Abstract
We discuss invertible and non-invertible topological condensation defects arising from gauging a discrete higher-form symmetry on a higher codimensional manifold in spacetime, which we define as higher gauging. A q-form symmetry is called p-gaugeable if it can be gauged on a codimension-p manifold in spacetime. We focus on 1-gaugeable 1-form symmetries in general 2+1d QFT, and gauge them on a surface in spacetime. The universal fusion rules of the resulting invertible and non-invertible condensation surfaces are determined. In the special case of 2+1d TQFT, every (invertible and non-invertible) 0-form global symmetry, including the \({\mathbb {Z}}_2\) electromagnetic symmetry of the \({\mathbb {Z}}_2\) gauge theory, is realized from higher gauging. We further compute the fusion rules between the surfaces, the bulk lines, and lines that only live on the surfaces, determining some of the most basic data for the underlying fusion 2-category. We emphasize that the fusion “coefficients” in these non-invertible fusion rules are generally not numbers, but rather 1+1d TQFTs. Finally, we discuss examples of non-invertible symmetries in non-topological 2+1d QFTs such as the free U(1) Maxwell theory and QED.
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Notes
For the most part of this paper, we only consider relativistic quantum systems in Euclidean signature, in which case the distinction between an operator that acts on the Hilbert space and a defect that extends in time is not very sharp. We will therefore use these two terms interchangeably. In non-relativistic systems, however, global symmetries are not necessarily generated by topological operators. Furthermore, the distinction between an operator and a defect is important. For instance, see [2] for a recent discussion that emphasizes this distinction in certain non-relativistic systems.
In Sect. 6, we will discuss examples of these defects where they are realized as the condensation of a Higgs field that only live on a higher codimensional manifold. These examples include the U(1) Maxwell theory, the U(1) Chern–Simons theory, and the \({\mathbb {Z}}_2\) gauge theory. This Higgs presentation of the condensation defect justifies the terminology at least in the above examples.
The observables of a bosonic/non-spin QFT do not require a choice of the spin structure. In contrast, a fermionic/spin QFT can only be defined on spin manifolds and its observables depend on the choice of the spin structure.
In contrast, a \({\mathbb {Z}}_2\) symmetry generated by a semion or an anti-semion is not even 1-gaugeable, and the would-be condensation defect is inconsistent.
Mathematically, d-dimensional topological defects form a module over the fusion ring of d-dimensional TQFTs. This is because given a d-dimensional topological defect we can stack a decoupled d-dimensional TQFT to it and get another topological defect.
We thank T. D. Décoppet for pointing out these reference to us.
Here and throughout we define a q-form symmetry to be a symmetry generated by a codimenion-\((q+1)\) topological operator, rather than by the requirement that it acts on q-dimensional obejcts. For an ordinary q-form symmetry, the two definitions coincide since the action of the symmetry on the charged objects is given by the canonical linking [1]. Condensation defects, however, do not act by canonical linkings, and we need to clarify which definition we are using. We thank Daniel Harlow for discussions on related points.
In this paper, as it is common in the condensed matter physics literature, we only restrict ourselves to robust TQFTs with no nontrivial local operators. This excludes BF theories of a 2-form gauge field and a compact scalar, which describes symmetry-breaking phases.
In fact, in the context of 2+1d SET, it is common that the global symmetries act nontrivially in the microscopic model, but act trivially both on the line defects and the local operators in the continuum TQFT limit.
Here we assume L is a simple line, i.e., it cannot be decomposed into non-negative linear combinations of other lines. Also, throughout the paper, we assume that the only bulk topological local operator is the identity operator.
In the current paper, we only determine the action of the surface defects (which include the 0-form symmetries) on the topological lines (i.e., the low-energy limit of the anyons). We leave the freedom in choosing the symmetry fractionalization class, which is an essential piece of data in SET and in the G-crossed modular tensor category, for future studies.
One needs to choose an appropriate boundary condition, such as the topological Dirichlet boundary condition, for the discrete gauge fields in defining such an interface.
In the condensed matter literature [84,85,86] in 2+1d, gauging a 1-form symmetry in a codimension-0 region is commonly referred to as anyon condensation. For this reason, it is natural to define the gauging of a higher-form symmetry on a higher codimensional manifold as higher condensation. See also footnote 2 for further justification of this terminology.
The only exception is in Sect. 6.6, where we discuss higher gauging in QED with a Dirac fermion.
The set of topological lines in a non-topological QFT only forms a braided tensor category, but not necessarily a modular tensor category. Generally, there are other non-topological lines that have nontrivial correlation functions with the topological lines. For example, 2+1d QED with a charge 2 scalar has a non-anomalous \({\mathbb {Z}}_2\) 1-form global symmetry, which forms a braided fusion category that is not modular. The line charged under this \({\mathbb {Z}}_2\) 1-form symmetry is a non-topological Wilson line.
For more general non-invertible lines, the topological spin is defined as \(\theta (a) = (R^{a, {\bar{a}}}_1)^{-1}\) where \({\bar{a}}\) is the orientation-reversal of a.
Because of this relation, B(a, b) is sometimes referred to as the double-braiding phase (or monodromy phase), and R as the braiding. We will loosely refer to both of them as braiding.
We will sometimes suppress the dependence of \(S(\Sigma )\) on the 2-dimensional manifold \(\Sigma \) and write it simply as S.
Note that generally there is no canonical way to gauge a 1-form symmetry on a surface, similar to the situation of gauging in 1+1d. In other words, the choice of the discrete torsion forms a torsor, rather than a group with a natural identity. For example, see the discussion around equation (5.34).
Throughout the paper, L always denotes a general, not necessarily topological line, while a or \(\eta ^a\) denote topological lines.
Quantum symmetry is also known as the dual or the orbifold symmetry.
See [3] for a review and generalizations to the cases of gauging non-abelian discrete symmetries and non-invertible lines.
More precisely, (3.10) specifies a junctions between a and the higher quantum symmetry lines on S.
These maps are called \(\alpha \)-induction in the mathematical literature, and are denoted by \(\alpha ^+(a) = a \times S\) and \(\alpha ^-(a) =S \times a\). They first appeared in subfactor theory [99, 100], and then in category theory [101, 102]. Finally, for their interpretation in terms of topological defects see [7, 15, 103].
This is because \(b\times S\) and \(S \times a\) are simple lines (i.e., they cannot be decomposed into other lines living on the surface), therefore they have a junction between them if and only if they are identical. For general non-invertible topological lines \(\ell ,\ell '\) we have \(S \cdot \ell = \sum _{\ell '} \textrm{dim Hom}(\ell ' \times S, S \times \ell ) \, \ell '\).
This can also be seen using (3.3) as follows. Since \(1=B(\eta , \eta ^2)= B(\eta ,\eta )^2 = 1/\theta (\eta )^4\), we find that \(\theta (\eta )\) must be a fourth root of unity.
Gauging a fermion line in the whole spacetime results in a spin QFT. Since we only consider non-spin QFT in most of this paper, we do not allow ourselves to gauge a fermion line in the whole spacetime. Instead, we will see momentarily that we can gauge the fermion line on a 2-dimensional surface, which gives a topological surface defect in a non-spin QFT.
We thank Po-Shen Hsin for pointing this reference to us.
As discussed below (2.1), \(P_+\) can be thought of as the condensation of a 0-form symmetry U on a codimension-1 manifold.
This is because the cohomology group classifying the anomaly of a \({\mathbb {Z}}_N\) 0-form symmetry is given by \(H^4(B{\mathbb {Z}}_N,U(1))=1\), which is trivial.
Compared to the general discussion in Sect. 3.1, the labels \(a,b,\ldots \) for the invertible topological lines here and below are additive rather than multiplicative. We hope this change of convention will not cause too much confusions.
This is related to the spin selection rule in 1+1d CFT. In [4, 17, 97], it is shown that an ordinary \({\mathbb {Z}}_N\) global symmetry in 1+1d is anomaly-free if and only if the operator living at the end of the line (e.g., the disorder operator) has Lorentz spin \(s=h-{\bar{h}}\in {\mathbb {Z}}/N\).
In general the quantum symmetry might be a non-trivial extension of \({\mathbb {Z}}_N/{\mathbb {Z}}_n\) by \(\widehat{{\mathbb {Z}}}_n\). As explained in [3, Section 5.3.2] (see also [105]), the extension is given by the mixed anomaly between the \({\mathbb {Z}}_n\) subgroup and \({\mathbb {Z}}_N/{\mathbb {Z}}_n\) before gauging. However, this anomaly is trivial in this case since the \({\mathbb {Z}}_N\) 1-form symmetry is 1-gaugeable.
A simple example is to choose \(N=4\) and \(n=2\). The order 2 higher quantum symmetry line \({\hat{\eta }}_2{{\tilde{\eta }}}_2\) is anomalous and depends on \(\gamma \) modulo 4, rather than 2.
The symmetry groups \({\mathbb {Z}}_N/{\mathbb {Z}}_n\) and \({\widehat{{\mathbb {Z}}}}_n\) are individually anomaly free and there is only a mixed anomaly between them in the sense that the product group \({\mathbb {Z}}_N/{\mathbb {Z}}_n \times {\widehat{{\mathbb {Z}}}}_n\) is anomalous.
Here \(\gamma = 0 \mod n\) for a 1-cycle \(\gamma \) means that there exists another 1-cycle \(\gamma '\in H_1(\Sigma , {\mathbb {Z}})\) such that \(\gamma = n \gamma '\).
When \(a=a'\), this fusion rule simplifies to
$$\begin{aligned} \begin{aligned} {\hat{\eta }}_n^a \times {\hat{\eta }}_{n'}^{a} = \left( {\mathcal {Z}}_{\textrm{gcd}(n,n',k\ell )} \right) \, {\hat{\eta }}_{\frac{\textrm{gcd}(n,n',k\ell )nn'}{\textrm{gcd}(n,n')^2}}^a \,. \end{aligned} \end{aligned}$$(5.26)Also when \(k=0\) (i.e., when the \({\mathbb {Z}}_N\) symmetry is non-anomalous), the fusion simplifies:
$$\begin{aligned} {\hat{\eta }}_{n}^a \times {\hat{\eta }}_{n'}^{a'} = \left( {\mathcal {Z}}_{\textrm{gcd}(n,n')}, W^{a-a'} \right) \, {\hat{\eta }}_{\textrm{lcm}(n,n')}^{\frac{pan'+p'a'n}{\textrm{gcd}(n,n')}} \,. \end{aligned}$$(5.27)In fact, whenever gcd\((N,k)=1\), \(S_N\) and \(\eta \) form a dihedral group \(D_{2N}\) even when N is not prime, but there are additional non-invertible surfaces \(S_n\) with n|N.
Since \(1=B(\eta _1^{N_1},\eta _2)= B(\eta _1,\eta _2)^{N_1}\) and similarly \(1=B(\eta _1,\eta _2)^{N_2}\), we see that \(k_{12}\in {\mathbb {Z}}_{\text {gcd}(N_1,N_2)}\).
The intersection number \(\langle \gamma _1,\gamma _2\rangle \in {\mathbb {Z}}_{\text {gcd}(N_1,N_2)}\) is defined by viewing \(\gamma _1, \gamma _2\) as elements in \(H_1(\Sigma , {\mathbb {Z}}_{\text {gcd}(N_1,N_2)})\).
Note that this is compatible with the braiding phases in (5.30), since \(R^{a,b}_{a+b}R^{b,a}_{a+b} = B(a,b) \equiv B(\eta _1^{a_1}\eta _2^{a_2}, \eta _1^{b_1}\eta _2^{b_2}) \).
The duality is given by \(dA\sim \star d \phi \), where \(\phi \) is a compact scalar. See, for instance, [108].
On the other hand, it has a mixed anomaly with the magnetic U(1) 0-form symmetry.
Relatedly, this algebra admits a 1-dimensional representation \(\langle S_N \rangle = N\).
SHS would like to thank Yichul Choi and Ho Tat Lam for enlightening discussions on this point and collaborations on a related project [69] in 3+1d.
By noting \(N = \ell nn' / \textrm{gcd}(n,n')\), we see that \(\textrm{gcd}(N/n,N/n') = \ell \), \(\textrm{gcd}:(n,N/n') = {\textrm{gcd}(n,n',\ell ) n \over \textrm{gcd}(n,n')}\) and \(\textrm{gcd}(n',N/n) = {\textrm{gcd}(n,n',\ell ) n' \over \textrm{gcd}(n,n')}\). Using these identities we find (6.13) is equivalent to the fusion rule presented in [103].
Our action differs from [103] by the last term. As a result, their action does not have the full left and right gauge symmetries implemented by \(\alpha _L,\alpha _R\), while ours does.
In Appendix A.2 we derive the fusion rule for the surfaces in the more general \({\mathbb {Z}}_p\) gauge theory with prime p. The translation between the notation here and there is given by:
$$\begin{aligned} S_{\textrm{e}}= S_{{\mathbb {Z}}_{2}^{(\infty )}} , \quad S_{\textrm{m}}= S_{{\mathbb {Z}}_{2}^{(0)}} , \quad S_\psi = S_{{\mathbb {Z}}_{2}^{(1)}} , \quad S_{\textrm{em}} = S_{({\mathbb {Z}}_2 \times {\mathbb {Z}}_2)^{(\infty )}} , \quad S_{\textrm{me}}= S_{({\mathbb {Z}}_2 \times {\mathbb {Z}}_2)^{(0)}}. \end{aligned}$$We slightly abuse the notation and use \(\vert {B} \rangle \) for both the abstract boundary condition and also the boundary state on \(\Sigma \), i.e. \(\vert {B} \rangle \in {\mathcal {H}}(\Sigma )\).
\(\Lambda _{\textbf{A}}(\Sigma )\) and \(\Lambda _{\textbf{B}}(\Sigma )\) are maximal isotropic subgroups of \(H_1(\Sigma ,{\mathbb {Z}}_2)\) that are called Lagrangian subgroups in the literature.
The insertion of anyons gives a delta function, and the normalization is given by the partition function on \({\overline{Y}} \sqcup _\Sigma Y = (S^2 \times S^1)^{\# g}\) where \(\#\) denotes connected sum. Note that \(Z\left( (S^2 \times S^1)^{\# g} \right) = { Z( S^2 \times S^1 )^g \over Z( S^3)^{g-1}} = 2^{g-1}\), since \(Z(S^3) = 1/2\).
Note that the composite boundary states \(\vert {B_{\textrm{e}}, \gamma } \rangle \) for different \(\gamma \) span a basis for the Hilbert space on \(\Sigma \) (and similarly for \(\vert {B_{\textrm{m}}, \gamma } \rangle \)). The basis \(|\alpha _{\textrm{e}},\alpha _{\textrm{m}}\rangle \) correspond to choosing a Lagrangian subgroup of \(H_1(\Sigma ,{\mathbb {Z}})\) (i.e. the \({\textbf{A}}\)-cycles) whereas the basis \(\vert {B_{\textrm{e}}, \gamma } \rangle \) correspond to the Lagrangian subgroup of anyons generated by \(\eta _{\textrm{e}}\).
SHS thanks Pranay Gorantla, Ho Tat Lam, and Nati Seiberg for discussions on the Lagrangians of boundary conditions in discrete gauge theory.
Throughout the paper, we have assumed the 2+1d QFT to be a bosonic QFT, with the exception of this subsection. Most of our previous results for the bosonic QFT still apply here.
In the UV, there are additional global symmetries including the magnetic U(1) symmetry and the time-reversal symmetry. We will not discuss them here.
More precisely, the algebra needs to be both commutative and separable with a unique unit. Such an algebra is the same as the connected \(\acute{e}\)tale algebra of [102, Definition 3.1] and rigid algebra with trivial spin of [127, Section 3]. Here we refer to them simply as commutative algebra objects.
This definition of the algebra object was originally introduced in [101, 128]. In the literature, it is also called the symmetric special Frobenius algebra in [7, 129] and the \(\Delta \)-separable Frobenius algebra in [63]. See [3, 41] for recent discussions in the context of non-invertible 0-form symmetries in 1+1d.
There are nontrivial SETs associated with symmetries that do not permute the lines but have a nontrivial symmetry fractionalization class (see, for instance, [76]). We do not discuss the freedom of choosing a symmetry fractionalization class in this paper.
Mathematically, two algebras \({{\mathcal {A}}}\) and \({{\mathcal {A}}}'\) are Mortia equivalent iff the category of (right) \({{\mathcal {A}}}\)-modules and \({{\mathcal {A}}}'\)-modules are the same (left) module categories over the modular tensor category of all topological lines [128]. The condensation defects only depend on the Morita equivalent class of the algebra objects [63, 129].
Here we only consider unitary 2+1d TQFTs with no non-trivial local operator.
In the context of fully extended TQFT, the necessary and sufficient condition for existence of a topological boundary condition was proven rigorously in [131].
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Acknowledgements
We thank M. Cheng, Y. Choi, C. Cordova, T. D. Décoppet, T. Dumitrescu, P. Gorantla, D. Harlow, P.-S. Hsin, J. Kaidi, R. Kobayashi, Z. Komargodski, H. T. Lam, M. Metlitski, R. Radhakrishnan, N. Seiberg, and Y. Wang for interesting discussions. We are grateful to Y. Choi, D. Delmastro, A. Kapustin, R. Kobayashi, and K. Ohmori for helpful comments on a draft. SHS would particularly like to thank Y. Choi and H. T. Lam for numerous enlightening discussions on a related project [69] on higher gauging in 3+1d. SHS would also like to thank P. Gorantla, H. T. Lam, and N. Seiberg for discussions on anyon condensations. KR would like to thank T. Dumitrescu for many useful discussions on this topic. The work of KR is supported by the Mani L. Bhaumik Institute for Theoretical Physics. SS is supported in part by the Simons Foundation grant 488657 (Simons Collaboration on the Non-Perturbative Bootstrap). The authors of this paper were ordered alphabetically.
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A More on the Fusion Rules
A More on the Fusion Rules
1.1 A.1 Fusion rules from the higher gauging of \({\mathbb {Z}}_N\) 1-form symmetries
In this appendix we will derive the fusion rule (5.22) between the higher quantum symmetry lines on the condensation surfaces that arise from a 1-gaugeable \({\mathbb {Z}}_N\) 1-form symmetry. The 0-anomaly of the 1-gaugeable \({\mathbb {Z}}_N\) 1-form symmetry is labeled by an integer k (see Sect. 5.1).
As a warm up, we fist derive the fusion rule (5.13) between the condensation surfaces \(S_n\), which come from the higher gauging of the \({\mathbb {Z}}_n\) 1-form symmetry subgroup with n|N. We will place the condensation surfaces on a genus-g surface \(\Sigma _g\) with generating 1-cycles \({\textbf{A}}_{i=1,\dots ,g},{\textbf{B}}_{i=1,\dots ,g} \in H_1(\Sigma _g, {\mathbb {Z}}_N)\).
Let \(n,n'\) be two divisors of N. The fusion of the corresponding condensation surfaces \(S_n\) and \(S_{n'}\) is
Below we will do a change of variables on \(\mu _i,\nu _i,\mu '_i,\nu '_i\) in order to simplify the above expression.
To proceed, we first note that for any pair of numbers \((\mu ,\mu ') \in {\mathbb {Z}}_n \times {\mathbb {Z}}_{n'}\) we can do the change of variable
for \(\alpha \in \left\{ 1, \dots , \textrm{lcm}(n,n') \right\} \) and \(\lambda \in {\mathbb {Z}}_{\textrm{gcd}(n,n')}\), where
for some fixed integers p and \(p'\). Note that (A.2) defines a map from \(\left\{ 1, \dots , \textrm{lcm}(n,n') \right\} \times {\mathbb {Z}}_{\textrm{gcd}(n,n')}\) to \({\mathbb {Z}}_n \times {\mathbb {Z}}_{n'}\) whose inverse is given by
Therefore we conclude that the map is bijective and hence the change of variable is legitimate.
Now let us apply the change of variable (A.2) to \(\mu _i,\mu _i',\nu _i,\nu _i'\) and write
where \(\alpha _i,\beta _i \in \left\{ 1, \dots , \textrm{lcm}(n,n') \right\} \), \(\lambda _i,\rho _i \in {\mathbb {Z}}_{\textrm{gcd}(n,n')}\), and \(pn'+p'n=\textrm{gcd}(n,n')\) for some fixed integers p and \(p'\). Using these new set of variables we get
where \(\ell = \frac{N}{\textrm{lcm}(n,n')}\). Summing over \(\lambda _i,\rho _i \in {\mathbb {Z}}_{\textrm{gcd}(n,n')}\) gives the Kronecker deltas
which forces \(\alpha _i\) and \(\beta _i\) to be divisible by \(\frac{\textrm{gcd}(n,n')}{\textrm{gcd}(n,n',k\ell )}\). Therefore we do the replacement \(\alpha _i,\beta _i \mapsto \frac{\textrm{gcd}(n,n')}{\textrm{gcd}(n,n',k\ell )} {\bar{\alpha }}_i, \frac{\textrm{gcd}(n,n')}{\textrm{gcd}(n,n',k\ell )}{\bar{\beta }}_i\) for \(1 \le {\bar{\alpha }}_i,{\bar{\beta }}_i \le \frac{\textrm{gcd}(n,n',k\ell )nn'}{\textrm{gcd}(n,n')^2}\) and get
We conclude that the fusion algebra is
where \(\left( {\mathcal {Z}}_{n}\right) \) stands for the 1+1d \({\mathbb {Z}}_n\) gauge theory.
Now we will derive the fusion between the higher quantum symmetry lines living on the surfaces (5.22). We put the composite defects \({\hat{\eta }}_{n}^a {\tilde{\eta }}_{n}^b\) of (5.21) on \(({\bar{\gamma }}, \Sigma )\) and perform the computations covariantly without specifying a basis for \(H_1(\Sigma , {\mathbb {Z}})\):
Next, we apply the same change of variable as in (A.2) to \(\gamma \in H_1(\Sigma ,{\mathbb {Z}}_{n})\) and \(\gamma ' \in H_1(\Sigma ,{\mathbb {Z}}_{n'})\). We write
for \(\alpha \in \left\{ \sum _{i,j} \alpha _i {\textbf{A}}_i + \beta _j {\textbf{B}}_j \in H_1(\Sigma ,{\mathbb {Z}}) \mid \alpha _i,\beta _j \in \{ 1, \dots , \textrm{lcm}(n,n') \} \right\} \) and \(\lambda \in H_1(\Sigma ,{\mathbb {Z}}_{\textrm{gcd}(n,n')})\), where the integers p and \(p'\) satisfy \(p n' + p'n = \textrm{gcd}(n,n')\). Here \({\textbf{A}}_{i},{\textbf{B}}_{j}\) are a fixed set of generators for \(H_1(\Sigma ,{\mathbb {Z}})\).
In terms of these new variables we get:
where \(c=a-kb'\), \(c'=a'+kb\), and \(\ell = {N \over \textrm{lcm}(n,n')}\). The sum over \(\lambda \) gives a Kronecker delta, multiplied by \(|H_1(\Sigma ,{\mathbb {Z}}_{\textrm{gcd}(n,n')})|\), that enforces \(\alpha \) to satisfy
Thus, we can rewrite the fusion as
If there is no solution to the constraint (A.13) we get zero on the righthand side. Otherwise, any solution can be written as
where
and \(\big ({k\ell \over \textrm{gcd}(n,n',k\ell )}\big )^{-1}_{N \over x\ell } \in ({\mathbb {Z}}_{N \over x\ell })^\times \) is the multiplicative inverse of \({k\ell \over \textrm{gcd}(n,n',k\ell )}\) modulo \({N \over x\ell } = {\textrm{gcd}(n,n') \over \textrm{gcd}(n,n',k\ell )}\). The multiplicative inverse always exists since \({k\ell \over \textrm{gcd}(n,n',k\ell )}\) is coprime with respect to \({\textrm{gcd}(n,n') \over \textrm{gcd}(n,n',k\ell )}\).
We substitute (A.15) into (A.14) to get
Comparing this with (5.21) we find
The fusion coefficient \(\delta _{(c-c'){\bar{\gamma }} \,\text { mod gcd}(n,n',k\ell ), 0} \, \sqrt{|H_1(\Sigma ,{\mathbb {Z}}_{\textrm{gcd}(n,n',k\ell )})|}\) is the partition function of the 1+1d \({\mathbb {Z}}_{\textrm{gcd}(n,n',k\ell )}\) gauge theory on \(\Sigma \) with the Wilson line \(W^{c-c'}\) on \({\bar{\gamma }}\) that we denote by \(({\mathcal {Z}}_{\textrm{gcd}(n,n',k\ell )}, W^{c-c'})({\bar{\gamma }},\Sigma )\). This can be seen by
We therefore conclude that
1.2 A.2 Fusion rules in the \({\mathbb {Z}}_p\) gauge theory
In this appendix we give the detail of the computation for the condensation surfaces in the \({\mathbb {Z}}_p\) gauge theory in Sect. 6.4.
Let us choose \(f,f' \in {\mathbb {Z}}_p\) and compute the fusion between \(S_{{\mathbb {Z}}_p \times {\mathbb {Z}}_p, f}\) and \(S_{{\mathbb {Z}}_p \times {\mathbb {Z}}_p, f'}\)
To simplifying the RHS, there are qualitatively two different cases depending on whether \(f+f'+1 = 0 \pmod {p}\) or not:
Case 1 (\(f+f'+1\ne 0\)): The sum over \(\gamma '_2\) results in the Kronecker delta function factor \({|H_1(\Sigma , {\mathbb {Z}}_p)|} \, \delta _{f\gamma _1 - [f+f'+1]\gamma '_1, 0} \) which sets \(\gamma '_1 = \frac{f}{f+f'+1}\gamma _1\) and we get
This translates to the invertible fusion rule \( S_{{\mathbb {Z}}_p \times {\mathbb {Z}}_p, f} \times S_{{\mathbb {Z}}_p \times {\mathbb {Z}}_p, f'} = S_{{\mathbb {Z}}_p \times {\mathbb {Z}}_p, \frac{ff'}{f+f'+1}}\). If we do the crucial change of variable \(f=\frac{1}{m-1}\), the fusion rule simplifies to
Case 2 (\(f+f'+1=0\)): In this case we can perform the sum over \(\gamma '_1\) and \(\gamma '_2\) to get
For reasons that become clear later, we have introduced a notation where \(S_{{\mathbb {Z}}_{p}^{(\infty )}}\) and \(S_{{\mathbb {Z}}_{p}^{(0)}}\) correspond to the higher gauging of the first and second \({\mathbb {Z}}_p\) subgroups (generated by \(\eta _1\) and \(\eta _2\)), respectively.
Putting everything together the fusion rules can be summarized as:
where we have introduced another notation of \(S_{{\mathbb {Z}}_p \times {\mathbb {Z}}_p, \infty } \equiv 1\). Therefore, we see that the surfaces \( S_{{\mathbb {Z}}_p \times {\mathbb {Z}}_p, f} \) with \(f\ne 0,-1\) form a cyclic group \({\mathbb {Z}}_{p-1}\) under fusion. In contrast, the surface defects \( S_{{\mathbb {Z}}_p \times {\mathbb {Z}}_p, 0} \) and \( S_{{\mathbb {Z}}_p \times {\mathbb {Z}}_p, -1} \) are non-invertible.
The \({\mathbb {Z}}_p \times {\mathbb {Z}}_p\) 1-form symmetry has \(p+1\) \({\mathbb {Z}}_p\) subgroups. Given any non-zero element \((m_1,m_2) \in {\mathbb {Z}}_p \times {\mathbb {Z}}_p\) associated with the topological line \(\eta _1^{m_1} \eta _2^{m_2}\), we can take the \({\mathbb {Z}}_p\) subgroup generated by it and denote it by \({\mathbb {Z}}_p^{(m_1/m_2)}\). Note that \({\mathbb {Z}}_{p}^{(m)}\) only depend on \(m=\frac{m_1}{m_2} \pmod {p}\), where \(m=\infty \) and \(m=0\) corresponds to the first and second \({\mathbb {Z}}_p\) subgroups which are 0-gaugeable. Therefore, from the results of Sect. 5.1, \(S_{{\mathbb {Z}}_{p}^{(\infty )}}\) and \(S_{{\mathbb {Z}}_{p}^{(0)}}\) are non-invertible and the rest are all invertible order 2 defects.
Denote the surface defect from the higher gauging of \({\mathbb {Z}}_{p}^{(m)}\) by
The fusion of this surface with itself has been computed in Sect. 5. Thus let us take \(m \ne m'\) and compute the fusion of \(S_{{\mathbb {Z}}_{p}^{(m)}}\) with \(S_{{\mathbb {Z}}_{p}^{(m')}}\):
Take \(m=m_1/m_2\) and \(f= 1/(m'-1)\), we have
and
Putting everything together, we have derived the fusion rule (6.70) of the surfaces, which includes the invertible \(D_{2(p-1)}\) 0-form symmetry, of the 2+1d \({\mathbb {Z}}_p\) gauge theory.
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Roumpedakis, K., Seifnashri, S. & Shao, SH. Higher Gauging and Non-invertible Condensation Defects. Commun. Math. Phys. 401, 3043–3107 (2023). https://doi.org/10.1007/s00220-023-04706-9
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DOI: https://doi.org/10.1007/s00220-023-04706-9