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<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/pty112</article-id>
<article-id pub-id-type="publisher-id">pty112</article-id>
<article-id pub-id-type="arxiv">arXiv:1808.02701</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/B01</subject>
<subject>PTEP/B31</subject>
</subj-group>
</article-categories>
<title-group>
<article-title>A calculation of the gauge anomaly with the chiral overlap operator</article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author" corresp="yes">
<name><surname>Ago</surname><given-names>Taichi</given-names></name>
<xref ref-type="corresp" rid="COR1"/>
<email xlink:type="simple">ago@hep-th.phys.s.u-tokyo.ac.jp</email>
<xref ref-type="aff" rid="AFF1"/>
</contrib>
</contrib-group>
<aff id="AFF1">Department of Physics, University of Tokyo, Tokyo, Japan</aff>
<author-notes>
<corresp id="COR1">E-mail: <email>ago@hep-th.phys.s.u-tokyo.ac.jp</email></corresp>
</author-notes>
<pub-date pub-type="cover">
<month>11</month>
<year>2018</year>
</pub-date>
<pub-date pub-type="collection">
<day>01</day>
<month>11</month>
<year>2018</year>
</pub-date>
<pub-date pub-type="epub" iso-8601-date="2018-11-19">
<day>19</day>
<month>11</month>
<year>2018</year>
</pub-date>
<volume>2018</volume>
<issue>11</issue>
<elocation-id>113B01</elocation-id>
<history>
<date date-type="received">
<day>20</day>
<month>09</month>
<year>2018</year>
</date>
<date date-type="accepted">
<day>03</day>
<month>10</month>
<year>2018</year>
</date>
<date date-type="accepted">
<day>06</day>
<month>11</month>
<year>2018</year>
</date>
</history>
<permissions>
<copyright-statement>&#x00A9; The Author(s) 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="pty112.pdf"/>
<abstract abstract-type="abstract"><title>Abstract</title>
<p>We investigate the property of the effective action with the chiral overlap operator, which was derived by Grabowska and Kaplan. They proposed a lattice formulation of four-dimensional chiral gauge theory, which is derived from their domain-wall formulation. In this formulation, an extra dimension is introduced and the gauge field along the extra dimension is evolved by the gradient flow. The chiral overlap operator satisfies the Ginsparg&#x2013;Wilson relation and only depends on the gauge fields on the two boundaries. We start from the arbitrary even-dimensional chiral overlap operator. We treat the gauge fields on the two boundaries independently, and derive the general expression to calculate the gauge anomaly with the chiral overlap operator in the continuum limit. As a result, we show that the gauge anomalies with the chiral overlap operator in two, four, and six dimensions in the continuum limit are equivalent to those known in the continuum theory up to total derivatives.</p>
</abstract>
<kwd-group kwd-group-type="jel">
<kwd>B01</kwd>
<kwd>B31</kwd>
</kwd-group>
<counts>
<page-count count="12"/>
</counts>
</article-meta>
</front>
<body>
<sec sec-type="intro" id="SEC1">
<title>1. Introduction</title>
<p>It has been a long-standing problem to construct a gauge-invariant regularization for a chiral gauge theory. Grabowska and Kaplan proposed a formulation of the chiral gauge theory on the lattice [<xref ref-type="bibr" rid="B1">1</xref>], which is developed based on the idea of the domain-wall fermion proposed by Kaplan [<xref ref-type="bibr" rid="B2">2</xref>]. In the formulation of the domain-wall fermions an extra dimension is introduced, and the left-handed fermion is localized on one domain wall and the right-handed fermion is localized on the other domain wall. In this formulation, the left- and right-handed fermions are coupled with the same gauge field because the gauge field is constant along the extra dimension. Thus this formulation is vector-like. On the other hand, in the Grabowska&#x2013;Kaplan formulation the gauge field along the extra dimension is given by the gradient flow [<xref ref-type="bibr" rid="B3">3</xref>&#x2013;<xref ref-type="bibr" rid="B6">6</xref>],
<disp-formula id="pty112M1-1"><label>(1.1)</label><tex-math notation="LaTeX" id="Equation1"><![CDATA[
\begin{equation}
\partial_{s}\mathcal{A}_{\mu} = \mathcal{D}_{\nu}\mathcal{F}_{\nu\mu},\quad \mathcal{A}_{\mu}(x,0)
= A_{\mu}(x), \label{eq:flow}
\end{equation}
]]></tex-math></disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation1"><![CDATA[$\mathcal{A}_{\mu}(x,s)$]]></tex-math></inline-formula> is the solution of the flow equation of Eq. (<xref ref-type="disp-formula" rid="pty112M1-1">1.1</xref>), and <inline-formula><tex-math notation="LaTeX" id="ImEquation2"><![CDATA[$\mathcal{D}_{\mu} = \partial_{\mu} + [\mathcal{A}_{\mu},\ \cdot \ ]$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation3"><![CDATA[$\mathcal{F}_{\mu\nu}= \partial_{\mu}\mathcal{A}_{\nu} - \partial_{\nu}\mathcal{A}_{\mu} + [\mathcal{A}_{\mu},\mathcal{A}_{\nu}]$]]></tex-math></inline-formula> are the covariant derivative and the field strength constructed from <inline-formula><tex-math notation="LaTeX" id="ImEquation4"><![CDATA[$\mathcal{A}_{\mu}(x,s)$]]></tex-math></inline-formula>, respectively. In other words, the gauge field is modified along the extra dimension by the gradient flow from the gauge field <inline-formula><tex-math notation="LaTeX" id="ImEquation5"><![CDATA[$A$]]></tex-math></inline-formula> on one domain wall to <inline-formula><tex-math notation="LaTeX" id="ImEquation6"><![CDATA[$A_{\star}$]]></tex-math></inline-formula> on the other domain wall. This means that the left- and right-handed fermions are coupled with the gauge field differently. Thus their formulation is expected to be a non-perturbative formulation of a chiral gauge theory. Grabowska and Kaplan also formulated a four-dimensional effective theory from the formulation explained above and obtained the chiral overlap operator [<xref ref-type="bibr" rid="B7">7</xref>], which obeys the Ginsparg&#x2013;Wilson relation [<xref ref-type="bibr" rid="B8">8</xref>]. This operator only depends on the gauge fields <inline-formula><tex-math notation="LaTeX" id="ImEquation7"><![CDATA[$A$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation8"><![CDATA[$A_{\star}$]]></tex-math></inline-formula>, and in the tree-level continuum limit, the left-handed fermion is only coupled with <inline-formula><tex-math notation="LaTeX" id="ImEquation9"><![CDATA[$A$]]></tex-math></inline-formula> and the right-handed fermion is only coupled with <inline-formula><tex-math notation="LaTeX" id="ImEquation10"><![CDATA[$A_{\star}$]]></tex-math></inline-formula>. For recent works related to Refs. [<xref ref-type="bibr" rid="B1">1</xref>,<xref ref-type="bibr" rid="B7">7</xref>], see Refs. [<xref ref-type="bibr" rid="B9">9</xref>&#x2013;<xref ref-type="bibr" rid="B13">13</xref>].</p>
<p>The effective action of the <inline-formula><tex-math notation="LaTeX" id="ImEquation11"><![CDATA[$(2n+1)$]]></tex-math></inline-formula>-dimensional domain-wall fermion with the gauge field evolved by the gradient flow is composed of three parts: the effective action of the <inline-formula><tex-math notation="LaTeX" id="ImEquation12"><![CDATA[$2n$]]></tex-math></inline-formula>-dimensional left-handed fermion, the effective action of the <inline-formula><tex-math notation="LaTeX" id="ImEquation13"><![CDATA[$2n$]]></tex-math></inline-formula>-dimensional right-handed fermion, and the Chern&#x2013;Simons term which is induced by the heavy modes in the bulk. Since the gradient flow assures the gauge invariance of the theory, the effective action of the <inline-formula><tex-math notation="LaTeX" id="ImEquation14"><![CDATA[$(2n+1)$]]></tex-math></inline-formula>-dimensional domain-wall fermion itself is gauge invariant. However, the effective actions of the left- and right-handed fermions are not gauge invariant because of gauge anomalies. In other words, the Chern&#x2013;Simons term plays the role of cancelling out the gauge variation from the effective actions of the boundary modes.</p>
<p>If the formulation is free from gauge anomalies, the Chern&#x2013;Simons term vanishes. Moreover, as shown in the two-dimensional <inline-formula><tex-math notation="LaTeX" id="ImEquation15"><![CDATA[$\mathrm{U}(1)$]]></tex-math></inline-formula> gauge theory in Refs. [<xref ref-type="bibr" rid="B1">1</xref>,<xref ref-type="bibr" rid="B7">7</xref>], the gauge field is expected to be evolved into a pure gauge so that the right-handed fermion on the other domain wall does not interact with the physical degrees of freedom of the gauge field. Thus we expect that the <inline-formula><tex-math notation="LaTeX" id="ImEquation16"><![CDATA[$(2n+1)$]]></tex-math></inline-formula>-dimensional domain-wall fermion with the gauge field evolved by the gradient flow results in a <inline-formula><tex-math notation="LaTeX" id="ImEquation17"><![CDATA[$2n$]]></tex-math></inline-formula>-dimensional effective theory in which only the left-handed fermion couples to the physical degrees of freedom of the gauge field.</p>
<p>In the lattice theory, we expect the same structure of the effective action in the continuum limit. The effective action constructed from the chiral overlap operator is composed of three parts: the functional of the gauge field <inline-formula><tex-math notation="LaTeX" id="ImEquation18"><![CDATA[$A$]]></tex-math></inline-formula>, the functional of the gauge field <inline-formula><tex-math notation="LaTeX" id="ImEquation19"><![CDATA[$A_{\star}$]]></tex-math></inline-formula>, and the cross terms of the gauge fields <inline-formula><tex-math notation="LaTeX" id="ImEquation20"><![CDATA[$A$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation21"><![CDATA[$A_{\star}$]]></tex-math></inline-formula>. This effective action is gauge invariant under the simultaneous gauge transformation of <inline-formula><tex-math notation="LaTeX" id="ImEquation22"><![CDATA[$A$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation23"><![CDATA[$A_{\star}$]]></tex-math></inline-formula>. In the case of four-dimensional effective theories, the cross terms of the gauge fields <inline-formula><tex-math notation="LaTeX" id="ImEquation24"><![CDATA[$A$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation25"><![CDATA[$A_{\star}$]]></tex-math></inline-formula> were calculated in the continuum limit and it was confirmed that the parity-odd part of the gauge variation of the functional of the gauge field <inline-formula><tex-math notation="LaTeX" id="ImEquation26"><![CDATA[$A$]]></tex-math></inline-formula> coincides with the gauge anomaly known in the continuum theory [<xref ref-type="bibr" rid="B12">12</xref>].</p>
<p>In order to confirm the correspondence of the structures of the effective actions between the formulation of the domain-wall fermion and the chiral overlap operator, we generalize this result; i.e., we calculate the gauge variation of the functional of the gauge field <inline-formula><tex-math notation="LaTeX" id="ImEquation27"><![CDATA[$A$]]></tex-math></inline-formula> for an arbitrary even-dimensional effective action of the chiral overlap operator in the continuum limit, and explicitly check that the parity-odd part indeed coincides with the gauge anomaly in the continuum theory in the case of two, four, and six dimensions.</p>
</sec>
<sec id="SEC2"><title>2. Notation and convention</title>
<p>In Ref. [<xref ref-type="bibr" rid="B7">7</xref>], the chiral overlap operator is defined through the transfer matrix which depends on the flow time due to the <inline-formula><tex-math notation="LaTeX" id="ImEquation28"><![CDATA[$s$]]></tex-math></inline-formula>-dependence of the gauge field. They consider the simplification that the gauge field is constant in the half of the interval <inline-formula><tex-math notation="LaTeX" id="ImEquation29"><![CDATA[$[0, L]$]]></tex-math></inline-formula> near the <inline-formula><tex-math notation="LaTeX" id="ImEquation30"><![CDATA[$s=0$]]></tex-math></inline-formula> boundary and is <inline-formula><tex-math notation="LaTeX" id="ImEquation31"><![CDATA[$A_{\star}$]]></tex-math></inline-formula> in the remaining region. <inline-formula><tex-math notation="LaTeX" id="ImEquation32"><![CDATA[$L$]]></tex-math></inline-formula> is the length of the extra dimension and in the large-<inline-formula><tex-math notation="LaTeX" id="ImEquation33"><![CDATA[$L$]]></tex-math></inline-formula> limit the effective theory for the boundary modes is obtained. In this case, the chiral overlap operator in arbitrary even dimensions is expressed as follows:
<disp-formula id="pty112M2-1"><label>(2.1)</label><tex-math notation="LaTeX" id="Equation2"><![CDATA[
\begin{equation}
a\hat{D}_{\chi} = 1+\gamma_{d+1}\left[1-(1-\epsilon_{\star})\frac{1}{1+\epsilon\epsilon_{\star}}(1-\epsilon)\right].
\end{equation}
]]></tex-math></disp-formula></p>
<p>Here, <inline-formula><tex-math notation="LaTeX" id="ImEquation34"><![CDATA[$\epsilon$]]></tex-math></inline-formula> is the sign function,
<disp-formula id="pty112M2-2"><label>(2.2)</label><tex-math notation="LaTeX" id="Equation3"><![CDATA[
\begin{equation}
\epsilon = H_{\mathrm{W}}[A]\left(H_{\mathrm{W}}[A]^2\right)^{-1/2}, \label{eq:epsilon}
\end{equation}
]]></tex-math></disp-formula>
of the Hermitian Wilson Dirac operator,
<disp-formula id="pty112M2-3"><label>(2.3)</label><tex-math notation="LaTeX" id="Equation4"><![CDATA[
\begin{equation}
H_{\mathrm{W}}[A] = \gamma_{d+1} \left\{\frac{1}{2}\left[\sum_{\mu}\gamma_{\mu}(\nabla^{*}_{\mu}[A] + \nabla_{\mu}[A]) -ar\sum_{\mu} \nabla^{*}_{\mu}[A]\nabla_{\mu}[A]\right] - M_0/a \right\}\!, \label{eq:HWDO}
\end{equation}
]]></tex-math></disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation35"><![CDATA[$a$]]></tex-math></inline-formula> is the lattice spacing, and <inline-formula><tex-math notation="LaTeX" id="ImEquation36"><![CDATA[$M_0$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation37"><![CDATA[$r$]]></tex-math></inline-formula> are free parameters. <inline-formula><tex-math notation="LaTeX" id="ImEquation38"><![CDATA[$\epsilon_{\star}$]]></tex-math></inline-formula> is also defined by replacing the gauge field <inline-formula><tex-math notation="LaTeX" id="ImEquation39"><![CDATA[$A$]]></tex-math></inline-formula> with <inline-formula><tex-math notation="LaTeX" id="ImEquation40"><![CDATA[$A_{\star}$]]></tex-math></inline-formula>, which is obtained from the original gauge field <inline-formula><tex-math notation="LaTeX" id="ImEquation41"><![CDATA[$A$]]></tex-math></inline-formula> according to the gradient flow equation, Eq. (<xref ref-type="disp-formula" rid="pty112M1-1">1.1</xref>). Here we consider Euclidean arbitrary even dimensions <inline-formula><tex-math notation="LaTeX" id="ImEquation42"><![CDATA[$d=2n$]]></tex-math></inline-formula>. Gamma matrices satisfy the following equations:
<disp-formula id="pty112M2-4"><label>(2.4)</label><tex-math notation="LaTeX" id="Equation5"><![CDATA[
\begin{equation}
\gamma_{\mu}^{\dagger} = \gamma_{\mu},\quad \{ \gamma_{\mu}, \gamma_{\nu} \} = 2\delta_{\mu \nu},\quad \gamma_{d+1} = i^n \gamma_1 \cdots \gamma_{d}. \label{def:gamma}
\end{equation}
]]></tex-math></disp-formula></p>
<p>The Greek letters, <inline-formula><tex-math notation="LaTeX" id="ImEquation43"><![CDATA[$\mu,\nu,\ldots$]]></tex-math></inline-formula>, run from <inline-formula><tex-math notation="LaTeX" id="ImEquation44"><![CDATA[$1$]]></tex-math></inline-formula> to <inline-formula><tex-math notation="LaTeX" id="ImEquation45"><![CDATA[$2n$]]></tex-math></inline-formula>. Therefore,
<disp-formula id="pty112M2-5"><label>(2.5)</label><tex-math notation="LaTeX" id="Equation6"><![CDATA[
\begin{equation}
\gamma_{d+1}^{\dagger} = \gamma_{d+1},\quad (\gamma_{d+1})^2 = 1,\quad {\mathop{\mathrm{tr}}\nolimits} \gamma_{d+1}\gamma_{\mu_1}\cdots \gamma_{\mu_d} = (-i)^n2^n\epsilon_{\mu_1 \cdots \mu_{d}}
\end{equation}
]]></tex-math></disp-formula>
follow from Eq. (<xref ref-type="disp-formula" rid="pty112M2-4">2.4</xref>). <inline-formula><tex-math notation="LaTeX" id="ImEquation46"><![CDATA[$\nabla_{\mu}$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation47"><![CDATA[$\nabla^{*}_{\mu}$]]></tex-math></inline-formula> are the forward and backward lattice covariant derivatives, respectively, which are defined as
<disp-formula id="pty112M2-6"><label>(2.6)</label><tex-math notation="LaTeX" id="Equation7"><![CDATA[
\begin{align}
\nabla_{\mu}[A]f(x) &= \frac{1}{a}\left[ U(x,\mu)[A]f(x+a\hat{\mu})- f(x) \right], \\
\end{align}
]]></tex-math></disp-formula>
<disp-formula id="pty112M2-7"><label>(2.7)</label><tex-math notation="LaTeX" id="Equation8"><![CDATA[
\begin{align}
\nabla^{*}_{\mu}[A]f(x) &= \frac{1}{a}\left[ f(x)-U^{\dagger}[A](x-a\hat{\mu},\mu) f(x-a\hat{\mu}) \right].
\end{align}
]]></tex-math></disp-formula></p>
<p>The generators <inline-formula><tex-math notation="LaTeX" id="ImEquation48"><![CDATA[$T^a\, (a=1,\ldots, \mathop{\mathrm{dim}}\nolimits \mathcal{G})$]]></tex-math></inline-formula> of the gauge group <inline-formula><tex-math notation="LaTeX" id="ImEquation49"><![CDATA[$\mathcal{G}$]]></tex-math></inline-formula> satisfy the following equations:
<disp-formula id="pty112M2-8"><label>(2.8)</label><tex-math notation="LaTeX" id="Equation9"><![CDATA[
\begin{equation}
(T^a)^{\dagger}=-T^a,\quad [T^a,T^b] = f^{abc}T^c,\quad {\mathop{\mathrm{tr}}\nolimits} T^aT^b = -1/2\delta^{ab}.
\end{equation}
]]></tex-math></disp-formula></p>
<p>Here the covariant derivative is defined as <inline-formula><tex-math notation="LaTeX" id="ImEquation50"><![CDATA[$D_{\mu}=\partial_{\mu} + A_{\mu}$]]></tex-math></inline-formula>, where <inline-formula><tex-math notation="LaTeX" id="ImEquation51"><![CDATA[$A_{\mu} = A^a_{\mu}T^a$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation52"><![CDATA[$A^a_{\mu}$]]></tex-math></inline-formula> is real. Thus, by defining the link variable as
<disp-formula id="pty112M2-9"><label>(2.9)</label><tex-math notation="LaTeX" id="Equation10"><![CDATA[
\begin{equation}
U(x,\mu)[A] = \mathcal{P}\exp\left[ a\int_0^1 {d} t\, A_{\mu}(x+ta\hat{\mu}) \right],
\end{equation}
]]></tex-math></disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation53"><![CDATA[$\mathcal{P}$]]></tex-math></inline-formula> denotes the path-ordered product and <inline-formula><tex-math notation="LaTeX" id="ImEquation54"><![CDATA[$\hat{\mu}$]]></tex-math></inline-formula> is the unit vector in the direction <inline-formula><tex-math notation="LaTeX" id="ImEquation55"><![CDATA[$\mu$]]></tex-math></inline-formula>, we obtain
<disp-formula id="pty112M2-10"><label>(2.10)</label><tex-math notation="LaTeX" id="Equation11"><![CDATA[
\begin{align}
\nabla_{\mu}[A]f(x) &= (D_{\mu} + \mathcal{O}(a))f(x), \\
\end{align}
]]></tex-math></disp-formula>
<disp-formula id="pty112M2-11"><label>(2.11)</label><tex-math notation="LaTeX" id="Equation12"><![CDATA[
\begin{align}
\nabla^{*}_{\mu}[A]f(x) &= (D_{\mu} + \mathcal{O}(a))f(x)
\end{align}
]]></tex-math></disp-formula>
in the continuum limit <inline-formula><tex-math notation="LaTeX" id="ImEquation56"><![CDATA[$a \rightarrow 0$]]></tex-math></inline-formula>. In Ref. [<xref ref-type="bibr" rid="B12">12</xref>], the fermion one-loop effective action defined by
<disp-formula id="pty112M2-12"><label>(2.12)</label><tex-math notation="LaTeX" id="Equation13"><![CDATA[
\begin{equation}
\Gamma_{\mathrm{lat.}}[A,A_{\star}]\equiv - \ln \int \prod_{x} [{d} \psi(x){d} \bar{\psi}(x)]\, \exp \left[ -a^d\sum_{x}\bar{\psi}(x)\hat{D}_{\chi}\psi(x) \right]
\end{equation}
]]></tex-math></disp-formula>
is studied and the following expression is obtained:
<disp-formula id="pty112M2-13"><label>(2.13)</label><tex-math notation="LaTeX" id="Equation14"><![CDATA[
\begin{equation}
\delta\delta_{\star} \Gamma_{\mathrm{lat.}}[A,A_{\star}] = -\frac{1}{2}{\mathop{\mathrm{Tr}}\nolimits} ( 1 - \epsilon_{\star} )\frac{1}{\epsilon + \epsilon_{\star}}\delta \epsilon \frac{1}{\epsilon + \epsilon_{\star}}\delta_{\star}\epsilon_{\star}, \label{eq:DVoEA}
\end{equation}
]]></tex-math></disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation57"><![CDATA[${\mathop{\mathrm{Tr}}\nolimits} \equiv \sum_x {\mathop{\mathrm{tr}}\nolimits}$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation58"><![CDATA[${\mathop{\mathrm{tr}}\nolimits}$]]></tex-math></inline-formula> denotes the trace over the spinor and gauge indices. <inline-formula><tex-math notation="LaTeX" id="ImEquation59"><![CDATA[$\delta$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation60"><![CDATA[$\delta_{\star}$]]></tex-math></inline-formula> are the infinitesimal variations which only act on <inline-formula><tex-math notation="LaTeX" id="ImEquation61"><![CDATA[$A$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation62"><![CDATA[$A_{\star}$]]></tex-math></inline-formula>, respectively:
<disp-formula id="pty112M2-14"><label>(2.14)</label><tex-math notation="LaTeX" id="Equation15"><![CDATA[
\begin{align}
\delta A &\not= 0,\quad \delta A_{\star} = 0, \\
\end{align}
]]></tex-math></disp-formula>
<disp-formula id="pty112M2-15"><label>(2.15)</label><tex-math notation="LaTeX" id="Equation16"><![CDATA[
\begin{align}
\delta_{\star} A_{\star} &\not= 0,\quad \delta_{\star} A=0.
\end{align}
]]></tex-math></disp-formula></p>
<p>Here, we treat the gauge fields <inline-formula><tex-math notation="LaTeX" id="ImEquation63"><![CDATA[$A$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation64"><![CDATA[$A_{\star}$]]></tex-math></inline-formula> independently, and the infinitesimal variations <inline-formula><tex-math notation="LaTeX" id="ImEquation65"><![CDATA[$\delta$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation66"><![CDATA[$\delta_{\star}$]]></tex-math></inline-formula> are independent.<xref ref-type="fn" rid="FN1"><sup>1</sup></xref> Equation (<xref ref-type="disp-formula" rid="pty112M2-13">2.13</xref>) is decomposed into the parity-odd and parity-even parts. The former is written as
<disp-formula id="pty112M2-16"><label>(2.16)</label><tex-math notation="LaTeX" id="Equation17"><![CDATA[
\begin{align}
(\text{parity-odd part}) &= \frac{1}{2}{\mathop{\mathrm{Tr}}\nolimits}\epsilon_{\star}\frac{1}{\epsilon+\epsilon_{\star}}\delta\epsilon\frac{1}{\epsilon+\epsilon_{\star}}\delta_{\star}\epsilon_{\star} \\
\end{align}
]]></tex-math></disp-formula>
<disp-formula id="pty112M2-17"><label>(2.17)</label><tex-math notation="LaTeX" id="Equation18"><![CDATA[
\begin{align}
&=-\frac{1}{2}\delta\left( {\mathop{\mathrm{Tr}}\nolimits}\epsilon_{\star}\frac{1}{\epsilon+\epsilon_{\star}}\delta_{\star}\epsilon_{\star} \right)\!,
\end{align}
]]></tex-math></disp-formula>
and the latter is written as
<disp-formula id="pty112M2-18"><label>(2.18)</label><tex-math notation="LaTeX" id="Equation19"><![CDATA[
\begin{align}
(\text{parity-even part}) &= -\frac{1}{2}{\mathop{\mathrm{Tr}}\nolimits}\frac{1}{\epsilon+\epsilon_{\star}}\delta\epsilon\frac{1}{\epsilon+\epsilon_{\star}}\delta_{\star}\epsilon_{\star} \\
\end{align}
]]></tex-math></disp-formula>
<disp-formula id="pty112M2-19"><label>(2.19)</label><tex-math notation="LaTeX" id="Equation20"><![CDATA[
\begin{align}
&=\frac{1}{2}\delta\delta_{\star}{\mathop{\mathrm{Tr}}\nolimits}\ln(\epsilon +\epsilon_{\star}).
\end{align}
]]></tex-math></disp-formula></p>
<p>By expressing the infinitesimal gauge transformation as
<disp-formula id="pty112M2-20"><label>(2.20)</label><tex-math notation="LaTeX" id="Equation21"><![CDATA[
\begin{alignat}{2}
\delta^{\omega} A_{\mu}(x) &= \partial_{\mu}\omega(x) + [ A_{\mu}(x) , \omega(x) ], &\qquad \delta^{\omega} {A_{\star}}_{\mu}(x) &= 0, \label{eq:gaugetrans_A} \\
\end{alignat}
]]></tex-math></disp-formula>
<disp-formula id="pty112M2-21"><label>(2.21)</label><tex-math notation="LaTeX" id="Equation22"><![CDATA[
\begin{alignat}{2}
\delta^{\omega}_{\star} {A_{\star}}_{\mu}(x) &= \partial_{\mu}\omega(x) + [ {A_{\star}}_{\mu}(x) , \omega(x) ], & \delta^{\omega}_{\star} A_{\mu}(x) &= 0, \label{eq:gaugetrans_Astar}
\end{alignat}
]]></tex-math></disp-formula>
and using the equations
<disp-formula id="pty112M2-22"><label>(2.22)</label><tex-math notation="LaTeX" id="Equation23"><![CDATA[
\begin{align}
(\delta^{\omega}+\delta_{\star}^{\omega})\Gamma_{\mathrm{lat.}}[A,A_{\star}] &= 0, \\
\end{align}
]]></tex-math></disp-formula>
<disp-formula id="pty112M2-23"><label>(2.23)</label><tex-math notation="LaTeX" id="Equation24"><![CDATA[
\begin{align}
(\delta^{\omega}+\delta_{\star}^{\omega}){\mathop{\mathrm{Tr}}\nolimits}\ln(\epsilon +\epsilon_{\star}) &= 0,
\end{align}
]]></tex-math></disp-formula>
we obtain the following equation which is related to the gauge anomaly:
<disp-formula id="pty112M2-24"><label>(2.24)</label><tex-math notation="LaTeX" id="Equation25"><![CDATA[
\begin{equation}
\delta^{\omega}\Gamma_{\mathrm{lat.}}[A,0] = \frac{1}{2} {\mathop{\mathrm{Tr}}\nolimits}\epsilon_{\star}\frac{1}{\epsilon+\epsilon_{\star}}\delta_{\star}^{\omega}\epsilon_{\star}[A,0] + \frac{1}{2}\delta^{\omega} {\mathop{\mathrm{Tr}}\nolimits}\ln(\epsilon +\epsilon_{\star})[A,0]. \label{eq:Gamma_lat}
\end{equation}
]]></tex-math></disp-formula></p>
<p>The parity-even part can be removed by local counterterms. As discussed in Ref. [<xref ref-type="bibr" rid="B12">12</xref>] for <inline-formula><tex-math notation="LaTeX" id="ImEquation67"><![CDATA[$d=4$]]></tex-math></inline-formula>, the parity-even part contains a mass term of the gauge field even if the anomaly-free condition is satisfied, and this part should be subtracted by local counterterms.</p>
</sec>
<sec id="SEC3"><title>3. Calculation of the gauge anomaly</title>
<p>In this section, we evaluate the parity-odd part following Ref. [<xref ref-type="bibr" rid="B14">14</xref>], in which the axial anomaly <inline-formula><tex-math notation="LaTeX" id="ImEquation68"><![CDATA[$-1/(2a^d){\mathop{\mathrm{tr}}\nolimits} \epsilon (x,x)$]]></tex-math></inline-formula> defined by the overlap operator is calculated in the continuum limit for arbitrary even dimensions. By expanding the parity-odd part of Eq. (<xref ref-type="disp-formula" rid="pty112M2-24">2.24</xref>) in powers of <inline-formula><tex-math notation="LaTeX" id="ImEquation69"><![CDATA[$\Delta \equiv \epsilon - \epsilon_{\star}= \mathcal{O}(a)$]]></tex-math></inline-formula>, we obtain the following equations:
<disp-formula id="pty112M3-1"><label>(3.1)</label><tex-math notation="LaTeX" id="Equation26"><![CDATA[
\begin{align}
\frac{1}{2} {\mathop{\mathrm{Tr}}\nolimits}\epsilon_{\star}\frac{1}{\epsilon+\epsilon_{\star}}\delta_{\star}^{\omega}\epsilon_{\star}[A,0]
&= \left.a^d\sum_{x}\frac{1}{2a^d}{\mathop{\mathrm{tr}}\nolimits} \epsilon_{\star}(\epsilon+\epsilon_{\star})\frac{1}{(\epsilon+\epsilon_{\star})^2}\delta_{\star}^{\omega}\epsilon_{\star}\right|_{A_{\star}=0}(x,x) \nonumber \\
&= \left.a^d\sum_{x}\frac{1}{2a^d}{\mathop{\mathrm{tr}}\nolimits} \epsilon_{\star}(2\epsilon_{\star}+\Delta)\frac{1}{4-\Delta^2}\delta_{\star}^{\omega}\epsilon_{\star}\right|_{A_{\star}=0}(x,x) \nonumber \\
&= \left.a^d\sum_{x}\frac{1}{4a^d}{\mathop{\mathrm{tr}}\nolimits} \left[\sum_{\ell=0}^{\infty}(\Delta/2)^{2\ell}+\epsilon_{\star}\sum_{\ell=0}^{\infty}(\Delta/2)^{2\ell+1}\right]\delta_{\star}^{\omega}\epsilon_{\star}\right|_{A_{\star}=0}(x,x).
\end{align}
]]></tex-math></disp-formula></p>
<p>Since <inline-formula><tex-math notation="LaTeX" id="ImEquation70"><![CDATA[$a^d \sum_x \rightarrow \int {d}^d x$]]></tex-math></inline-formula>, we only need to calculate <inline-formula><tex-math notation="LaTeX" id="ImEquation71"><![CDATA[$\mathcal{O}(a^m)$]]></tex-math></inline-formula> terms with <inline-formula><tex-math notation="LaTeX" id="ImEquation72"><![CDATA[$m \leq d$]]></tex-math></inline-formula> in the trace of
<disp-formula id="pty112M3-2"><label>(3.2)</label><tex-math notation="LaTeX" id="Equation27"><![CDATA[
\begin{equation}
\mathcal{A}_{\mathrm{gauge}}(x) \equiv \left.\frac{1}{4a^d}{\mathop{\mathrm{tr}}\nolimits} \left[\sum_{\ell=0}^{\infty}(\Delta/2)^{2\ell}+\epsilon_{\star}\sum_{\ell=0}^{\infty}(\Delta/2)^{2\ell+1}\right]\delta_{\star}^{\omega}\epsilon_{\star}\right|_{A_{\star}=0}(x,x). \label{eq:gauge-anomaly}
\end{equation}
]]></tex-math></disp-formula></p>
<p>From Eqs. (<xref ref-type="disp-formula" rid="pty112M2-2">2.2</xref>) and (<xref ref-type="disp-formula" rid="pty112M2-3">2.3</xref>), it is clear that <inline-formula><tex-math notation="LaTeX" id="ImEquation73"><![CDATA[$\epsilon$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation74"><![CDATA[$\epsilon_{\star}$]]></tex-math></inline-formula> contain one <inline-formula><tex-math notation="LaTeX" id="ImEquation75"><![CDATA[$\gamma_{d+1}$]]></tex-math></inline-formula>. Thus, the <inline-formula><tex-math notation="LaTeX" id="ImEquation76"><![CDATA[$\gamma_{d+1}$]]></tex-math></inline-formula>s appear an odd number of times in all of the terms of Eq. (<xref ref-type="disp-formula" rid="pty112M3-2">3.2</xref>), and these terms are reduced to the form that contains the factor <inline-formula><tex-math notation="LaTeX" id="ImEquation77"><![CDATA[${\mathop{\mathrm{tr}}\nolimits} \gamma_{d+1}\gamma_{\mu_1}\cdots \gamma_{\mu_m}$]]></tex-math></inline-formula>, which is zero if <inline-formula><tex-math notation="LaTeX" id="ImEquation78"><![CDATA[$m < d$]]></tex-math></inline-formula>. Therefore, we only need to take account of the terms in which the <inline-formula><tex-math notation="LaTeX" id="ImEquation79"><![CDATA[$\gamma_{\mu}$]]></tex-math></inline-formula>s appear at least <inline-formula><tex-math notation="LaTeX" id="ImEquation80"><![CDATA[$d$]]></tex-math></inline-formula> times. Note that a diagonal element of the kernel of an operator <inline-formula><tex-math notation="LaTeX" id="ImEquation81"><![CDATA[$\mathcal{O}$]]></tex-math></inline-formula> on the lattice is calculated from
<disp-formula id="pty112M3-3"><label>(3.3)</label><tex-math notation="LaTeX" id="Equation28"><![CDATA[
\begin{equation}
\mathcal{O}(x,x) = \int_{\mathcal{B}^d} \frac{{d}^d k}{(2\pi)^d}\, e^{-ikx/a}(\mathcal{O}e^{ikx/a}),
\end{equation}
]]></tex-math></disp-formula>
where
<disp-formula id="pty112M3-4"><label>(3.4)</label><tex-math notation="LaTeX" id="Equation29"><![CDATA[
\begin{equation}
\mathcal{B}^d \equiv \left\{\, (k_1, \ldots, k_d)\in \mathbb{R}^d \, \big|\, -\pi \leq k_{\mu} \leq \pi,\ \forall \mu \in \{1,\ldots,d\} \,\right\}\!.
\end{equation}
]]></tex-math></disp-formula></p>
<p>From Eqs. (<xref ref-type="disp-formula" rid="pty112M2-2">2.2</xref>) and (<xref ref-type="disp-formula" rid="pty112M2-3">2.3</xref>), we obtain
<disp-formula id="pty112M3-5"><label>(3.5)</label><tex-math notation="LaTeX" id="Equation30"><![CDATA[
\begin{equation}
\epsilon e^{ikx/a} f(x) =e^{ikx/a} \gamma_{d+1}\left[(V + aS^{-1}P_1)\sum_{\ell=0}^{\infty} a^{2\ell}\alpha_{2\ell}S^{-2\ell}P_2^{\ell} + \cdots \right]f(x), \label{eq:epsilon_obtained}
\end{equation}
]]></tex-math></disp-formula>
where the ellipsis denotes the terms which do not contribute to Eq. (<xref ref-type="disp-formula" rid="pty112M3-2">3.2</xref>) in the continuum limit for the reason explained later. The expressions that appear in Eq. (<xref ref-type="disp-formula" rid="pty112M3-5">3.5</xref>) are defined as follows:
<disp-formula id="pty112M3-6"><label>(3.6)</label><tex-math notation="LaTeX" id="Equation31"><![CDATA[
\begin{align}
S &= \left( \sum_{\nu}s_{\nu}^2 + M^2 \right)^{1/2}, \\
\end{align}
]]></tex-math></disp-formula>
<disp-formula id="pty112M3-7"><label>(3.7)</label><tex-math notation="LaTeX" id="Equation32"><![CDATA[
\begin{align}
V &= \left(\sum_{\mu}\gamma_{\mu}is_{\mu} - M \right)S^{-1}, \\
\end{align}
]]></tex-math></disp-formula>
<disp-formula id="pty112M3-8"><label>(3.8)</label><tex-math notation="LaTeX" id="Equation33"><![CDATA[
\begin{align}
P_1 &= \sum_{\mu}\gamma_{\mu} c_{\mu}D_{\mu} - r\sum_{\mu} is_{\mu}D_{\mu}, \label{eq:P_1}\\
\end{align}
]]></tex-math></disp-formula>
<disp-formula id="pty112M3-9"><label>(3.9)</label><tex-math notation="LaTeX" id="Equation34"><![CDATA[
\begin{align}
P_2 &= \frac{1}{2}\sum_{\nu,\rho}\gamma_{\nu}\gamma_{\rho}c_{\nu}c_{\rho}F_{\nu\rho} - r\sum_{\nu,\rho}\gamma_{\nu}c_{\nu} is_{\rho}F_{\nu\rho}, \label{eq:P_2}
\end{align}
]]></tex-math></disp-formula>
where
<disp-formula id="pty112M3-10"><label>(3.10)</label><tex-math notation="LaTeX" id="Equation35"><![CDATA[
\begin{equation}
s_{\mu} = \sin k_{\mu},\quad c_{\mu} = \cos k_{\mu},
\end{equation}
]]></tex-math></disp-formula>
<disp-formula id="pty112M3-11"><label>(3.11)</label><tex-math notation="LaTeX" id="Equation36"><![CDATA[
\begin{equation}
M = M_0 + r\sum_{\rho}(c_{\rho}-1),
\end{equation}
]]></tex-math></disp-formula>
and <inline-formula><tex-math notation="LaTeX" id="ImEquation82"><![CDATA[$F_{\mu\nu} = [D_{\mu},D_{\nu}]=\partial_{\mu}A_{\nu}-\partial_{\nu}A_{\mu} + [A_{\mu},A_{\nu}]$]]></tex-math></inline-formula> denotes the field strength of the gauge field <inline-formula><tex-math notation="LaTeX" id="ImEquation83"><![CDATA[$A_{\mu}(x)$]]></tex-math></inline-formula>. <inline-formula><tex-math notation="LaTeX" id="ImEquation84"><![CDATA[$\alpha_{2\ell}$]]></tex-math></inline-formula> is defined as the coefficient of <inline-formula><tex-math notation="LaTeX" id="ImEquation85"><![CDATA[$z^{2\ell}$]]></tex-math></inline-formula> in the power series of <inline-formula><tex-math notation="LaTeX" id="ImEquation86"><![CDATA[$(1-z^2)^{-1/2}$]]></tex-math></inline-formula>; that is, <inline-formula><tex-math notation="LaTeX" id="ImEquation87"><![CDATA[$(1-z^2)^{-1/2} = \sum_{\ell} \alpha_{2\ell}z^{2\ell}$]]></tex-math></inline-formula>, and the explicit form of <inline-formula><tex-math notation="LaTeX" id="ImEquation88"><![CDATA[$\alpha_{2\ell}$]]></tex-math></inline-formula> is given as follows:
<disp-formula id="pty112M3-12"><label>(3.12)</label><tex-math notation="LaTeX" id="Equation37"><![CDATA[
\begin{equation}
\alpha_{2\ell} = \frac{1}{\ell!} \frac{\Gamma(\ell+1/2)}{\Gamma(1/2)}.
\end{equation}
]]></tex-math></disp-formula></p>
<p>Since we have <inline-formula><tex-math notation="LaTeX" id="ImEquation89"><![CDATA[$P_2=0$]]></tex-math></inline-formula> if <inline-formula><tex-math notation="LaTeX" id="ImEquation90"><![CDATA[$A_{\mu}=0$]]></tex-math></inline-formula>, we obtain the following expressions:
<disp-formula id="pty112M3-13"><label>(3.13)</label><tex-math notation="LaTeX" id="Equation38"><![CDATA[
\begin{align}
\left.\epsilon_{\star}\right|_{A_{\star}=0}e^{ikx/a} f(x) &= e^{ikx/a}\gamma_{d+1}(V + aS^{-1}P_1|_{A=0} + \cdots)f(x), \label{eq:epsilon-star} \\
\end{align}
]]></tex-math></disp-formula>
<disp-formula id="pty112M3-14"><label>(3.14)</label><tex-math notation="LaTeX" id="Equation39"><![CDATA[
\begin{align}
\left.\delta_{\star}^{\omega}\epsilon_{\star}\right|_{A_{\star}=0}e^{ikx/a} f(x) &= e^{ikx/a}\gamma_{d+1} (aS^{-1}\delta^{\omega} P_1|_{A=0} + \cdots)f(x), \label{eq:delta-epsilon-star}
\end{align}
]]></tex-math></disp-formula>
and
<disp-formula id="pty112M3-15"><label>(3.15)</label><tex-math notation="LaTeX" id="Equation40"><![CDATA[
\begin{align}
&\left.\Delta \right|_{A_{\star}=0}e^{ikx/a}f(x) \nonumber\\
&=e^{ikx/a} \gamma_{d+1}\left[aS^{-1}( P_1-P_1|_{A=0}) +(V + aS^{-1}P_1) \sum_{\ell=1}^{\infty} a^{2\ell}\alpha_{2\ell}S^{-2\ell}P_2^{\ell}+ \cdots\right] f(x). \label{eq:Delta}
\end{align}
]]></tex-math></disp-formula></p>
<p>The number of <inline-formula><tex-math notation="LaTeX" id="ImEquation91"><![CDATA[$\gamma_{\mu}$]]></tex-math></inline-formula>s for each of the <inline-formula><tex-math notation="LaTeX" id="ImEquation92"><![CDATA[$a^{m}$]]></tex-math></inline-formula> terms in Eqs. (<xref ref-type="disp-formula" rid="pty112M3-13">3.13</xref>), (<xref ref-type="disp-formula" rid="pty112M3-14">3.14</xref>), and (<xref ref-type="disp-formula" rid="pty112M3-15">3.15</xref>) is less than or equal to <inline-formula><tex-math notation="LaTeX" id="ImEquation93"><![CDATA[$m$]]></tex-math></inline-formula>, except for the terms which contain <inline-formula><tex-math notation="LaTeX" id="ImEquation94"><![CDATA[$V$]]></tex-math></inline-formula>s. On the other hand, the maximum number of <inline-formula><tex-math notation="LaTeX" id="ImEquation95"><![CDATA[$\gamma_{\mu}$]]></tex-math></inline-formula>s for the <inline-formula><tex-math notation="LaTeX" id="ImEquation96"><![CDATA[$a^{m}$]]></tex-math></inline-formula> terms that contain <inline-formula><tex-math notation="LaTeX" id="ImEquation97"><![CDATA[$V$]]></tex-math></inline-formula>s is <inline-formula><tex-math notation="LaTeX" id="ImEquation98"><![CDATA[$m+1$]]></tex-math></inline-formula>. Therefore, in the <inline-formula><tex-math notation="LaTeX" id="ImEquation99"><![CDATA[$a^{p}$]]></tex-math></inline-formula> terms in Eq. (<xref ref-type="disp-formula" rid="pty112M3-2">3.2</xref>) where <inline-formula><tex-math notation="LaTeX" id="ImEquation100"><![CDATA[$V$]]></tex-math></inline-formula>s appear <inline-formula><tex-math notation="LaTeX" id="ImEquation101"><![CDATA[$q$]]></tex-math></inline-formula> times, <inline-formula><tex-math notation="LaTeX" id="ImEquation102"><![CDATA[$\gamma_{\mu}$]]></tex-math></inline-formula>s appear at most <inline-formula><tex-math notation="LaTeX" id="ImEquation103"><![CDATA[$p+q$]]></tex-math></inline-formula> times. However, the number of <inline-formula><tex-math notation="LaTeX" id="ImEquation104"><![CDATA[$\gamma_{\mu}$]]></tex-math></inline-formula>s can be reduced as we explain below.</p>
<p>From the equation,
<disp-formula id="pty112M3-16"><label>(3.16)</label><tex-math notation="LaTeX" id="Equation41"><![CDATA[
\begin{equation}
\gamma_{\nu}(\gamma_{\mu_1}\cdots \gamma_{\mu_m}) = \sum_j (-1)^{j-1}2\delta_{\nu\mu_j}\gamma_{\mu_1}\cdots \hat{\gamma}_{\mu_j}\cdots \gamma_{\mu_m} + (-1)^m(\gamma_{\mu_1}\cdots \gamma_{\mu_m})\gamma_{\nu},
\end{equation}
]]></tex-math></disp-formula>
we obtain the following equations:
<disp-formula id="pty112M3-17"><label>(3.17)</label><tex-math notation="LaTeX" id="Equation42"><![CDATA[
\begin{align}
\gamma_{d+1}V(\gamma_{\mu_1} \cdots \gamma_{\mu_{2m'}})\gamma_{d+1}V = \gamma_{\mu_{1}} \cdots \gamma_{\mu_{2m'}} +\sum_{j}(-1)^{j}2 is_{\mu_j}(\gamma_{\mu_1} \cdots \hat{\gamma}_{\mu_j} \cdots \gamma_{\mu_{2m'}})S^{-1} V, \label{eq:V-gamma} \\
\end{align}
]]></tex-math></disp-formula>
<disp-formula id="pty112M3-18"><label>(3.18)</label><tex-math notation="LaTeX" id="Equation43"><![CDATA[
\begin{align}
V(\gamma_{\mu_1} \cdots \gamma_{\mu_{2m'-1}})V = \gamma_{\mu_{1}} \cdots \gamma_{\mu_{2m'-1}} +\sum_{j}(-1)^{j-1}2 is_{\mu_j}(\gamma_{\mu_1} \cdots \hat{\gamma}_{\mu_j} \cdots \gamma_{\mu_{2m'-1}}) S^{-1} V. \label{eq:V-gamma_odd}
\end{align}
]]></tex-math></disp-formula></p>
<p>Here, <inline-formula><tex-math notation="LaTeX" id="ImEquation105"><![CDATA[$\hat{\gamma}_{\mu_j}$]]></tex-math></inline-formula> means that <inline-formula><tex-math notation="LaTeX" id="ImEquation106"><![CDATA[$\gamma_{\mu_j}$]]></tex-math></inline-formula> is omitted. From Eqs. (<xref ref-type="disp-formula" rid="pty112M3-17">3.17</xref>) and (<xref ref-type="disp-formula" rid="pty112M3-18">3.18</xref>), the <inline-formula><tex-math notation="LaTeX" id="ImEquation107"><![CDATA[$a^{m}$]]></tex-math></inline-formula> terms in Eq. (<xref ref-type="disp-formula" rid="pty112M3-2">3.2</xref>) are reduced to a form in which the number of <inline-formula><tex-math notation="LaTeX" id="ImEquation108"><![CDATA[$\gamma_{\mu}$]]></tex-math></inline-formula>s is less than or equal to <inline-formula><tex-math notation="LaTeX" id="ImEquation109"><![CDATA[$m+1$]]></tex-math></inline-formula>. In addition, since the maximum numbers of <inline-formula><tex-math notation="LaTeX" id="ImEquation110"><![CDATA[$\gamma_{\mu}$]]></tex-math></inline-formula>s in <inline-formula><tex-math notation="LaTeX" id="ImEquation111"><![CDATA[$P_1P_2^{m}$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation112"><![CDATA[$VP_2^m$]]></tex-math></inline-formula> are odd, and the terms in Eq. (<xref ref-type="disp-formula" rid="pty112M3-2">3.2</xref>) are the products of an odd number of them, the maximum number of <inline-formula><tex-math notation="LaTeX" id="ImEquation113"><![CDATA[$\gamma_{\mu}$]]></tex-math></inline-formula>s in the <inline-formula><tex-math notation="LaTeX" id="ImEquation114"><![CDATA[$a^{d-1}$]]></tex-math></inline-formula> terms in Eq. (<xref ref-type="disp-formula" rid="pty112M3-2">3.2</xref>) is odd, that is, not <inline-formula><tex-math notation="LaTeX" id="ImEquation115"><![CDATA[$d$]]></tex-math></inline-formula> but <inline-formula><tex-math notation="LaTeX" id="ImEquation116"><![CDATA[$d-1$]]></tex-math></inline-formula>. Therefore, we only need to consider the <inline-formula><tex-math notation="LaTeX" id="ImEquation117"><![CDATA[$a^{d}$]]></tex-math></inline-formula> terms in Eq. (<xref ref-type="disp-formula" rid="pty112M3-2">3.2</xref>) in the continuum limit.</p>
<p>Let <inline-formula><tex-math notation="LaTeX" id="ImEquation118"><![CDATA[$N_V$]]></tex-math></inline-formula> be the number of <inline-formula><tex-math notation="LaTeX" id="ImEquation119"><![CDATA[$V$]]></tex-math></inline-formula>s in each of the <inline-formula><tex-math notation="LaTeX" id="ImEquation120"><![CDATA[$a^{d}$]]></tex-math></inline-formula> terms and <inline-formula><tex-math notation="LaTeX" id="ImEquation121"><![CDATA[$N_{\gamma}$]]></tex-math></inline-formula> the number of <inline-formula><tex-math notation="LaTeX" id="ImEquation122"><![CDATA[$\gamma_{\mu}$]]></tex-math></inline-formula>s without <inline-formula><tex-math notation="LaTeX" id="ImEquation123"><![CDATA[$\gamma_{\mu}$]]></tex-math></inline-formula>s in <inline-formula><tex-math notation="LaTeX" id="ImEquation124"><![CDATA[$V$]]></tex-math></inline-formula>s in each of the <inline-formula><tex-math notation="LaTeX" id="ImEquation125"><![CDATA[$a^{d}$]]></tex-math></inline-formula> terms. Then each of the <inline-formula><tex-math notation="LaTeX" id="ImEquation126"><![CDATA[$a^{d}$]]></tex-math></inline-formula> terms in Eq. (<xref ref-type="disp-formula" rid="pty112M3-2">3.2</xref>) can be classified into one of six cases.</p>
<list list-type="simple">
<list-item><p>(i) <inline-formula><tex-math notation="LaTeX" id="ImEquation127"><![CDATA[$N_V$]]></tex-math></inline-formula> is odd and <inline-formula><tex-math notation="LaTeX" id="ImEquation128"><![CDATA[$N_{\gamma}=d$]]></tex-math></inline-formula>.</p>
<p>The terms classified into case (i) are the products of <inline-formula><tex-math notation="LaTeX" id="ImEquation129"><![CDATA[$V$]]></tex-math></inline-formula>s and the first terms of the right-hand sides of Eqs. (<xref ref-type="disp-formula" rid="pty112M3-8">3.8</xref>) and (<xref ref-type="disp-formula" rid="pty112M3-9">3.9</xref>). From Eqs. (<xref ref-type="disp-formula" rid="pty112M3-17">3.17</xref>) and (<xref ref-type="disp-formula" rid="pty112M3-18">3.18</xref>), the number of <inline-formula><tex-math notation="LaTeX" id="ImEquation130"><![CDATA[$\gamma_{\mu}$]]></tex-math></inline-formula>s is reduced to <inline-formula><tex-math notation="LaTeX" id="ImEquation131"><![CDATA[$d+1$]]></tex-math></inline-formula> at most.
<disp-formula id="pty112M3-19"><label>(3.19)</label><tex-math notation="LaTeX" id="Equation44"><![CDATA[
\begin{equation}
{\mathop{\mathrm{tr}}\nolimits} (\text{odd $\gamma$s})V \cdots \underbrace{V(\text{odd $\gamma$s})V}_{\text{Eq.(3.17) or (3.18)}}(\text{odd $\gamma$s})\underbrace{V(\text{odd $\gamma$s})V}_{\text{Eq.(3.17) or (3.18)}} \cdots V(\text{even $\gamma$s})
\end{equation}
]]></tex-math></disp-formula></p>
<p>Since <inline-formula><tex-math notation="LaTeX" id="ImEquation137"><![CDATA[${\mathop{\mathrm{tr}}\nolimits} \gamma_{d+1}\gamma_{\mu_1}\cdots \gamma_{\mu_{d+1}} = 0$]]></tex-math></inline-formula>, the terms that contain <inline-formula><tex-math notation="LaTeX" id="ImEquation138"><![CDATA[$d$]]></tex-math></inline-formula> <inline-formula><tex-math notation="LaTeX" id="ImEquation139"><![CDATA[$\gamma_{\mu}$]]></tex-math></inline-formula>s only contribute to Eq. (<xref ref-type="disp-formula" rid="pty112M3-2">3.2</xref>). In the terms that contain the second term of Eq. (<xref ref-type="disp-formula" rid="pty112M3-17">3.17</xref>) or (<xref ref-type="disp-formula" rid="pty112M3-18">3.18</xref>), <inline-formula><tex-math notation="LaTeX" id="ImEquation140"><![CDATA[$V$]]></tex-math></inline-formula>s appear at least twice and the total number of <inline-formula><tex-math notation="LaTeX" id="ImEquation141"><![CDATA[$\gamma_{\mu}$]]></tex-math></inline-formula>s and <inline-formula><tex-math notation="LaTeX" id="ImEquation142"><![CDATA[$\gamma_{d+1}$]]></tex-math></inline-formula>s between them is odd. Using Eq. (<xref ref-type="disp-formula" rid="pty112M3-17">3.17</xref>) or (<xref ref-type="disp-formula" rid="pty112M3-18">3.18</xref>), one can reduce the number of <inline-formula><tex-math notation="LaTeX" id="ImEquation143"><![CDATA[$\gamma_{\mu}$]]></tex-math></inline-formula>s in these terms by two and only the first terms of Eq. (<xref ref-type="disp-formula" rid="pty112M3-17">3.17</xref>) remain. Thus the terms classified into case (i) are equivalent to the terms from which all <inline-formula><tex-math notation="LaTeX" id="ImEquation144"><![CDATA[$V$]]></tex-math></inline-formula>s are removed and that are multiplied by <inline-formula><tex-math notation="LaTeX" id="ImEquation145"><![CDATA[$-M/S$]]></tex-math></inline-formula> because one <inline-formula><tex-math notation="LaTeX" id="ImEquation146"><![CDATA[$V$]]></tex-math></inline-formula> remains.</p></list-item>
<list-item><p>(ii) <inline-formula><tex-math notation="LaTeX" id="ImEquation147"><![CDATA[$N_V$]]></tex-math></inline-formula> is odd and <inline-formula><tex-math notation="LaTeX" id="ImEquation148"><![CDATA[$N_{\gamma}=d-1$]]></tex-math></inline-formula>.</p>
<p>The terms classified into case (ii) are the products of <inline-formula><tex-math notation="LaTeX" id="ImEquation149"><![CDATA[$V$]]></tex-math></inline-formula>s and the first terms of the right-hand sides of Eqs. (<xref ref-type="disp-formula" rid="pty112M3-8">3.8</xref>) and (<xref ref-type="disp-formula" rid="pty112M3-9">3.9</xref>), except for one factor which is replaced with the second term. From Eqs. (<xref ref-type="disp-formula" rid="pty112M3-17">3.17</xref>) and (<xref ref-type="disp-formula" rid="pty112M3-18">3.18</xref>), the number of <inline-formula><tex-math notation="LaTeX" id="ImEquation150"><![CDATA[$\gamma_{\mu}$]]></tex-math></inline-formula>s is reduced to <inline-formula><tex-math notation="LaTeX" id="ImEquation151"><![CDATA[$d$]]></tex-math></inline-formula> at most.
<disp-formula id="pty112M3-20"><label>(3.20)</label><tex-math notation="LaTeX" id="Equation45"><![CDATA[
\begin{equation}
 {\mathop{\mathrm{tr}}\nolimits} (\text{odd $\gamma$s})V \cdots \underbrace{V(\text{odd $\gamma$s})V}_{\text{Eq.(3.17) or (3.18)}}(\text{odd $\gamma$s})V(\text{even $\gamma$s})\underbrace{V(\text{odd $\gamma$s})V}_{\text{Eq.(3.17) or (3.18)}} \cdots V(\text{even $\gamma$s})
\end{equation}
]]></tex-math></disp-formula></p>
<p>The second terms of Eqs. (<xref ref-type="disp-formula" rid="pty112M3-17">3.17</xref>) and (<xref ref-type="disp-formula" rid="pty112M3-18">3.18</xref>) do not contribute to Eq. (<xref ref-type="disp-formula" rid="pty112M3-2">3.2</xref>), as explained in case (i). Moreover, only the <inline-formula><tex-math notation="LaTeX" id="ImEquation158"><![CDATA[$\sum_{\nu}\gamma_{\nu}is_{\nu}/S$]]></tex-math></inline-formula> part in the remaining <inline-formula><tex-math notation="LaTeX" id="ImEquation159"><![CDATA[$V$]]></tex-math></inline-formula> contributes to Eq. (<xref ref-type="disp-formula" rid="pty112M3-2">3.2</xref>). The total number of <inline-formula><tex-math notation="LaTeX" id="ImEquation160"><![CDATA[$\gamma_{\mu}$]]></tex-math></inline-formula>s and <inline-formula><tex-math notation="LaTeX" id="ImEquation161"><![CDATA[$\gamma_{d+1}$]]></tex-math></inline-formula>s between the factor <inline-formula><tex-math notation="LaTeX" id="ImEquation162"><![CDATA[$\sum_{\nu}\gamma_{\nu}is_{\nu}/S$]]></tex-math></inline-formula> and the factor with respect to the second term of the right-hand sides of Eqs. (<xref ref-type="disp-formula" rid="pty112M3-8">3.8</xref>) and (<xref ref-type="disp-formula" rid="pty112M3-9">3.9</xref>) is odd for Eq. (<xref ref-type="disp-formula" rid="pty112M3-8">3.8</xref>) and even for Eq. (<xref ref-type="disp-formula" rid="pty112M3-9">3.9</xref>). Therefore, the terms classified into case (ii) are equivalent to the terms from which all <inline-formula><tex-math notation="LaTeX" id="ImEquation163"><![CDATA[$V$]]></tex-math></inline-formula>s are removed and in which the factor <inline-formula><tex-math notation="LaTeX" id="ImEquation164"><![CDATA[$\mp \sum_{\nu}\gamma_{\nu}is_{\nu}/S$]]></tex-math></inline-formula> is inserted before the factor with respect to the second term of the right-hand sides of Eqs. (<xref ref-type="disp-formula" rid="pty112M3-8">3.8</xref>) and (<xref ref-type="disp-formula" rid="pty112M3-9">3.9</xref>), with a negative sign for Eq. (<xref ref-type="disp-formula" rid="pty112M3-8">3.8</xref>) and a positive sign for Eq. (<xref ref-type="disp-formula" rid="pty112M3-9">3.9</xref>).</p></list-item>
<list-item><p>(iii-a) <inline-formula><tex-math notation="LaTeX" id="ImEquation165"><![CDATA[$N_V$]]></tex-math></inline-formula> is odd and <inline-formula><tex-math notation="LaTeX" id="ImEquation166"><![CDATA[$N_{\gamma}$]]></tex-math></inline-formula> is odd with <inline-formula><tex-math notation="LaTeX" id="ImEquation167"><![CDATA[$N_{\gamma} \leq d-3$]]></tex-math></inline-formula>.</p></list-item>
<list-item><p>(iii-b) <inline-formula><tex-math notation="LaTeX" id="ImEquation168"><![CDATA[$N_V$]]></tex-math></inline-formula> is even and <inline-formula><tex-math notation="LaTeX" id="ImEquation169"><![CDATA[$N_{\gamma}$]]></tex-math></inline-formula> is even with <inline-formula><tex-math notation="LaTeX" id="ImEquation170"><![CDATA[$N_{\gamma} \leq d-2$]]></tex-math></inline-formula>. From Eqs. (<xref ref-type="disp-formula" rid="pty112M3-17">3.17</xref>) and (<xref ref-type="disp-formula" rid="pty112M3-18">3.18</xref>), the number of <inline-formula><tex-math notation="LaTeX" id="ImEquation171"><![CDATA[$\gamma_{\mu}$]]></tex-math></inline-formula>s is reduced to <inline-formula><tex-math notation="LaTeX" id="ImEquation172"><![CDATA[$d$]]></tex-math></inline-formula> at most and at least two <inline-formula><tex-math notation="LaTeX" id="ImEquation173"><![CDATA[$V$]]></tex-math></inline-formula>s remain. Thus, in the terms in which <inline-formula><tex-math notation="LaTeX" id="ImEquation174"><![CDATA[$\gamma_{\mu}$]]></tex-math></inline-formula>s appear <inline-formula><tex-math notation="LaTeX" id="ImEquation175"><![CDATA[$d$]]></tex-math></inline-formula> times, the <inline-formula><tex-math notation="LaTeX" id="ImEquation176"><![CDATA[$\left(\sum_{\nu}\gamma_{\nu}s_{\nu}\right)$]]></tex-math></inline-formula>s from the remaining <inline-formula><tex-math notation="LaTeX" id="ImEquation177"><![CDATA[$V$]]></tex-math></inline-formula>s appear twice at least. Since <inline-formula><tex-math notation="LaTeX" id="ImEquation178"><![CDATA[${\mathop{\mathrm{tr}}\nolimits} \gamma_{d+1}\gamma_{\mu_1}\cdots \gamma_{\mu_d} = (-i)^n2^n\epsilon_{\mu_1 \cdots \mu_{d}}$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation179"><![CDATA[$\epsilon_{\mu_1 \cdots \mu_{d}}$]]></tex-math></inline-formula> is antisymmetric with respect to the subscripts, the terms classified into cases (iii-a) and (iii-b) do not contribute to Eq. (<xref ref-type="disp-formula" rid="pty112M3-2">3.2</xref>).</p></list-item>
<list-item><p>(iv-a) <inline-formula><tex-math notation="LaTeX" id="ImEquation180"><![CDATA[$N_V$]]></tex-math></inline-formula> is odd and <inline-formula><tex-math notation="LaTeX" id="ImEquation181"><![CDATA[$N_{\gamma}$]]></tex-math></inline-formula> is even with <inline-formula><tex-math notation="LaTeX" id="ImEquation182"><![CDATA[$N_{\gamma} \leq d-2$]]></tex-math></inline-formula>.</p></list-item>
<list-item><p>(iv-b) <inline-formula><tex-math notation="LaTeX" id="ImEquation183"><![CDATA[$N_V$]]></tex-math></inline-formula> is even and <inline-formula><tex-math notation="LaTeX" id="ImEquation184"><![CDATA[$N_{\gamma}$]]></tex-math></inline-formula> is odd with <inline-formula><tex-math notation="LaTeX" id="ImEquation185"><![CDATA[$N_{\gamma} \leq d-1$]]></tex-math></inline-formula>. From Eqs. (<xref ref-type="disp-formula" rid="pty112M3-17">3.17</xref>) and (<xref ref-type="disp-formula" rid="pty112M3-18">3.18</xref>), the number of <inline-formula><tex-math notation="LaTeX" id="ImEquation186"><![CDATA[$\gamma_{\mu}$]]></tex-math></inline-formula>s is reduced to <inline-formula><tex-math notation="LaTeX" id="ImEquation187"><![CDATA[$d-1$]]></tex-math></inline-formula> at most. Thus, the terms classified into cases (iv-a) and (iv-b) do not contribute to Eq. (<xref ref-type="disp-formula" rid="pty112M3-2">3.2</xref>).</p></list-item>
</list>
<p>Therefore, the terms classified into cases (i) and (ii) only contribute to Eq. (<xref ref-type="disp-formula" rid="pty112M3-2">3.2</xref>) in the continuum limit. Note that the terms which contain the factors of ellipses in Eqs. (<xref ref-type="disp-formula" rid="pty112M3-13">3.13</xref>), (<xref ref-type="disp-formula" rid="pty112M3-14">3.14</xref>), and (<xref ref-type="disp-formula" rid="pty112M3-15">3.15</xref>) do not contribute to Eq. (<xref ref-type="disp-formula" rid="pty112M3-2">3.2</xref>) in the continuum limit, because they correspond to the cases (iii-a), (iii-b), (iv-a), and (iv-b).</p>
<p>Now, we can write down the terms which contribute to Eq. (<xref ref-type="disp-formula" rid="pty112M3-2">3.2</xref>) in the continuum limit. Here we define the following functions:
<disp-formula id="pty112M3-21"><label>(3.21)</label><tex-math notation="LaTeX" id="Equation46"><![CDATA[
\begin{align}
\tilde{D}(\lambda) &= \sum_{\mu}\gamma_{\mu} c_{\mu}D_{\mu}-\lambda \left(\sum_{\mu}\gamma_{\mu}is_{\mu} \right)\left(- r\sum_{\mu} is_{\mu}D_{\mu}\right)\!, \\
\end{align}
]]></tex-math></disp-formula>
<disp-formula id="pty112M3-22"><label>(3.22)</label><tex-math notation="LaTeX" id="Equation47"><![CDATA[
\begin{align}
\tilde{F}(\lambda) &= \frac{1}{2}\sum_{\nu,\rho}\gamma_{\nu}\gamma_{\rho}c_{\nu}c_{\rho}F_{\nu\rho}+\lambda \left(\sum_{\mu}\gamma_{\mu}is_{\mu}\right)\left(-r\sum_{\nu,\rho}\gamma_{\nu}c_{\nu} is_{\rho}F_{\nu\rho}\right)\!,
\end{align}
]]></tex-math></disp-formula>
and
<disp-formula id="pty112M3-23"><label>(3.23)</label><tex-math notation="LaTeX" id="Equation48"><![CDATA[
\begin{equation}
\left\{
\begin{aligned}
\tilde{P}_1(\lambda) &= \tilde{D}(\lambda) - \tilde{D}^0(\lambda), \\
\tilde{P}_{2\ell}(\lambda) &= \alpha_{2\ell}\tilde{F}(\lambda)^{\ell}, \\
\tilde{P}_{2\ell+1}(\lambda) &= \alpha_{2\ell}\tilde{D}(\lambda)\tilde{F}(\lambda)^{\ell},
\end{aligned}
\right.
\end{equation}
]]></tex-math></disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation188"><![CDATA[$\tilde{D}^0(\lambda)= \tilde{D}(\lambda)|_{A=0}$]]></tex-math></inline-formula>. Then, we obtain
<disp-formula id="pty112M3-24"><label>(3.24)</label><tex-math notation="LaTeX" id="Equation49"><![CDATA[
\begin{align}
&e^{-ikx/a}\left(\frac{1}{a^d}\left. {\mathop{\mathrm{tr}}\nolimits} \Delta^{2\ell}\delta_{\star}^{\omega}\epsilon_{\star}\right|_{A_{\star}=0}\right)e^{ikx/a} \nonumber \\
&=S^{-2n-1}{\mathop{\mathrm{tr}}\nolimits} \sum_{\sum\limits_{m=1}^{2\ell}i_m=d-1} \Biggl( (-M)( \gamma_{d+1}\tilde{P}_{i_1})\cdots (\gamma_{d+1}\tilde{P}_{i_{2\ell}})(\gamma_{d+1}\delta^{\omega}\tilde{P}_1) \nonumber \\
&\hspace{4cm}+ \frac{{d}}{{d} \lambda}(\gamma_{d+1}\tilde{P}_{i_1})\cdots (\gamma_{d+1}\tilde{P}_{i_{2\ell}})(\gamma_{d+1}\delta^{\omega}\tilde{P}_1) \Biggr)\Biggr|_{\lambda = 0} + \mathcal{O}(a) \nonumber \\
&=-S^{-2n-1}{\mathop{\mathrm{tr}}\nolimits} \sum_{\sum\limits_{m=1}^{2\ell}i_m=d-1}(-1)^{\sum\limits_{m'=1}^{\ell}i_{2m'}}\Biggl( M\gamma_{d+1}\tilde{P}_{i_1}\cdots \tilde{P}_{i_{2\ell}}\delta^{\omega}\tilde{P}_1\nonumber \\
&\hspace{6.1cm}- \gamma_{d+1}\frac{{d}}{{d} \lambda}\tilde{P}_{i_1}\cdots \tilde{P}_{i_{2\ell}} \delta^{\omega}\tilde{P}_1 \Biggr)\Biggr|_{\lambda = 0} + \mathcal{O}(a), \label{eq:Delta^2l}
\end{align}
]]></tex-math></disp-formula>
and
<disp-formula id="pty112M3-25"><label>(3.25)</label><tex-math notation="LaTeX" id="Equation50"><![CDATA[
\begin{align}
&e^{-ikx/a}\left(\frac{1}{a^d}\left. {\mathop{\mathrm{tr}}\nolimits} \epsilon_{\star}\Delta^{2\ell+1}\delta_{\star}^{\omega}\epsilon_{\star}\right|_{A_{\star}=0}\right)e^{ikx/a} \nonumber \\
&=S^{-2n-1} {\mathop{\mathrm{tr}}\nolimits} \sum_{\sum\limits_{m=1}^{2\ell+1}i_m=d-1} \Biggl((-M)\gamma_{d+1}( \gamma_{d+1}\tilde{P}_{i_1})\cdots (\gamma_{d+1}\tilde{P}_{i_{2\ell+1}}) (\gamma_{d+1}\delta^{\omega}\tilde{P}_1) \nonumber\\
&\hspace{4cm}+ \frac{{d}}{{d} \lambda}\gamma_{d+1}(\gamma_{d+1}\tilde{P}_{i_1})\cdots (\gamma_{d+1}\tilde{P}_{i_{2\ell+1}}) (\gamma_{d+1}\delta^{\omega}\tilde{P}_1)\Biggr)\Biggr|_{\lambda=0}\nonumber\\
&\quad+S^{-2n-1} {\mathop{\mathrm{tr}}\nolimits} \sum_{\sum\limits_{m=1}^{2\ell+1}i_m=d-2}\Biggl( (-M)(\gamma_{d+1}\tilde{D}^0) (\gamma_{d+1}\tilde{P}_{i_1}) \cdots (\gamma_{d+1}\tilde{P}_{i_{2\ell+1}}) (\gamma_{d+1}\delta^{\omega}\tilde{P}_1) \nonumber \\
&\hspace{3cm}+ \frac{{d}}{{d} \lambda} (\gamma_{d+1}\tilde{D}^0) (\gamma_{d+1}\tilde{P}_{i_1}) \cdots (\gamma_{d+1}\tilde{P}_{i_{2\ell+1}}) (\gamma_{d+1}\delta^{\omega}\tilde{P}_1) \Biggr)\Biggr|_{\lambda=0}+ \mathcal{O}(a) \nonumber \\
&=-S^{-2n-1} {\mathop{\mathrm{tr}}\nolimits} \sum_{\sum\limits_{m=1}^{2\ell+1}i_m=d-2} (-1)^{\sum\limits_{m'=0}^{\ell}i_{2m'+1}}\Biggl(M\gamma_{d+1}\tilde{P}_{i_1}\cdots \tilde{P}_{i_{2\ell+1}}\delta^{\omega}\tilde{P}_1 \nonumber\\
&\hspace{6.4cm}- \gamma_{d+1}\frac{{d}}{{d} \lambda}\tilde{P}_{i_1}\cdots \tilde{P}_{i_{2\ell+1}}\delta^{\omega}\tilde{P}_1\Biggr)\Biggr|_{\lambda=0}\nonumber\\
&\quad -S^{-2n-1} {\mathop{\mathrm{tr}}\nolimits} \sum_{\sum\limits_{m=1}^{2\ell+1}i_m=d-2}(-1)^{\sum\limits_{m'=0}^{\ell}i_{2m'+1}}\Biggl( M\gamma_{d+1}\tilde{D}^0\tilde{P}_{i_1}\cdots \tilde{P}_{i_{2\ell+1}}\delta^{\omega}\tilde{P}_1 \nonumber \\
&\hspace{6.4cm}- \gamma_{d+1}\frac{{d}}{{d} \lambda}\tilde{D}^0\tilde{P}_{i_1}\cdots \tilde{P}_{i_{2\ell+1}}\delta^{\omega}\tilde{P}_1\Biggr)\Biggr|_{\lambda=0}+ \mathcal{O}(a). \label{eq:Delta^2l+1}
\end{align}
]]></tex-math></disp-formula></p>
<p>Equations (<xref ref-type="disp-formula" rid="pty112M3-24">3.24</xref>) and (<xref ref-type="disp-formula" rid="pty112M3-25">3.25</xref>) can be simplified further by evaluating the trace over the spinor index and the integral with respect to the variable <inline-formula><tex-math notation="LaTeX" id="ImEquation189"><![CDATA[$k$]]></tex-math></inline-formula>. In general, by defining
<disp-formula id="pty112M3-26"><label>(3.26)</label><tex-math notation="LaTeX" id="Equation51"><![CDATA[
\begin{align}
X_1 &\equiv M\sum_{\mu_1,\ldots, \mu_{2n}} \gamma_{\mu_1}\cdots\gamma_{\mu_{2n}}c_{\mu_1}\cdots c_{\mu_{2n}}X_{\mu_1 \cdots \mu_{2n}}, \\
\end{align}
]]></tex-math></disp-formula>
<disp-formula id="pty112M3-27"><label>(3.27)</label><tex-math notation="LaTeX" id="Equation52"><![CDATA[
\begin{align}
X_2 &\equiv r\sum_{i} (-1)^{i-1}\sum_{\sigma}\gamma_{\sigma}s_{\sigma}\sum_{\mu_1,\ldots, \mu_{2n}}\gamma_{\mu_1}\cdots\hat{\gamma}_{\mu_i}\cdots \gamma_{\mu_{2n}} s_{\mu_i}c_{\mu_1}\cdots \hat{c}_{\mu_{i}}\cdots c_{\mu_{2n}}X_{\mu_1 \cdots \mu_{2n}},
\end{align}
]]></tex-math></disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation190"><![CDATA[$X_{\mu_1 \cdots \mu_{2n}}$]]></tex-math></inline-formula> is independent of <inline-formula><tex-math notation="LaTeX" id="ImEquation191"><![CDATA[$k_{\mu}$]]></tex-math></inline-formula> and valued in the Lie algebra of the gauge group <inline-formula><tex-math notation="LaTeX" id="ImEquation192"><![CDATA[$\mathcal{G}$]]></tex-math></inline-formula> with <inline-formula><tex-math notation="LaTeX" id="ImEquation193"><![CDATA[$2n$]]></tex-math></inline-formula> subscripts running from <inline-formula><tex-math notation="LaTeX" id="ImEquation194"><![CDATA[$1$]]></tex-math></inline-formula> to <inline-formula><tex-math notation="LaTeX" id="ImEquation195"><![CDATA[$2n$]]></tex-math></inline-formula>, we have the following equations:
<disp-formula id="pty112M3-28"><label>(3.28)</label><tex-math notation="LaTeX" id="Equation53"><![CDATA[
\begin{align}
&\int_{\mathcal{B}^d} \frac{{d}^d k}{(2\pi)^d}\, S^{-2n-1} \left[ {\mathop{\mathrm{tr}}\nolimits} \left( \gamma_{d+1}X_1 \right) +{\mathop{\mathrm{tr}}\nolimits} \left( \gamma_{d+1}X_2 \right)\right] \nonumber \\
&=\int_{\mathcal{B}^d} \frac{{d}^d k}{(2\pi)^d}\, S^{-2n-1} (-i)^n2^n\sum_{\mu_1,\ldots, \mu_{2n}}\epsilon_{\mu_1 \cdots \mu_{2n}}c_{\mu_1}\cdots c_{\mu_{2n}}\left( M +r\sum_{i}s_{\mu_i}^2/c_{\mu_i}\right) X_{\mu_1 \cdots \mu_{2n}} \nonumber \\
&=\int_{\mathcal{B}^d} \frac{{d}^d k}{(2\pi)^d}\, S^{-2n-1} (-i)^n2^n\left(\prod_{\mu}c_{\mu}\right)\left( M +r\sum_{\rho}s_{\rho}^2/c_{\rho}\right)\sum_{\mu_1,\ldots, \mu_{2n}}\epsilon_{\mu_1 \cdots \mu_{2n}} X_{\mu_1 \cdots \mu_{2n}} \nonumber \\
&=\frac{2(-i)^n}{(2\pi)^n}\frac{\Gamma(1/2)}{\Gamma(n+1/2)}I(M_0,r)\sum_{\mu_1,\ldots ,\mu_{2n}}\epsilon_{\mu_1 \cdots \mu_{2n}}X_{\mu_1\cdots \mu_{2n}} \nonumber \\
&= \frac{(-i)^n}{(2\pi)^nn!} \frac{2}{\alpha_{2n}}\sum_{\mu_1,\ldots ,\mu_{2n}}\epsilon_{\mu_1 \cdots \mu_{2n}}X_{\mu_1\cdots \mu_{2n}}, \label{eq:X}
\end{align}
]]></tex-math></disp-formula>
where <inline-formula><tex-math notation="LaTeX" id="ImEquation196"><![CDATA[${\mathop{\mathrm{tr}}\nolimits}$]]></tex-math></inline-formula> denotes the trace over the spinor only, and
<disp-formula id="pty112M3-29"><label>(3.29)</label><tex-math notation="LaTeX" id="Equation54"><![CDATA[
\begin{align}
I(M_0,r) &\equiv \frac{1}{2\pi^n}\frac{\Gamma(n+1/2)}{\Gamma(1/2)} \int_{\mathcal{B}^d}{d}^d k\, \left(\prod_{\mu}c_{\mu}\right) S^{-n-1/2} \left( M+r\sum_{\rho}s_{\rho}^2/c_{\rho} \right) \nonumber \\
&= \sum_{n_{\pi}=0}^{\lfloor M_0/(2r)\rfloor} \frac{d!}{n_{\pi}!(d-n_{\pi})!} (-1)^{n_{\pi}}. \label{eq:derivation_of_I}
\end{align}
]]></tex-math></disp-formula>
<inline-formula><tex-math notation="LaTeX" id="ImEquation197"><![CDATA[$\lfloor x \rfloor$]]></tex-math></inline-formula> denotes the maximum integer which is less than or equal to <inline-formula><tex-math notation="LaTeX" id="ImEquation198"><![CDATA[$x$]]></tex-math></inline-formula>. For the derivation of Eq. (<xref ref-type="disp-formula" rid="pty112M3-29">3.29</xref>), see Ref. [<xref ref-type="bibr" rid="B14">14</xref>]. In the last equality of Eq. (<xref ref-type="disp-formula" rid="pty112M3-28">3.28</xref>) we used <inline-formula><tex-math notation="LaTeX" id="ImEquation199"><![CDATA[$I(M_0,r)=1$]]></tex-math></inline-formula> by assuming <inline-formula><tex-math notation="LaTeX" id="ImEquation200"><![CDATA[$0<M_0/r<2$]]></tex-math></inline-formula>. Therefore, using Eqs. (<xref ref-type="disp-formula" rid="pty112M3-24">3.24</xref>), (<xref ref-type="disp-formula" rid="pty112M3-25">3.25</xref>), and (<xref ref-type="disp-formula" rid="pty112M3-28">3.28</xref>), we finally obtain the following expression:
<disp-formula id="pty112M3-30"><label>(3.30)</label><tex-math notation="LaTeX" id="Equation55"><![CDATA[
\begin{equation}
\lim_{a \to 0} a^d\sum_x \mathcal{A}_{\mathrm{gauge}}(x) = \frac{1}{n!}\left( \frac{-i}{2\pi}\right)^n \int \frac{-1}{2\alpha_{2n}}{\mathop{\mathrm{tr}}\nolimits} G,
\end{equation}
]]></tex-math></disp-formula>
where
<disp-formula id="pty112M3-31"><label>(3.31)</label><tex-math notation="LaTeX" id="Equation56"><![CDATA[
\begin{align}
G &=\sum_{\ell=0}^{\infty}\left[\sum_{\sum\nolimits_{m=1}^{2\ell}i_m=d-1} (-1)^{\sum_{m'}i_{2m'}} (1/2)^{2\ell}g_{i_1}\cdots g_{i_{2\ell}} \right.\nonumber\\
&\hspace{0.9cm}+ \sum_{\sum\nolimits_{m=1}^{2\ell+1}i_m=d-1} (-1)^{\sum_{m'}i_{2m'+1}}(1/2)^{2\ell+1}g_{i_1}\cdots g_{i_{2\ell+1}} \nonumber\\
& \hspace{0.9cm}\left.+ \sum_{\sum\nolimits_{m=1}^{2\ell+1}i_m=d-2} (-1)^{\sum_{m'}i_{2m'+1}}(1/2)^{2\ell+1} {d} g_{i_1}\cdots g_{i_{2\ell+1}} \right]{d} \omega, \label{eq:G}
\end{align}
]]></tex-math></disp-formula>
and
<disp-formula id="pty112M3-32"><label>(3.32)</label><tex-math notation="LaTeX" id="Equation57"><![CDATA[
\begin{equation}
\left\{
\begin{aligned}
g_1 &= A, \\
g_{2m} &= \alpha_{2m}F^m, \\
g_{2m+1} &= \alpha_{2m}DF^m.
\end{aligned}
\right.
\end{equation}
]]></tex-math></disp-formula></p>
<p>Here, <inline-formula><tex-math notation="LaTeX" id="ImEquation201"><![CDATA[$\omega$]]></tex-math></inline-formula> is defined by Eqs. (<xref ref-type="disp-formula" rid="pty112M2-20">2.20</xref>) and (<xref ref-type="disp-formula" rid="pty112M2-21">2.21</xref>), and we used the differential form. That is, <inline-formula><tex-math notation="LaTeX" id="ImEquation202"><![CDATA[$A= A_{\mu}{d} x^{\mu}$]]></tex-math></inline-formula>, <inline-formula><tex-math notation="LaTeX" id="ImEquation203"><![CDATA[$D={d} +A$]]></tex-math></inline-formula>, and <inline-formula><tex-math notation="LaTeX" id="ImEquation204"><![CDATA[$F = D^2 = 1/2F_{\mu\nu}{d} x^{\mu} \wedge {d} x^{\nu}$]]></tex-math></inline-formula>. We can obtain the explicit form in the specific dimensions as follows:</p>
<list list-type="simple">
<list-item><p>(1) <inline-formula><tex-math notation="LaTeX" id="ImEquation205"><![CDATA[$d=2$]]></tex-math></inline-formula>: From Eq. (<xref ref-type="disp-formula" rid="pty112M3-31">3.31</xref>), we have
<disp-formula id="pty112M3-33"><label>(3.33)</label><tex-math notation="LaTeX" id="Equation58"><![CDATA[
\begin{equation}
G = -1/2A{d} \omega.
\end{equation}
]]></tex-math></disp-formula></p>
<p>Thus we obtain
<disp-formula id="pty112M3-34"><label>(3.34)</label><tex-math notation="LaTeX" id="Equation59"><![CDATA[
\begin{align}
\lim_{a \to 0} a^2\sum_x \mathcal{A}_{\mathrm{gauge}}(x) =-\frac{i}{4\pi}\int {\mathop{\mathrm{tr}}\nolimits} A{d} \omega.
\end{align}
]]></tex-math></disp-formula></p></list-item>
<list-item><p>(2) <inline-formula><tex-math notation="LaTeX" id="ImEquation206"><![CDATA[$d=4$]]></tex-math></inline-formula>: From Eq. (<xref ref-type="disp-formula" rid="pty112M3-31">3.31</xref>), we have
<disp-formula id="pty112M3-35"><label>(3.35)</label><tex-math notation="LaTeX" id="Equation60"><![CDATA[
\begin{align}
G &= (- 1/2 \alpha_2 DF+1/4 \alpha_2 A\cdot F -1/4 \alpha_2 F\cdot A +1/2 \alpha_2{d} F + 1/8 A\cdot A\cdot A){d} \omega \nonumber \\
&= -1/8(A({d} A) + ({d} A) A + A^3){d} \omega.
\end{align}
]]></tex-math></disp-formula></p>
<p>Thus we obtain
<disp-formula id="pty112M3-36"><label>(3.36)</label><tex-math notation="LaTeX" id="Equation61"><![CDATA[
\begin{align}
\lim_{a \to 0} a^4\sum_x \mathcal{A}_{\mathrm{gauge}}(x) =-\frac{1}{48\pi^2}\int (A({d} A) + ({d} A) A + A^3){d} \omega.
\end{align}
]]></tex-math></disp-formula></p>
<p>This result is derived in Ref. [<xref ref-type="bibr" rid="B12">12</xref>].</p></list-item>
<list-item><p>(3) <inline-formula><tex-math notation="LaTeX" id="ImEquation207"><![CDATA[$d=6$]]></tex-math></inline-formula>: From Eq. (<xref ref-type="disp-formula" rid="pty112M3-31">3.31</xref>), we have
<disp-formula id="pty112M3-37"><label>(3.37)</label><tex-math notation="LaTeX" id="Equation62"><![CDATA[
\begin{align}
G &= [ 1/4(\alpha_4A\cdot F^2- \alpha_2^2 F\cdot DF+\alpha_2^2DF \cdot F - \alpha_4 F^2 \cdot A) \nonumber\\
&\quad +1/16 (\alpha_2 F\cdot A \cdot A \cdot A- \alpha_2 A\cdot F \cdot A \cdot A+ \alpha_2 A\cdot A \cdot F \cdot A-\alpha_2 A\cdot A \cdot A \cdot F )\nonumber\\
&\quad - 1/2 \alpha_4 DF^2 +1/8(\alpha_2 A\cdot A \cdot DF +\alpha_2 A\cdot DF \cdot A + \alpha_2 DF\cdot A \cdot A) \nonumber\\
&\quad +1/8(-\alpha_2^2 A \cdot F \cdot F + \alpha_2^2 F \cdot A \cdot F - \alpha_2^2F \cdot F \cdot A) \nonumber\\
& \quad-1/32 A\cdot A \cdot A \cdot A \cdot A \nonumber \\
&\quad +1/2\alpha_4 {d} F^2 +1/8( -\alpha_2 {d} F \cdot A \cdot A+\alpha_2 {d} A \cdot F \cdot A-\alpha_2{d} A \cdot A \cdot F )]{d} \omega \nonumber \\
&=-1/32( 2A({d} A)^2+({d} A)A({d} A)+2({d} A)^2 A + 2({d} A)A^3 \nonumber\\
&\hspace{2cm}+ A({d} A)A^2+ A^2({d} A)A +2A^3({d} A) + 2A^5 ){d} \omega.
\end{align}
]]></tex-math></disp-formula></p>
<p>Thus we obtain
<disp-formula id="pty112M3-38"><label>(3.38)</label><tex-math notation="LaTeX" id="Equation63"><![CDATA[
\begin{align}
\lim_{a \to 0} a^6\sum_x \mathcal{A}_{\mathrm{gauge}}(x) &=\frac{i}{48\pi}\int {\mathop{\mathrm{tr}}\nolimits} \Bigl(\frac{1}{20}(2({d} A)^2A+({d} A)A({d} A)+2A({d} A)^2) \nonumber \\
&\quad+\frac{1}{20}(2({d} A)A^3+A({d} A)A^2+A^2({d} A)A+2A^3({d} A))+\frac{1}{10}A^5\Bigr){d} \omega.
\end{align}
]]></tex-math></disp-formula></p></list-item>
</list>
<p>It turns out from the above results that the gauge anomalies in two, four, and six dimensions in the continuum limit obtained here are equivalent to those known in the continuum theory up to total derivatives (for a review of the gauge anomaly, see Ref. [<xref ref-type="bibr" rid="B15">15</xref>]).</p>
</sec>
<sec id="SEC4"><title>4. Conclusion</title>
<p>In this paper, we generalized the result in Ref. [<xref ref-type="bibr" rid="B12">12</xref>], in which the gauge anomaly of the four-dimensional effective theory is calculated; i.e., we performed the explicit calculation of the arbitrary even-dimensional gauge anomaly with the chiral overlap operator in the continuum limit. The resultant expressions in two, four, and six dimensions are found to be equivalent to those known in the continuum theory up to total derivatives. If the gauge field is evolved by the gradient flow, the total effective action is gauge invariant, and the anomalies are cancelled by the cross terms of the gauge fields <inline-formula><tex-math notation="LaTeX" id="ImEquation208"><![CDATA[$A$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation209"><![CDATA[$A_{\star}$]]></tex-math></inline-formula>. This means that the parity-odd part of the cross terms corresponds to the Chern&#x2013;Simons term. Thus the parity-odd part of the cross terms vanishes if the anomaly cancellation condition is satisfied.</p>
</sec>
</body>
<back>
<ack><title>Acknowledgements</title>
<p>The author would like to thank Takeo Moroi and Natsumi Nagata for helpful discussion and advice.</p>
</ack>
<sec id="SEC"><title>Funding</title>
<p>Open Access funding: SCOAP<inline-formula><tex-math notation="LaTeX" id="ImEquation210"><![CDATA[$^3$]]></tex-math></inline-formula>.</p>
</sec>
<fn-group>
<title>Footnotes</title>
<fn id="FN1"><label>1</label><p>We also assume that <inline-formula><tex-math notation="LaTeX" id="ImEquation211"><![CDATA[$A$]]></tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX" id="ImEquation212"><![CDATA[$A_{\star}$]]></tex-math></inline-formula> have the same winding number so that <inline-formula><tex-math notation="LaTeX" id="ImEquation213"><![CDATA[$\epsilon + \epsilon_{\star}$]]></tex-math></inline-formula> does not have zero eigenvalues (see the Appendix in Ref. [<xref ref-type="bibr" rid="B7">7</xref>]).</p></fn>
</fn-group>
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