains massive BPS particles with different charges. For a configuration in <inline-formula><tex-math notation="LaTeX" id="ImEquation169"><![CDATA[$\boldsymbol{S}^3\times{\mathbb{R}}_t$]]></tex-math></inline-formula> to preserve the supercharges <inline-formula><tex-math notation="LaTeX" id="ImEquation170"><![CDATA[$Q$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation171"><![CDATA[$\overline Q$]]></tex-math></inline-formula>, which are necessary to define the Schur index, the particles must be aligned along a large circle in <inline-formula><tex-math notation="LaTeX" id="ImEquation172"><![CDATA[$\boldsymbol{S}^3$]]></tex-math></inline-formula>, and the position <inline-formula><tex-math notation="LaTeX" id="ImEquation173"><![CDATA[$\theta_\gamma$]]></tex-math></inline-formula> on the circle is determined by the central charge <inline-formula><tex-math notation="LaTeX" id="ImEquation174"><![CDATA[$Z_\gamma$]]></tex-math></inline-formula> by <inline-formula><tex-math notation="LaTeX" id="ImEquation175"><![CDATA[$\theta_\gamma=\arg Z_\gamma$]]></tex-math></inline-formula>. Thus we can specify the particle distribution in a BPS configuration by giving a set of occupation numbers <inline-formula><tex-math notation="LaTeX" id="ImEquation176"><![CDATA[$n_\gamma$]]></tex-math></inline-formula> for <inline-formula><tex-math notation="LaTeX" id="ImEquation177"><![CDATA[$\gamma\in L$]]></tex-math></inline-formula>. We denote this set by <inline-formula><tex-math notation="LaTeX" id="ImEquation178"><![CDATA[$\{n_\gamma\}_{\gamma\in L}$]]></tex-math></inline-formula>.</p>
<p>If we expand the function <inline-formula><tex-math notation="LaTeX" id="ImEquation179"><![CDATA[$K_\gamma$]]></tex-math></inline-formula> as
<disp-formula id="pty025-M32"><label>(32)</label><tex-math notation="LaTeX" id="Equation32"><![CDATA[
\begin{align}
K_\gamma(z)=\sum_{n=0}^\infty C_\gamma(n)z^n,
\end{align}
]]></tex-math></disp-formula>
then the index is given as the summation over the occupation numbers:
<disp-formula id="pty025-M33"><label>(33)</label><tex-math notation="LaTeX" id="Equation33"><![CDATA[
\begin{align}
I
&=\sum_{\{n_\gamma\}_{\gamma\in L}}
\lambda^r
\left(\prod_{\gamma\in L} C_\gamma(n_\gamma)\right)
{\rm tr}\left(\prod^\curvearrowleft_{\gamma\in L} X_\gamma^{n_\gamma}\right)\!.
\end{align}
]]></tex-math></disp-formula></p>
<p>The summand gives the contribution of a specific set of occupation numbers, and consists of the following three factors:
<list list-type="simple">
<list-item><p>&#x2218; The factor <inline-formula><tex-math notation="LaTeX" id="ImEquation180"><![CDATA[$\lambda^r$]]></tex-math></inline-formula> is the one-loop contribution of the massless vector multiplets.</p></list-item>
<list-item><p>&#x2218; The factor <inline-formula><tex-math notation="LaTeX" id="ImEquation181"><![CDATA[$\prod C$]]></tex-math></inline-formula> is the contribution associated with internal degrees of freedom of BPS particles.</p></list-item>
<list-item><p>&#x2218; The trace factor can be identified with the classical contribution of massless vector multiplets. The angular momentum induced by the Poynting vector due to the existence of mutually non-local charges contributes to the index by the factor <inline-formula><tex-math notation="LaTeX" id="ImEquation182"><![CDATA[$e^{2\pi i(J+\overline J)}q^{J+\overline J}$]]></tex-math></inline-formula>, and the <inline-formula><tex-math notation="LaTeX" id="ImEquation183"><![CDATA[$q$]]></tex-math></inline-formula>-dependence of the trace factor gives this factor. For example, let us consider two adjacent charges <inline-formula><tex-math notation="LaTeX" id="ImEquation184"><![CDATA[$\gamma$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation185"><![CDATA[$\gamma'$]]></tex-math></inline-formula> on the large circle. If they carry mutually non-local charges, the induced massless gauge fields contribute to the angular momentum <inline-formula><tex-math notation="LaTeX" id="ImEquation186"><![CDATA[$J+\overline J$]]></tex-math></inline-formula> by <inline-formula><tex-math notation="LaTeX" id="ImEquation187"><![CDATA[$\pm\frac{1}{2}\langle\gamma,\gamma'\rangle$]]></tex-math></inline-formula>. The angular momentum is independent of the distance between charges while the signature depends on the order of the charges along the circle. This order dependence is correctly reproduced by the algebra of Eq. (<xref ref-type="disp-formula" rid="pty025-M31">31</xref>). This factor also provides the dependence on the flavor fugacities.</p></list-item>
</list></p>
<p>Now we suggest an IR formula for the orbifold as a natural generalization of the original one. <inline-formula><tex-math notation="LaTeX" id="ImEquation188"><![CDATA[${\mathbb{Z}}_n$]]></tex-math></inline-formula> acts on the large circle as a shift by <inline-formula><tex-math notation="LaTeX" id="ImEquation189"><![CDATA[$2\pi/n$]]></tex-math></inline-formula> and the orbifolding makes it a circle with circumference <inline-formula><tex-math notation="LaTeX" id="ImEquation190"><![CDATA[$2\pi/n$]]></tex-math></inline-formula>. In other words, the large circle in the covering space consists of <inline-formula><tex-math notation="LaTeX" id="ImEquation191"><![CDATA[$n$]]></tex-math></inline-formula> fundamental regions, and only BPS particles in one of the fundamental regions are independent. Let <inline-formula><tex-math notation="LaTeX" id="ImEquation192"><![CDATA[$L_n$]]></tex-math></inline-formula> be the set of primitive charges associated with a specific fundamental region. The charge distribution of a BPS configuration in the orbifold is specified by <inline-formula><tex-math notation="LaTeX" id="ImEquation193"><![CDATA[$\{n_\gamma\}_{\gamma\in L_n}$]]></tex-math></inline-formula>. Therefore, the index should be given as the summation over <inline-formula><tex-math notation="LaTeX" id="ImEquation194"><![CDATA[$\{n_\gamma\}_{\gamma\in L_n}$]]></tex-math></inline-formula>.</p>
<p>The first factor in the summand should be replaced by the <inline-formula><tex-math notation="LaTeX" id="ImEquation195"><![CDATA[$U(1)$]]></tex-math></inline-formula> factor <inline-formula><tex-math notation="LaTeX" id="ImEquation196"><![CDATA[$\lambda_n^r$]]></tex-math></inline-formula>, with <inline-formula><tex-math notation="LaTeX" id="ImEquation197"><![CDATA[$\lambda_n$]]></tex-math></inline-formula> given in Eq. (<xref ref-type="disp-formula" rid="pty025-M23">23</xref>). The second factor associated with the internal degrees of freedom of BPS particles should be the product of <inline-formula><tex-math notation="LaTeX" id="ImEquation198"><![CDATA[$C_\gamma(n_\gamma)$]]></tex-math></inline-formula> for <inline-formula><tex-math notation="LaTeX" id="ImEquation199"><![CDATA[$\gamma\in L_n$]]></tex-math></inline-formula>. The third factor, as we mentioned above, can be regarded as the classical contribution to the angular momentum and the flavor charges. The angular momentum can be obtained by integrating the contribution of the Poynting vector over the orbifold. The same result is obtained by first calculating the angular momentum for the covering space <inline-formula><tex-math notation="LaTeX" id="ImEquation200"><![CDATA[${\boldsymbol S}^3$]]></tex-math></inline-formula>, and dividing the result by <inline-formula><tex-math notation="LaTeX" id="ImEquation201"><![CDATA[$n$]]></tex-math></inline-formula>. This is also the case for the flavor charges. Correspondingly, the trace factor should be replaced by the <inline-formula><tex-math notation="LaTeX" id="ImEquation202"><![CDATA[$n$]]></tex-math></inline-formula>th root of the trace for the configuration in the covering space. Combining these, we obtain
<disp-formula id="pty025-M34"><label>(34)</label><tex-math notation="LaTeX" id="Equation34"><![CDATA[
\begin{align}
I_n=
\sum_{\{n_\gamma\}_{L_n}}
\lambda_n^r
\left(\prod_{\gamma\in L_n}C_\gamma(n_\gamma)\right)
\left[{\rm tr}\left(\prod_{\gamma\in L}^\curvearrowleft X_\gamma^{n_\gamma}\right)\right]^{1/n}.
\label{irzn}
\end{align}
]]></tex-math></disp-formula></p>
<p>This is the IR formula we want to discuss in the next section.</p>
<p>An additional comment on the trace factor would be in order. As we mentioned above, only charge distribution in a specific fundamental region is independent, and the distribution in other regions should be determined by the <inline-formula><tex-math notation="LaTeX" id="ImEquation203"><![CDATA[${\mathbb{Z}}_n$]]></tex-math></inline-formula> symmetry. The phase-ordered trance in Eq. (<xref ref-type="disp-formula" rid="pty025-M34">34</xref>) must be taken over all charges in the covering space. It is important that the <inline-formula><tex-math notation="LaTeX" id="ImEquation204"><![CDATA[${\mathbb{Z}}_n$]]></tex-math></inline-formula> acts on charges non-trivially, and the product is not the simple <inline-formula><tex-math notation="LaTeX" id="ImEquation205"><![CDATA[$n$]]></tex-math></inline-formula>th power of the product in the fundamental region. In the <inline-formula><tex-math notation="LaTeX" id="ImEquation206"><![CDATA[$n=2$]]></tex-math></inline-formula> case, for example, the <inline-formula><tex-math notation="LaTeX" id="ImEquation207"><![CDATA[${\mathbb{Z}}_2$]]></tex-math></inline-formula> action flips the signs of charges, as we will see explicitly in the next section, and the trace factor takes the form <inline-formula><tex-math notation="LaTeX" id="ImEquation208"><![CDATA[$\left[{\rm tr}(X_{\gamma_1}^{n_1}X_{\gamma_2}^{n_2}\cdots X_{-\gamma_1}^{n_1}X_{-\gamma_2}^{n_2}\cdots)\right]^{1/2}$]]></tex-math></inline-formula>.</p>
</sec>
<sec id="SEC4"><title>4. Comparison</title>
<p>Let us apply the IR formula in Eq. (<xref ref-type="disp-formula" rid="pty025-M34">34</xref>) to a few simple examples and compare the results with those obtained by the UV formula.</p>
<p>We first consider the system of a free hypermultiplet <inline-formula><tex-math notation="LaTeX" id="ImEquation209"><![CDATA[$\vec q=(q,\widetilde q)$]]></tex-math></inline-formula>. Before computing the index by the UV and IR formulae it is important to check the consistency between BPS configurations in the Coulomb branch and the orbifold action.</p>
<p>In the system of a single hypermultiplet, we have only two sorts of particles with flavor charge <inline-formula><tex-math notation="LaTeX" id="ImEquation210"><![CDATA[$\pm\gamma$]]></tex-math></inline-formula>. In a BPS configuration there are particles with charge <inline-formula><tex-math notation="LaTeX" id="ImEquation211"><![CDATA[$+\gamma$]]></tex-math></inline-formula> at <inline-formula><tex-math notation="LaTeX" id="ImEquation212"><![CDATA[$\theta_\gamma=\arg Z_\gamma$]]></tex-math></inline-formula> and anti-particles with charge <inline-formula><tex-math notation="LaTeX" id="ImEquation213"><![CDATA[$-\gamma$]]></tex-math></inline-formula> at <inline-formula><tex-math notation="LaTeX" id="ImEquation214"><![CDATA[$\theta_\gamma+\pi$]]></tex-math></inline-formula>. This cannot be invariant under <inline-formula><tex-math notation="LaTeX" id="ImEquation215"><![CDATA[${\mathbb{Z}}_n$]]></tex-math></inline-formula> action with <inline-formula><tex-math notation="LaTeX" id="ImEquation216"><![CDATA[$n\geq 3$]]></tex-math></inline-formula>. Even for <inline-formula><tex-math notation="LaTeX" id="ImEquation217"><![CDATA[$n=2$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation218"><![CDATA[${\mathbb{Z}}_2$]]></tex-math></inline-formula> exchanges particles and anti-particles, and the orbifolding seems to contradict the BPS configuration in the Coulomb branch. When <inline-formula><tex-math notation="LaTeX" id="ImEquation219"><![CDATA[$n=2$]]></tex-math></inline-formula>, actually, we can take it back to the original configuration by performing additional charge conjugation. This additional transformation is also necessary to keep the mass term in the Lagrangian <inline-formula><tex-math notation="LaTeX" id="ImEquation220"><![CDATA[${\mathbb{Z}}_2$]]></tex-math></inline-formula> invariant. To make the hypermultiplet massive we need to turn on the vacuum expectation value (VEV) <inline-formula><tex-math notation="LaTeX" id="ImEquation221"><![CDATA[$\langle\phi\rangle=m$]]></tex-math></inline-formula> of the scalar component <inline-formula><tex-math notation="LaTeX" id="ImEquation222"><![CDATA[$\phi$]]></tex-math></inline-formula> of the non-dynamical background vector multiplet coupling to the <inline-formula><tex-math notation="LaTeX" id="ImEquation223"><![CDATA[$U(1)_F$]]></tex-math></inline-formula> current. Because <inline-formula><tex-math notation="LaTeX" id="ImEquation224"><![CDATA[$\phi$]]></tex-math></inline-formula> carries a <inline-formula><tex-math notation="LaTeX" id="ImEquation225"><![CDATA[$U(1)_r$]]></tex-math></inline-formula> charge of <inline-formula><tex-math notation="LaTeX" id="ImEquation226"><![CDATA[$+2$]]></tex-math></inline-formula>, the <inline-formula><tex-math notation="LaTeX" id="ImEquation227"><![CDATA[$g_2$]]></tex-math></inline-formula> action changes its sign. This is compensated by the additional charge conjugation, which flips the sign of the background vector multiplet.</p>
<p>The charge conjugation exchanging <inline-formula><tex-math notation="LaTeX" id="ImEquation228"><![CDATA[$q$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation229"><![CDATA[$\widetilde q$]]></tex-math></inline-formula> is realized by the <inline-formula><tex-math notation="LaTeX" id="ImEquation230"><![CDATA[$SU(2)_F$]]></tex-math></inline-formula> transformation <inline-formula><tex-math notation="LaTeX" id="ImEquation231"><![CDATA[$\vec q\rightarrow U\vec q$]]></tex-math></inline-formula> with
<disp-formula id="pty025-M35"><label>(35)</label><tex-math notation="LaTeX" id="Equation35"><![CDATA[
\begin{align}
U=i\sigma_x.
\label{un2}
\end{align}
]]></tex-math></disp-formula></p>
<p>This anti-commutes with the <inline-formula><tex-math notation="LaTeX" id="ImEquation232"><![CDATA[$U(1)_F$]]></tex-math></inline-formula> generator <inline-formula><tex-math notation="LaTeX" id="ImEquation233"><![CDATA[$i\sigma_z$]]></tex-math></inline-formula>, and works as the charge conjugation. For consistency, we should set the <inline-formula><tex-math notation="LaTeX" id="ImEquation234"><![CDATA[$U(1)_F$]]></tex-math></inline-formula> Wilson line to be <inline-formula><tex-math notation="LaTeX" id="ImEquation235"><![CDATA[$z=\pm 1$]]></tex-math></inline-formula>. (A generic Wilson line is not allowed because the operator <inline-formula><tex-math notation="LaTeX" id="ImEquation236"><![CDATA[$z^F$]]></tex-math></inline-formula> does not commute with <inline-formula><tex-math notation="LaTeX" id="ImEquation237"><![CDATA[$i\sigma_x$]]></tex-math></inline-formula>, and is incompatible with the orbifold action.)</p>
<p>Now we have chosen a <inline-formula><tex-math notation="LaTeX" id="ImEquation238"><![CDATA[${\mathbb{Z}}_2$]]></tex-math></inline-formula> generator <inline-formula><tex-math notation="LaTeX" id="ImEquation239"><![CDATA[$g_2U$]]></tex-math></inline-formula> consistent with the Coulomb branch VEV. Let us calculate the index by using the UV and IR formulae. When <inline-formula><tex-math notation="LaTeX" id="ImEquation240"><![CDATA[$z=\pm1$]]></tex-math></inline-formula>, the orbifold with the charge conjugation twist is in fact equivalent to the <inline-formula><tex-math notation="LaTeX" id="ImEquation241"><![CDATA[${\mathbb{Z}}_2$]]></tex-math></inline-formula> orbifold with fractional holonomies studied in the previous section up to <inline-formula><tex-math notation="LaTeX" id="ImEquation242"><![CDATA[$SU(2)_F$]]></tex-math></inline-formula> rotation, because the fractional holonomy <inline-formula><tex-math notation="LaTeX" id="ImEquation243"><![CDATA[$\omega_2^{hF}=\pm i\sigma_z$]]></tex-math></inline-formula> is <inline-formula><tex-math notation="LaTeX" id="ImEquation244"><![CDATA[$SU(2)_F$]]></tex-math></inline-formula> conjugate to the charge conjugation <inline-formula><tex-math notation="LaTeX" id="ImEquation245"><![CDATA[$U=i\sigma_x$]]></tex-math></inline-formula>. Therefore, the index is still given by Eq. (<xref ref-type="disp-formula" rid="pty025-M27">27</xref>) with <inline-formula><tex-math notation="LaTeX" id="ImEquation246"><![CDATA[$z=\pm1$]]></tex-math></inline-formula>. By setting <inline-formula><tex-math notation="LaTeX" id="ImEquation247"><![CDATA[$z=1$]]></tex-math></inline-formula>, the one-particle index becomes
<disp-formula id="pty025-M36"><label>(36)</label><tex-math notation="LaTeX" id="Equation36"><![CDATA[
\begin{align}
i_2^{\pm\frac{1}{2}}=\frac{q^{\frac{1}{2}}}{1-q},
\label{irresult}
\end{align}
]]></tex-math></disp-formula>
and the Schur index is
<disp-formula id="pty025-M37"><label>(37)</label><tex-math notation="LaTeX" id="Equation37"><![CDATA[
\begin{align}
I_2={\rm Pexp}\frac{q^{\frac{1}{2}}}{1-q}=E_q(1).
\label{i2z}
\end{align}
]]></tex-math></disp-formula></p>
<p>On the IR side, we have only one charge <inline-formula><tex-math notation="LaTeX" id="ImEquation248"><![CDATA[$\gamma$]]></tex-math></inline-formula> in <inline-formula><tex-math notation="LaTeX" id="ImEquation249"><![CDATA[$L_2$]]></tex-math></inline-formula>. The suggested formula in Eq. (<xref ref-type="disp-formula" rid="pty025-M34">34</xref>) gives
<disp-formula id="pty025-M38"><label>(38)</label><tex-math notation="LaTeX" id="Equation38"><![CDATA[
\begin{align}
I_2=\sum_{n=0}^\infty C_\gamma(n)=E_q(1),
\end{align}
]]></tex-math></disp-formula>
and this agrees with Eq. (<xref ref-type="disp-formula" rid="pty025-M37">37</xref>).</p>
<p>By introducing multiple hypermultiplets we can realize more general orbifolds. Let us consider a system of <inline-formula><tex-math notation="LaTeX" id="ImEquation250"><![CDATA[$k$]]></tex-math></inline-formula> free hypermultiplets. There are <inline-formula><tex-math notation="LaTeX" id="ImEquation251"><![CDATA[$2k$]]></tex-math></inline-formula> sorts of particles. For <inline-formula><tex-math notation="LaTeX" id="ImEquation252"><![CDATA[${\mathbb{Z}}_{2k}$]]></tex-math></inline-formula> invariance, we need to tune the Coulomb branch VEV <inline-formula><tex-math notation="LaTeX" id="ImEquation253"><![CDATA[$\phi$]]></tex-math></inline-formula> and introduce an appropriate twist <inline-formula><tex-math notation="LaTeX" id="ImEquation254"><![CDATA[$U_k$]]></tex-math></inline-formula>. Let <inline-formula><tex-math notation="LaTeX" id="ImEquation255"><![CDATA[$\phi={\rm diag}(a_1,\ldots,a_k)\otimes\sigma_z\in sp(k)$]]></tex-math></inline-formula> be the Coulomb branch VEV (we use the basis in which the <inline-formula><tex-math notation="LaTeX" id="ImEquation256"><![CDATA[$Sp(k)$]]></tex-math></inline-formula> invariant tensor is given by <inline-formula><tex-math notation="LaTeX" id="ImEquation257"><![CDATA[$J=\boldsymbol{1}_k\otimes\epsilon$]]></tex-math></inline-formula>). We tune <inline-formula><tex-math notation="LaTeX" id="ImEquation258"><![CDATA[$a_i$]]></tex-math></inline-formula> so that the central charges are <inline-formula><tex-math notation="LaTeX" id="ImEquation259"><![CDATA[${\mathbb{Z}}_{2k}$]]></tex-math></inline-formula> symmetric and given by
<disp-formula id="pty025-M39"><label>(39)</label><tex-math notation="LaTeX" id="Equation39"><![CDATA[
\begin{align}
Z(q_i)=a_i=\omega^i_{2k}a,\quad Z(\widetilde q_i)=-a_i=\omega^{k+i}_{2k}a.
\end{align}
]]></tex-math></disp-formula></p>
<p>The action of <inline-formula><tex-math notation="LaTeX" id="ImEquation260"><![CDATA[$g_{2k}$]]></tex-math></inline-formula> shifts <inline-formula><tex-math notation="LaTeX" id="ImEquation261"><![CDATA[$a_i$]]></tex-math></inline-formula> to <inline-formula><tex-math notation="LaTeX" id="ImEquation262"><![CDATA[$a_{i+1}$]]></tex-math></inline-formula> for <inline-formula><tex-math notation="LaTeX" id="ImEquation263"><![CDATA[$i=1\sim k-1$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation264"><![CDATA[$a_k$]]></tex-math></inline-formula> to <inline-formula><tex-math notation="LaTeX" id="ImEquation265"><![CDATA[$-a_1$]]></tex-math></inline-formula>. To keep the background unchanged, we need a twist <inline-formula><tex-math notation="LaTeX" id="ImEquation266"><![CDATA[$U_k$]]></tex-math></inline-formula> such that the transformation <inline-formula><tex-math notation="LaTeX" id="ImEquation267"><![CDATA[$\phi'=U_k\phi U_k^\dagger$]]></tex-math></inline-formula> acts on <inline-formula><tex-math notation="LaTeX" id="ImEquation268"><![CDATA[$a_i$]]></tex-math></inline-formula> as
<disp-formula id="pty025-M40"><label>(40)</label><tex-math notation="LaTeX" id="Equation40"><![CDATA[
\begin{align}
a_1'=-a_k,\quad a_i'=a_{i-1}\quad(i=2\sim k).
\end{align}
]]></tex-math></disp-formula></p>
<p>The following <inline-formula><tex-math notation="LaTeX" id="ImEquation269"><![CDATA[$U_k$]]></tex-math></inline-formula> realize this transformation:
<disp-formula id="pty025-M41"><label>(41)</label><tex-math notation="LaTeX" id="Equation41"><![CDATA[
\begin{align}
U_k=\left(\begin{array}{cccc}
& \boldsymbol{1}_2 \\
&& \ddots \\
&&& \boldsymbol{1}_2 \\
i\sigma_x
\end{array}\right)\in Sp(k).
\label{udef}
\end{align}
]]></tex-math></disp-formula></p>
<p>(This is a generalization of the charge conjugation in Eq. (<xref ref-type="disp-formula" rid="pty025-M35">35</xref>) in the <inline-formula><tex-math notation="LaTeX" id="ImEquation270"><![CDATA[$k=1$]]></tex-math></inline-formula> case.) For the same reason as the <inline-formula><tex-math notation="LaTeX" id="ImEquation271"><![CDATA[${\mathbb{Z}}_2$]]></tex-math></inline-formula> case we set the Wilson line to vanish. The diagonalization of <inline-formula><tex-math notation="LaTeX" id="ImEquation272"><![CDATA[$U_k$]]></tex-math></inline-formula> gives the eigenvalues <inline-formula><tex-math notation="LaTeX" id="ImEquation273"><![CDATA[$\pm\alpha_m$]]></tex-math></inline-formula> with
<disp-formula id="pty025-M42"><label>(42)</label><tex-math notation="LaTeX" id="Equation42"><![CDATA[
\begin{align}
\alpha_m=\exp\left(\frac{2\pi i}{2k}\left(m+\frac{1}{2}\right)\right)\!,\quad m=0,\ldots,k-1.
\end{align}
]]></tex-math></disp-formula></p>
<p>For each pair <inline-formula><tex-math notation="LaTeX" id="ImEquation274"><![CDATA[$(\alpha_m,-\alpha_m)$]]></tex-math></inline-formula> of eigenvalues this is the same as the action of the fractional holonomy <inline-formula><tex-math notation="LaTeX" id="ImEquation275"><![CDATA[$h=m+1/2$]]></tex-math></inline-formula> on a single hypermultiplet, and the one-particle index of the whole system is the sum of Eq. (<xref ref-type="disp-formula" rid="pty025-M26">26</xref>) over <inline-formula><tex-math notation="LaTeX" id="ImEquation276"><![CDATA[$h=1/2,\ldots,k-1/2$]]></tex-math></inline-formula>:
<disp-formula id="pty025-M43"><label>(43)</label><tex-math notation="LaTeX" id="Equation43"><![CDATA[
\begin{align}
i_n=\frac{q^{\frac{1}{2}}}{1-q^{2k}}(1+q+\cdots+q^{2k-1})=\frac{q^{\frac{1}{2}}}{1-q}.
\end{align}
]]></tex-math></disp-formula></p>
<p>The Schur index is <inline-formula><tex-math notation="LaTeX" id="ImEquation277"><![CDATA[$I_n=\,{\rm Pexp}\,i_n=E_q(1)$]]></tex-math></inline-formula>, and this is the same as what we obtain from the IR formula. Each fundamental region of the large circle contains one sort of particle and the IR formula in Eq. (<xref ref-type="disp-formula" rid="pty025-M34">34</xref>) gives <inline-formula><tex-math notation="LaTeX" id="ImEquation278"><![CDATA[$I=E_q(1)$]]></tex-math></inline-formula>.</p>
<p>We can consider a more general case in which <inline-formula><tex-math notation="LaTeX" id="ImEquation279"><![CDATA[$n$]]></tex-math></inline-formula> is not <inline-formula><tex-math notation="LaTeX" id="ImEquation280"><![CDATA[$2k$]]></tex-math></inline-formula> but its divisor, <inline-formula><tex-math notation="LaTeX" id="ImEquation281"><![CDATA[$n=2k/d$]]></tex-math></inline-formula>. Such an orbifold is defined by using <inline-formula><tex-math notation="LaTeX" id="ImEquation282"><![CDATA[$(g_{2k}U_k)^d$]]></tex-math></inline-formula> as the <inline-formula><tex-math notation="LaTeX" id="ImEquation283"><![CDATA[${\mathbb{Z}}_n$]]></tex-math></inline-formula> generator, and the one-particle index becomes
<disp-formula id="pty025-M44"><label>(44)</label><tex-math notation="LaTeX" id="Equation44"><![CDATA[
\begin{align}
i_n
=\frac{q^{\frac{1}{2}}}{1-q^k}\sum_{m=0}^{2k-1}q^{[m]_n}
=d\frac{q^{\frac{1}{2}}}{1-q} ;
\end{align}
]]></tex-math></disp-formula>
the Schur index is <inline-formula><tex-math notation="LaTeX" id="ImEquation284"><![CDATA[$I_n=\,{\rm Pexp}\,i_n=E_q(1)^d$]]></tex-math></inline-formula>. Again, this is reproduced by the IR formula of Eq. (<xref ref-type="disp-formula" rid="pty025-M34">34</xref>) by taking account of the <inline-formula><tex-math notation="LaTeX" id="ImEquation285"><![CDATA[$d$]]></tex-math></inline-formula> sorts of particles in a fundamental region.</p>
<p>Up to here we have found good agreement between the UV and IR results. Let us move on to a more complicated system, QED with <inline-formula><tex-math notation="LaTeX" id="ImEquation286"><![CDATA[$N_f$]]></tex-math></inline-formula> hypermultiplets. Although this system is not conformal, it is known that the two formulae give the same answer for the ordinary Schur index [<xref ref-type="bibr" rid="B4">4</xref>], and it is natural to expect this to hold for orbifolds, too. However, disappointingly, we find a discrepancy for the orbifold index in this case.</p>
<p>For example, let us consider the <inline-formula><tex-math notation="LaTeX" id="ImEquation287"><![CDATA[${\mathbb{Z}}_2$]]></tex-math></inline-formula> orbifold of two-flavored QED. The UV formula gives the index in Eq. (<xref ref-type="disp-formula" rid="pty025-M28">28</xref>). When we use the IR formula we need to take account of the existence of two sorts of particles in the fundamental region. Let <inline-formula><tex-math notation="LaTeX" id="ImEquation288"><![CDATA[$\gamma_1$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation289"><![CDATA[$\gamma_2$]]></tex-math></inline-formula> be their charges and <inline-formula><tex-math notation="LaTeX" id="ImEquation290"><![CDATA[$n_1$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation291"><![CDATA[$n_2$]]></tex-math></inline-formula> be the corresponding occupation numbers. In the covering space the charges of particles in a fundamental region are always canceled by the mirror images in the other fundamental region, and the trace factor in Eq. (<xref ref-type="disp-formula" rid="pty025-M34">34</xref>) does not impose any constraints on <inline-formula><tex-math notation="LaTeX" id="ImEquation292"><![CDATA[$n_1$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation293"><![CDATA[$n_2$]]></tex-math></inline-formula>. If we assume the trivial flavor holonomy, the trace factor simply gives <inline-formula><tex-math notation="LaTeX" id="ImEquation294"><![CDATA[$1$]]></tex-math></inline-formula>. This means that the index is essentially the same as that for two half-hypermultiplets in <inline-formula><tex-math notation="LaTeX" id="ImEquation295"><![CDATA[$\boldsymbol{S}^3$]]></tex-math></inline-formula>, and given by
<disp-formula id="pty025-M45"><label>(45)</label><tex-math notation="LaTeX" id="Equation45"><![CDATA[
\begin{align}
I_2
=\lambda_2\sum_{n_1,n_2=0}^\infty C_\gamma(n_1)C_\gamma(n_2)
=\lambda_2E_q^2(1)
=1+2q^{\frac{1}{2}}+3q+6q^{\frac{3}{2}}+\cdots.
\end{align}
]]></tex-math></disp-formula></p>
<p>This is obviously different from the result of the UV formula in Eq. (<xref ref-type="disp-formula" rid="pty025-M28">28</xref>).</p>
</sec>
<sec id="SEC5"><title>5. Discussions</title>
<p>In this paper we generalized the Schur index to the orbifold <inline-formula><tex-math notation="LaTeX" id="ImEquation296"><![CDATA[$\boldsymbol{S}^3/{\mathbb{Z}}_n$]]></tex-math></inline-formula> in such a way that the <inline-formula><tex-math notation="LaTeX" id="ImEquation297"><![CDATA[${\mathbb{Z}}_n$]]></tex-math></inline-formula> action preserves the two supersymmetries respected by the definition of the Schur index. We also naively generalized Cordova and Shao&#x2019;s IR formula for the Schur index to the orbifold case. This reproduces the correct index for a system of free hypermultiplets when the fugacities and holonomies are chosen in a <inline-formula><tex-math notation="LaTeX" id="ImEquation298"><![CDATA[${\mathbb{Z}}_n$]]></tex-math></inline-formula>-invariant way. However, it is far from satisfactory, with the following deficiencies:
<list list-type="simple">
<list-item><p>&#x2218; Although any SCFT admits a <inline-formula><tex-math notation="LaTeX" id="ImEquation299"><![CDATA[${\mathbb{Z}}_n$]]></tex-math></inline-formula> orbifold with an arbitrary <inline-formula><tex-math notation="LaTeX" id="ImEquation300"><![CDATA[$n=2,3,\ldots$]]></tex-math></inline-formula> in the UV description, the IR formula works only for special values of <inline-formula><tex-math notation="LaTeX" id="ImEquation301"><![CDATA[$n$]]></tex-math></inline-formula> depending on the theory.</p></list-item>
<list-item><p>&#x2218; Even for a system of free hypermultiplets it is not possible to turn on generic Wilson lines.</p></list-item>
<list-item><p>&#x2218; For systems with dynamical vector multiplets the formula does not reproduce the correct answer.</p></list-item>
</list></p>
<p>The second and third deficiencies may be related to each other. The incompatibility of the generic Wilson lines seems to prevent us from performing path integrals over all gauge field configurations. At present, we cannot claim anything definite for this point, and more investigation is desired. It is important to study more general systems to clarify to what extent our formula works and (if possible) how we should improve it to make it applicable to general systems. In particular, it would be interesting and important to study the orbifold Schur index of non-Lagrangian theories such as Argyres&#x2013;Douglas theories. Lagrangian theories that flow to a class of Argyres&#x2013;Douglas theories have been proposed in Refs. [<xref ref-type="bibr" rid="B25">25</xref>&#x2013;<xref ref-type="bibr" rid="B31">31</xref>], and this enables us to apply the UV formula of the orbifold index to the non-Lagrangian theories.</p>
<p>It is also interesting to analyze the relation between the orbifold index and chiral algebra. In the unorbifolded case, the chiral algebra is realized in a complex plane, which is identified by Weyl rescaling with <inline-formula><tex-math notation="LaTeX" id="ImEquation302"><![CDATA[$\boldsymbol{S}^1\times{\mathbb{R}}_t\subset \boldsymbol{S}^3\times{\mathbb{R}}_t$]]></tex-math></inline-formula>, where <inline-formula><tex-math notation="LaTeX" id="ImEquation303"><![CDATA[$\boldsymbol{S}^1$]]></tex-math></inline-formula> is the large circle in <inline-formula><tex-math notation="LaTeX" id="ImEquation304"><![CDATA[$\boldsymbol{S}^3$]]></tex-math></inline-formula> on which BPS particles are aligned. The Virasoro generators <inline-formula><tex-math notation="LaTeX" id="ImEquation305"><![CDATA[$L_0$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation306"><![CDATA[$\overline L_0$]]></tex-math></inline-formula> on the plane are related to the superconformal generators by
<disp-formula id="pty025-M46"><label>(46)</label><tex-math notation="LaTeX" id="Equation46"><![CDATA[
\begin{align}
L_0&=\frac{1}{2}(H+J+\overline J)=\frac{1}{2}(\mu_x+\mu_p)+\mu_q,\nonumber\\
\overline L_0&=\frac{1}{2}(H-J-\overline J-2R)=\frac{1}{2}(\mu_x+\mu_p).
\end{align}
]]></tex-math></disp-formula></p>
<p>For Schur operators with <inline-formula><tex-math notation="LaTeX" id="ImEquation307"><![CDATA[$\mu_x=\mu_p=0$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation308"><![CDATA[$\overline L_0=0$]]></tex-math></inline-formula> and the <inline-formula><tex-math notation="LaTeX" id="ImEquation309"><![CDATA[${\mathbb{Z}}_n$]]></tex-math></inline-formula> generator <inline-formula><tex-math notation="LaTeX" id="ImEquation310"><![CDATA[$g_n=\omega_n^{\mu_x-\mu_p+\mu_q}$]]></tex-math></inline-formula> is given by
<disp-formula id="pty025-M47"><label>(47)</label><tex-math notation="LaTeX" id="Equation47"><![CDATA[
\begin{align}
g_n
=
\omega_n^{L_0}.
\end{align}
]]></tex-math></disp-formula></p>
<p>Namely, this is the <inline-formula><tex-math notation="LaTeX" id="ImEquation311"><![CDATA[${\mathbb{Z}}_n$]]></tex-math></inline-formula> orbifold acting on the worldsheet. Therefore, in the context of the chiral algebra, the orbifolding should be regarded as the insertion of a twist operator at the origin. Such a relation is studied for an orbifold version of the Macdonald index in Ref. [<xref ref-type="bibr" rid="B24">24</xref>]. It would be interesting to do a similar analysis for the orbifold Schur index.</p>
</sec>
</body>
<back>
<ack><title>Acknowledgments</title>
<p>I would like to thank Hirotaka Kato for valuable discussions. This work was partially supported by Grant-in-Aid for Scientific Research (C) (No. 15K05044), Ministry of Education, Science and Culture, Japan.</p>
</ack>
<sec><title>Funding</title>
<p>Open Access funding: SCOAP<inline-formula><tex-math notation="LaTeX" id="ImEquation312"><![CDATA[$^3$]]></tex-math></inline-formula>.</p>
</sec>
<fn-group>
<title>Footnotes</title>
<fn id="FN1"><p><sup>1</sup> Our convention is different from the standard one used, for example, in Ref. [<xref ref-type="bibr" rid="B3">3</xref>]. The standard one is obtained from ours by the replacement <inline-formula><tex-math notation="LaTeX" id="ImEquation313"><![CDATA[$t\rightarrow t/q$]]></tex-math></inline-formula>, and then the Schur limit is given by <inline-formula><tex-math notation="LaTeX" id="ImEquation314"><![CDATA[$t\rightarrow q$]]></tex-math></inline-formula>, while in our convention the Schur limit is <inline-formula><tex-math notation="LaTeX" id="ImEquation315"><![CDATA[$t\rightarrow 1$]]></tex-math></inline-formula>.</p></fn>
<fn id="FN2"><p><sup>2</sup> The reason why <inline-formula><tex-math notation="LaTeX" id="ImEquation316"><![CDATA[$i_V$]]></tex-math></inline-formula> in Eq. (<xref ref-type="disp-formula" rid="pty025-M12">12</xref>) is not simply <inline-formula><tex-math notation="LaTeX" id="ImEquation317"><![CDATA[$i_{U(1)}\chi_{\rm adj}'$]]></tex-math></inline-formula> but <inline-formula><tex-math notation="LaTeX" id="ImEquation318"><![CDATA[$(i_{U(1)}-1)\chi_{\rm adj}'$]]></tex-math></inline-formula> is that we include the measure factor (Vandermonde determinant) in <inline-formula><tex-math notation="LaTeX" id="ImEquation319"><![CDATA[$i_V$]]></tex-math></inline-formula>. In other words, &#x201C;<inline-formula><tex-math notation="LaTeX" id="ImEquation320"><![CDATA[$-1$]]></tex-math></inline-formula>&#x201D; is the contribution of the Faddeev&#x2013;Popov ghost associated with constant gauge transformation over <inline-formula><tex-math notation="LaTeX" id="ImEquation321"><![CDATA[${\boldsymbol S}^3$]]></tex-math></inline-formula>.</p></fn>
<fn id="FN3"><p><sup>3</sup> In the literature, <inline-formula><tex-math notation="LaTeX" id="ImEquation322"><![CDATA[$q'$]]></tex-math></inline-formula> defined by <inline-formula><tex-math notation="LaTeX" id="ImEquation323"><![CDATA[$q'^{1/2}=-q^{1/2}$]]></tex-math></inline-formula> is often used and then the minus sign does not appear.</p></fn>
</fn-group>
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