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Non-invertible Condensation, Duality, and Triality Defects in 3+1 Dimensions

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Abstract

We discuss a variety of codimension-one, non-invertible topological defects in general 3+1d QFTs with a discrete one-form global symmetry. These include condensation defects from higher gauging of the one-form symmetries on a codimension-one manifold, each labeled by a discrete torsion class, and duality and triality defects from gauging in half of spacetime. The universal fusion rules between these non-invertible topological defects and the one-form symmetry surface defects are determined. Interestingly, the fusion coefficients are generally not numbers, but 2+1d TQFTs, such as invertible SPT phases, \({\mathbb {Z}}_N\) gauge theories, and \(U(1)_N\) Chern-Simons theories. The associativity of these algebras over TQFT coefficients relies on nontrivial facts about 2+1d TQFTs. We further prove that some of these non-invertible symmetries are intrinsically incompatible with a trivially gapped phase, leading to nontrivial constraints on renormalization group flows. Duality and triality defects are realized in many familiar gauge theories, including free Maxwell theory, non-abelian gauge theories with orthogonal gauge groups, \({{{\mathcal {N}}}}=1,\) and \({{{\mathcal {N}}}}=4\) super Yang-Mills theories.

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Notes

  1. Throughout out this paper, we will focus on relativistic QFT in Euclidean signature, and we will use the terms “operator” and “defect” interchangeably.

  2. All the condensation defects we will encounter in this paper are non-invertible. More generally, an anomalous higher-form symmetry can give rise to an invertible condensation defect. For example, a one-gaugeable fermion line in 2+1d leads to a \({\mathbb {Z}}_2\) condensation surface under one-gauging [19] (see also [55, 65]).

  3. For defects of any dimensionality, when the fusion “coefficient” is a \({\mathbb {Z}}_N\)-valued topological scalar theory that gives N trivial vacua on any manifold, it corresponds to a fusion multiplicity N. In general, we can decorate a simple object \(x(\Sigma )\) that supports on submanifold \(\Sigma \) by a lower dimensional TQFT supported on \(\Sigma \). If such lower-dimensional TQFT has a non-trivial topological domain wall, then \(\text {Hom}(x,x)\not \cong {\mathbb {C}}\) and the decoration produces a non-simple object.

  4. On the other hand, to be precise, the duality defect \({{{\mathcal {D}}}}_2\) should really be called a “quadrality defect” since \(S^2=C\) and \(S^4=1\), where C is the charge conjugation.

  5. In some of the examples we have analyzed in this paper, the 2+1d TQFT coefficients arise as the boundary theories of 3+1d invertible TQFTs. In these cases we have implicitly chosen a preferred framing for the 2+1d worldvolume of the defect coming from the embedding into the 3+1d bulk.

  6. Denote the two-form \({\mathbb {Z}}_N\) gauge fields for the \({\mathbb {Z}}_N^{(1)}\) one-form symmetries by \(B,B'\), then this minimal mixed local counterterm is \(\frac{2\pi i}{N}\int B\cup B'\).

  7. The \({\mathbb {Z}}^{(1)}_N\) one-form symmetry in a 3+1d theory is potentially anomalous as can be seen, for instance, from the nontrivial bordism group \(\Omega ^{\text {SO}}_5(B^2 {\mathbb {Z}}_2) \cong {\mathbb {Z}}_2 \times {\mathbb {Z}}_2\) [72] where one of the \({\mathbb {Z}}_2\) factors corresponds to a possible anomaly for the \({\mathbb {Z}}^{(1)}_2\) one-form symmetry (the other \({\mathbb {Z}}_2\) factor corresponds to the \(w_2 w_3\) gravitational anomaly). This particular anomaly vanishes for spin theories since \(\Omega ^{\text {Spin}}_5(B^2 {\mathbb {Z}}_2)\) is trivial.

  8. Throughout the paper (with an exception in Sect. 6.1), we use the upper case letters to denote classical background fields, and the lower case letters to denote dynamical fields.

  9. In both cases the partition function is equal to \(e^{2\pi i \sigma (X) /8}\), modulo Euler counterterms, where \(\sigma (X)\) is the signature of the manifold X if we assume that the integral cohomology of the spacetime manifold is torsionless (see, for example, [1, 73, 76]).

  10. The number \(Q(M,\Sigma )\) is non-trivial only if \(\Sigma \) is given by a discrete \({\mathbb {Z}}_N\) cycle, i.e., \(\partial \Sigma =N\gamma \) for some one-cycle \(\gamma \), where \(\beta (a)=\text {PD}:(\gamma )\) mod N. Then \(Q(M,\Sigma )\) equals the intersection number of \(\Sigma \) and \(\gamma \), or N times the linking form evaluated on the torsion cycle \(\gamma \). When \(N=2\), using \(\beta (a)=a^2\) one finds the number equals to the triple intersection number of \(\Sigma \).

  11. We thank Sahand Seifnashri for the discussions related to the orientation reversal of defects. See [19] for more discussions.

  12. This is related to the fact that we can take the “square root” of the orientation-reversal-invariant condensation defects, but not those that are not invariant under the orientation reversal. We will discuss this more in later sections.

  13. To be more precise, we use the integer BF lattice presentation of discrete higher-form gauge theories in [77, 78] (see also [22]).

  14. Generally, any two defects which are different only in the presence of such transverse junctions are considered as equivalent defects, i.e., they are isomorphic but not identical. This is expected to be the higher categorical analogue of the familiar fact in the 1+1d fusion category symmetry case where one has the freedom to choose basis vectors for junction vector spaces.

  15. We will set \(B=0\) since the coupling to B contains information about the junction between the \(({\mathcal {Z}}_N)_0\) theory and the symmetry defect, which we do not discuss for parallel fusion.

  16. To be precise, this \(({\mathcal {Z}}_N)_0\) gauge theory differs from the previous one in the presence of a transverse junction with \(\eta \), which we ignore as we explained at the end of Sect. 2.1.

  17. Since we assume that M has a neighborhood \(M \times I\) inside the spacetime manifold X, M is spin as long as X is spin.

  18. In general, two defects of the same dimensionalities can be fused in the presence of such higher codimensional topological operators living inside them [19, 22, 49, 88]. From this more general perspective, the fusion between \({\mathcal {N}}\) and \(\eta \) can be thought of as fusing the trivial surface operator inside \({\mathcal {N}}\) with a nontrivial surface operator given by \(\eta \) inside a trivial three-dimensional defect. A simple analogy can be made in a 1+1d QFT having a non-invertible symmetry described by a fusion category. Consider two topological line defects \({\mathcal {L}}_1\) and \({\mathcal {L}}_2\) in a 1+1d theory which are not necessarily simple, and also the morphisms \(\alpha _1: {\mathcal {L}}_1 \rightarrow {\mathcal {L}}_1\) and \(\alpha _2: {\mathcal {L}}_2 \rightarrow {\mathcal {L}}_2\) inside these lines, which are topological point operators living on these lines. The morphisms \(\alpha _1\) and \(\alpha _2\) can be represented by finite-dimensional matrices, and the fusion \(\alpha _1 \times \alpha _2: {\mathcal {L}}_1 \times {\mathcal {L}}_2 \rightarrow {\mathcal {L}}_1 \times {\mathcal {L}}_2\) is simply given by the tensor product of two matrices, and it defines a topological point operator living on the line \({\mathcal {L}}_1 \times {\mathcal {L}}_2\). If we let \(\alpha _1 = \text {Id}_{{\mathcal {L}}_1}\) to be the trivial point operator and \({\mathcal {L}}_2 = 1\) to be the trivial line defect, then the fusion can be thought as the fusion between the topological line defect \({\mathcal {L}}_1\) and the topological local operator \(\alpha _2\). We thank Kantaro Ohmori for discussions on this point.

  19. In [19], Eq. (4.6) was interpreted as a map from the zero-anomaly to the one-anomaly of a \({\mathbb {Z}}_N^{(1)}\) one-form symmetry in 2+1d.

  20. For the fusion with the condensation defect \({\mathcal {C}}_{\frac{N\ell }{2}}\), one can also use the definition (2.5) to obtain the same results.

  21. We note that the solution is \(p'=4^{-1}(-1\pm y)\) mod N, which satisfies \(\gcd (p',N)=1\), as both \(y+1,y-1\) are coprime with N. Otherwise, \((y+1)(y-1)=y^2-1\) would have a common factor with N, which cannot happen since \(y^2=-3\) mod N and N is odd.

  22. Gauging the \({\mathbb {Z}}_N^{(1)}\times {\mathbb {Z}}_N^{(1)}\) one-form symmetry produces a dual \({\mathbb {Z}}_N^{(1)}\times {\mathbb {Z}}_N^{(1)}\) one-form symmetry, and we turn on background \(B^1,B^2\). In the following we choose the generators for the dual one-form symmetry to be \(\oint b^2,\oint b^1\), but the conclusion does not change if we choose the generators to be \(\oint b^1,\oint b^2\). This corresponds to choosing a different bicharacter under the gauging (see e.g. the discussion below (2.15)). Our results below imply that the triality defect arising from invariance under twisted gauging with this different bicharacter also obstructs a trivially gapped phase.

  23. In contrast to the convention elsewhere in this paper (see Footnote 8), in this subsection we use upper case letters for the dynamical bulk gauge fields, and lower case letters for dynamical gauge fields living on the defects.

  24. We use a different font here to distinguish between \({\mathbb {S}},{\mathbb {T}}\) electromagnetic duality of the Maxwell theory and the ST operations defined in (2.1).

  25. Generally, the worldvolume Lagrangian \(\mathcal{L}_{{{\mathcal {N}}}}[A_L,A_R]\) also depend on other dynamical fields that only live on the defect. We will not write the dependence on the defect fields explicitly.

  26. Here we use a mixed notation where \(a,A_L,A_R\) are represented as U(1) gauge fields and PD\((\Sigma )\) is a \({\mathbb {Z}}_N\) gauge field. We hope this will not cause too much confusion.

  27. Since the theories involved in the duality are Abelian TQFTs, the duality can be proven by matching the spin and the fusion of the lines. The duality map is

    $$\begin{aligned} (q_1,q_2,l)\rightarrow (q_1+q_2,q_1+2q_2,l+q_1)\sim (q_1+q_2,q_1-q_2,l+q_1+q_2)~, \end{aligned}$$
    (6.49)

    where \(q_1,q_2\in {\mathbb {Z}}_6\) labels the charge for the \(U(1)\times U(1)\) gauge groups, and \(l\in {\mathbb {Z}}_2\) labels the transparent fermion line \(\psi ^l=1,\psi \) for \(l=0,1\). We have the identification \((q_1,q_2,l)\sim (q_1+3n,q_2+3\,m,l+n+m)\), \(l\sim l+2\).

  28. The discrete theta angles for \(Spin(4n)/({\mathbb {Z}}_2\times {\mathbb {Z}}_2)\) bundle can be specified by \(n_{11},n_{22},n_{12}\) that take value in \({\mathbb {Z}}_2\) on spin manifolds, with the action [98]

    $$\begin{aligned} \frac{i\pi n_{11}}{2}\int q(w_2^{(1)})+\frac{i\pi n_{22}}{2}\int q(w_2^{(2)})+i n_{12}\pi \int w_2^{(1)}\cup w_2^{(2)}~, \end{aligned}$$
    (6.59)

    where \(w_2^{(1)},w_2^{(2)}\) is the obstruction to lifting the bundle to an Sc(4n), Ss(4n) bundle, respectively. Shifting the theta angle by \(2\pi \) is equivalent to shifting \((n_{11},n_{12},n_{22})\rightarrow (n_{11}+n,n_{12}+n+1,n_{22}+n)\). For even n this is the theory \(PSO(4n)^{n_{12},n_{11}}_{n_{22},n_{12}}\) with \({\mathbb {Z}}_2\) values 0, 1 denoted by \(+,-\), and for odd n this is \(PSO(4n)^{n_{11},n_{12}}_{n_{12},n_{22}}\).

  29. We use the same symbols \({{{\mathcal {D}}}}_2\) for these duality defects (and similarly for the triality defects \({{{\mathcal {D}}}}_3\) below) which arise from gauging a \({\mathbb {Z}}_N^{(1)}\times {\mathbb {Z}}_N^{(1)}\) symmetry, even though we anticipate that these defects may obey different fusion algebras from those discussed in Sects. 34. We hope this will not cause much confusion.

  30. For instance, in 3+1d the SO(8) gauge theory flows to the pure \({\mathbb {Z}}_2\) gauge theory at low energy, which can be represented by a \({\mathbb {Z}}_2\) two-form gauge theory with gauge field b. The coupling to \(B_m\) is

    $$\begin{aligned} i\pi \int b\cup B_m~, \end{aligned}$$
    (6.64)

    and the theory is invariant under stacking \(i \pi \int B_e\cup B_m\) using the field redefinition \(b\rightarrow b+B_e\). If we turn on theta angle (which is present in the Spin(8) gauge theory), then for \(\theta =2\pi k\) with odd k the action has additional \(i\pi \int ( b\cup b+b\cup B_e+B_e\cup B_e)\), which is invariant mod \(2\pi \) under the redefinition \(b\rightarrow b+B_e\), and thus the redefinition still produces \(i\pi \int B_e\cup B_m\) from the total action.

  31. For notational simplicity, we suppress the normalization factor from gauging of the one-form symmetry in this appendix.

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Acknowledgements

We are grateful to M. Cheng, D. Freed, J. Kaidi, R. Kobayashi, K. Ohmori, S. Seifnashri, Y. Zheng for helpful conversations. SHS would particularly like to thank S. Seifnashri for numerous illuminating discussions on a related project [19]. We thank J. Kaidi, G. Zafrir, and Y. Zheng for comments on the first version of the paper. CC is supported by the US Department of Energy DE-SC0021432 and the Simons Collaboration on Global Categorical Symmetries. PSH is supported by the Simons Collaboration on Global Categorical Symmetries. HTL is supported in part by a Croucher fellowship from the Croucher Foundation, the Packard Foundation and the Center for Theoretical Physics at MIT. The authors of this paper were ordered alphabetically.

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Appendices

\( (-1)^{Q}\times U(1)_N \,\hbox {=}\, U(1)_N\)

Let M be an oriented three-manifold. In this appendix, we prove that, for even N, the \(U(1)_{N}\) Chern-Simons theory is invariant under stacking the 2+1d \({\mathbb {Z}}_N^{(0)}\)-SPT given by the Dijkgraaf-Witten term

$$\begin{aligned} \begin{aligned} (-1)^{Q(M,\Sigma )} = \exp \left( {i \pi \over N} \int _M A\cup \delta A\right) , \end{aligned} \end{aligned}$$
(A.1)

where \(A=\)PD\((\Sigma )\) is the Poincaré dual of the surface \(\Sigma \) in M. This \({\mathbb {Z}}_N^{(0)}\)-SPT corresponds to the order 2 element of \(H^3(B{\mathbb {Z}}_N;U(1))\cong {\mathbb {Z}}_N\). More precisely, we mean the following

$$\begin{aligned} \begin{aligned} (-1)^{Q(M,\Sigma )} Z_{U(1)_N} [M ]=Z_{U(1)_N} [M ], \end{aligned} \end{aligned}$$
(A.2)

where \(Z_{U(1)_N}[M]\) is the partition function of \(U(1)_N\) on M. This fact was crucial for the triality fusion rule in (3.10) to be associative, where both the SPT \((-1)^Q\) and the TQFT \(U(1)_N\) appear as the fusion “coefficients” of the defects.

We can schematically write the above equality as

$$\begin{aligned} \begin{aligned} \hbox {``} \, (-1)^Q \times U(1)_N = U(1)_N.\hbox {''} \end{aligned} \end{aligned}$$
(A.3)

Here, \((-1)^Q\), which is an SPT of PD\((\Sigma )\), and \(U(1)_N\), which is a TQFT, are both regarded as special cases of an SET of a \({\mathbb {Z}}_N^{(0)}\) bundle on M, and the product above means the tensor product between two SETs. Indeed, most generally the fusion “coefficients” between two topological defects are SETs (see, for example, [19]).

Using the U(1) gauge field notations, the combined system of the Chern-Simons theory and this SPT phase can be expressed by the following Lagrangian:

$$\begin{aligned} \frac{iN}{4\pi } ada + \frac{iN}{4\pi } AdA + \frac{iN}{2\pi } A d{\tilde{a}} \end{aligned}$$
(A.4)

where a and \({\tilde{a}}\) are dynamical U(1) gauge fields and A is a classical background U(1) gauge field. The first term corresponds to the \(U(1)_{N}\) Chern-Simons theory. In the last term, \({\tilde{a}}\) is a Lagrange multiplier enforcing A to be a \({\mathbb {Z}}_N\) gauge field. The second term is the Dijkgraaf-Witten term \((-1)^{Q(M,\Sigma )}\) for the \({\mathbb {Z}}_N\) gauge field A.

We can rewrite the Lagrangian as

$$\begin{aligned} \frac{iN}{4\pi } (a+A)d(a+A) + \frac{iN}{2\pi } A d({\tilde{a}}-a). \end{aligned}$$
(A.5)

By performing field redefinitions, \(a' \equiv a+A\) and \({\tilde{a}}' \equiv {\tilde{a}} - a\), we see that this Lagrangian describes \(U(1)_{N} \times (\text {trivial SPT}) = U(1)_{N}\). Thus, the \(U(1)_{N}\) Chern-Simons theory is invariant under stacking the \((-1)^{Q(M,\Sigma )}\) SPT phase. This implies that the partition function of \(U(1)_{N}\) on M must vanish if there exists a two-cycle \(\Sigma \subset M\) such that \((-1)^{Q(M,\Sigma )} \ne 1\).

For example, take \(N=2\), \(M = {\mathbb {R}}P^3\), and \(\Sigma = {\mathbb {R}}P^2 \subset {\mathbb {R}}P^3\). Then, we have \((-1)^{Q(M,\Sigma )} = -1\), and indeed one can verify that the partition function of the \(U(1)_{2}\) Chern-Simons theory on \({\mathbb {R}}P^3\) vanishes.

More on the Triality Fusion Rules

In this appendix we give the detailed derivation of the triality fusion rules presented in Sects. 3.2 and 3.3. Below all the codimension-one defects are supported on a three-dimensional manifold M at \(x=0\).

B.1. Even N Here we derive the fusion rule in Sect. 3.2 for the triality defect \(\mathcal{D}_3\) and the condensation defects \({{{\mathcal {C}}}}_{N\ell \over 2}\) in any 3+1d QFT \({{\mathcal {Q}}}\) invariant under the ST gauging in the sense of (2.16) for the case of even N.

  • \(\overline{{\mathcal {D}}}_3 \times {\mathcal {D}}_3\): We have

    $$\begin{aligned} \begin{aligned} \overline{{\mathcal {D}}}_3 \times {\mathcal {D}}_3 :&{\mathcal {L}}[b_1] + \frac{2\pi i}{N}\left( -b_1 \cup b_2 - \frac{1}{2} q(b_2) + b_2 \cup B + \frac{1}{2} q(b_2) \right) \\ =&{\mathcal {L}}[b_1] + \frac{2\pi i}{N} \left( -b_1 \cup b_2 + b_2 \cup B \right) \,. \end{aligned} \end{aligned}$$
    (B.1)

    By flipping the sign of \(b_2\), we see that \(\overline{{\mathcal {D}}}_3 \times {\mathcal {D}}_3 = {\mathcal {C}}_0\).

  • \({\mathcal {D}}_3 \times \overline{{\mathcal {D}}}_3\): We have

    $$\begin{aligned} {\mathcal {D}}_3 \times \overline{{\mathcal {D}}}_3 :{\mathcal {L}}[b_1] + \frac{2\pi i}{N} \left( b_1 \cup b_2 + \frac{1}{2} q(b_1) - b_2 \cup B - \frac{1}{2} q(B) \right) , \end{aligned}$$
    (B.2)

    which is our definition of \({\mathcal {C}}_{\frac{N}{2}}\). Thus, \({\mathcal {D}}_3 \times \overline{{\mathcal {D}}}_3 = {\mathcal {C}}_{\frac{N}{2}}\).

  • \({\mathcal {D}}_3 \times {\mathcal {D}}_3\): We have

    $$\begin{aligned} {\mathcal {D}}_3 \times {\mathcal {D}}_3 :{\mathcal {L}}[b_1] + \frac{2\pi i}{N}\left( b_1 \cup b_2 + \frac{1}{2} q(b_1) +b_2 \cup B + \frac{1}{2} q(b_2) \right) . \end{aligned}$$
    (B.3)

    If we redefine the dynamical gauge fields as \(b \equiv b_1\) and \({\tilde{b}} \equiv b_1 + b_2\), the expression becomes

    $$\begin{aligned} {\mathcal {D}}_3 \times {\mathcal {D}}_3 :\left( \frac{2\pi i}{2N} q({\tilde{b}}+B) \right) + \left( {\mathcal {L}}[b] + \frac{2\pi i}{N} \left( -b \cup B - \frac{1}{2} q(B) \right) \right) \,. \end{aligned}$$
    (B.4)

    In the first term we see that the \({\tilde{b}}\) gauge field is decoupled from other dynamical fields including the matter fields. The path integral over \({\tilde{b}}\) defines a 3+1d invertible field theory in the region \(x>0\), with the Dirichlet boundary condition \({{\tilde{b}}}|=0\) imposed at \(x=0\). This gives the \(U(1)_{N}\) Chern-Simons theory living on M at \(x=0\) as shown in [1, 79]. Its coupling to B only affects transverse junctions. The remaining terms correspond to the definition of \(\overline{{\mathcal {D}}}_3\). Thus, we conclude \({\mathcal {D}}_3 \times {\mathcal {D}}_3 = U(1)_{N} \,\overline{{\mathcal {D}}}_3\).

  • \({\mathcal {D}}_3 \times {\mathcal {C}}_{\frac{N\ell }{2}}\) and \({\mathcal {C}}_{\frac{N\ell }{2}} \times {\mathcal {D}}_3\): We have

    $$\begin{aligned}{} & {} {\mathcal {D}}_3 \times {\mathcal {C}}_{\frac{N\ell }{2}} :{\mathcal {L}}[b_1] + \frac{2\pi i}{N}\nonumber \\ {}{} & {} \left( b_1 \cup b_2 + \frac{1}{2} q(b_1) + b_2 \cup b_3 + \frac{1}{2} \ell q(b_2) - b_3 \cup B - \frac{1}{2} \ell q(B) \right) , \end{aligned}$$
    (B.5)

    and

    $$\begin{aligned}{} & {} {\mathcal {C}}_{\frac{N\ell }{2}} \times {\mathcal {D}}_3 :{\mathcal {L}}[b_1] + \frac{2\pi i}{N}\nonumber \\ {}{} & {} \left( b_1 \cup b_2 + \frac{1}{2} \ell q(b_1) - b_2 \cup b_3 - \frac{1}{2}\ell q(b_3) + b_3 \cup B + \frac{1}{2}q(b_3) \right) . \end{aligned}$$
    (B.6)

    By setting \(\ell =0\) in Eq. (B.5) and redefining \(b_3 \rightarrow -b_3\), we obtain \({\mathcal {D}}_3 \times {\mathcal {C}}_0 = {\mathcal {C}}_{\frac{N}{2}} \times {\mathcal {D}}_3\). Furthermore, if we let \(b \equiv b_1\) and \(b'_3 \equiv b_3 + b_1\), we get

    $$\begin{aligned} {\mathcal {D}}_3 \times {\mathcal {C}}_0 :\left( \frac{2\pi i}{N}(b_2 - B) \cup b'_3 \right) + \left( {\mathcal {L}}[b] + \frac{2\pi i}{N} \left( b \cup B + \frac{1}{2}q(b) \right) \right) . \end{aligned}$$
    (B.7)

    The first term gives the 2+1d \(({\mathcal {Z}}_N)_0\) theory as we explained in Sect. 3.1, and the other terms give \({\mathcal {D}}_3\). Thus, \({\mathcal {D}}_3 \times {\mathcal {C}}_0 = {\mathcal {C}}_{\frac{N}{2}} \times {\mathcal {D}}_3 = ({\mathcal {Z}}_N)_0 \,{\mathcal {D}}_3\). Next, we have

    $$\begin{aligned} \begin{aligned}&{\mathcal {C}}_0 \times {\mathcal {D}}_3 :{\mathcal {L}}[b_1] + \frac{2\pi i}{N} \left( b_1 \cup b_2 - b_2 \cup b_3 + \frac{1}{2} q(b_3) + b_3 \cup B \right) \\&\quad = \frac{2\pi i}{N} \left( (-b'_2 + B) \cup b'_3 + \frac{1}{2} q(b'_3) \right) + \left( {\mathcal {L}}[b] + \frac{2\pi i}{N} \left( b \cup B + \frac{1}{2}q(b) \right) \right) \end{aligned} \end{aligned}$$
    (B.8)

    where \(b \equiv b_1\), \(b'_2 \equiv b_2 - b_1\), and \(b'_3 \equiv b_3 - b_1\). The terms inside the first pair of parentheses define a 2+1d \(({\mathcal {Z}}_N)_N\) gauge theory living on the defect [79]. To see this, we first set \(B=0\) for simplicity, as the coupling to B only affects the transverse junctions. Next, following a similar discussion around Fig. 2, we integrate out \(b'_2\) to force \(b'_3\) to effectively become a gauge field \(a \in H^1(M;{\mathbb {Z}}_N)\) living on M. The 4d twist term \(\frac{2\pi i}{2N} q(b'_3)\) reduces to the level N 3d Dijkgraaf-Witten twist for the gauge field a as shown in [49]. We therefore obtain a 2+1d \(({\mathcal {Z}}_N)_N\) gauge theory on M. Finally, remaining terms define the triality defect \({\mathcal {D}}_3\). We conclude \({\mathcal {C}}_0 \times {\mathcal {D}}_3 = ({\mathcal {Z}}_N)_N \, {\mathcal {D}}_3\). If instead \(\ell =1\) in Eq. (B.5), we redefine the variables as \(b_2 \rightarrow -b_3\) and \(b_3 \rightarrow b_1 + b_2\) to obtain

    $$\begin{aligned} {\mathcal {D}}_3 \times {\mathcal {C}}_{\frac{N}{2}} :{\mathcal {L}}[b_1] + \frac{2\pi i}{N} \left( b_1 \cup b_2 - b_2 \cup b_3 + \frac{1}{2} q(b_3) + b_2 \cup B - \frac{1}{2}q(B) \right) .\nonumber \\ \end{aligned}$$
    (B.9)

    Let \(b \equiv b_1\), \(b'_2 \equiv b_2 - b_1\), and \(b'_3 \equiv b_3 - b_1\), then we obtain

    $$\begin{aligned}{} & {} {\mathcal {D}}_3 \times {\mathcal {C}}_{\frac{N}{2}} :\frac{2\pi i}{N} \left( -(b'_2-B) \cup (b'_3 -B) + \frac{1}{2} q(b'_3 -B) \right) \nonumber \\{} & {} \quad + \left( {\mathcal {L}}[b] + \frac{2\pi i}{N} \left( b \cup B + \frac{1}{2}q(b) \right) \right) . \end{aligned}$$
    (B.10)

    We again see the decoupled 2+1d \(({\mathcal {Z}}_N)_N\) gauge theory on the defect and also \({\mathcal {D}}_3\). The coupling of this \(({\mathcal {Z}}_N)_N\) to the bulk symmetry background B is different from the previous case, but it only affects transverse junctions. We conclude that \({\mathcal {D}}_3 \times {\mathcal {C}}_{\frac{N}{2}} = ({\mathcal {Z}}_N)_N \,{\mathcal {D}}_3\).

  • \({\mathcal {C}}_{\frac{N\ell _1}{2}} \times {\mathcal {C}}_{\frac{N\ell _2}{2}}\): We have already derived \({\mathcal {C}}_0 \times {\mathcal {C}}_0 = ({\mathcal {Z}}_N)_0 \,{\mathcal {C}}_0\) in Sect. 3.1. Now, consider the fusion

    $$\begin{aligned} {\mathcal {C}}_0 \times {\mathcal {C}}_{\frac{N}{2}} :{\mathcal {L}}[b_1] +\frac{2\pi i}{N}\left( b_1 \cup b_2 - b_2 \cup b_3 + b_3 \cup b_4 +\frac{1}{2} q(b_3) - b_4 \cup B - \frac{1}{2} q(B) \right) .\nonumber \\ \end{aligned}$$
    (B.11)

    Let \(b'_4 \equiv b_4 - b_2\), then this becomes

    $$\begin{aligned} {\mathcal {C}}_0 \times {\mathcal {C}}_{\frac{N}{2}} :\frac{2\pi i}{N} \left( (b'_4 +B) \cup (b_3 -B) + \frac{1}{2} q(b_3 -B) \right) + \left( {\mathcal {L}}[b_1] + \frac{2\pi i}{N} \left( b_1 \cup b_2 - b_2 \cup B \right) \right) \nonumber \\ \end{aligned}$$
    (B.12)

    which gives \({\mathcal {C}}_0 \times {\mathcal {C}}_{\frac{N}{2}} = ({\mathcal {Z}}_N)_N \,{\mathcal {C}}_0\). Again, the coupling of the coefficient TQFT \(({\mathcal {Z}}_N)_N\) to the bulk symmetry background B only affects transverse junctions. We can perform an alternative change of variables \(b'_3 \equiv b_3 - b_1\) and \(b'_2 \equiv -b_2 + b_1 + b_4\) to rewrite (B.11) as

    $$\begin{aligned}{} & {} {\mathcal {C}}_0 \times {\mathcal {C}}_{\frac{N}{2}} :\frac{2\pi i}{N} \left( b'_2 \cup b'_3 + \frac{1}{2} q(b'_3) \right) \nonumber \\{} & {} \quad + \left( {\mathcal {L}}[b_1] + \frac{2\pi i}{N} \left( b_1 \cup b_4 + \frac{1}{2} q(b_1) - b_4 \cup B - \frac{1}{2} q(B) \right) \right) \end{aligned}$$
    (B.13)

    which gives \({\mathcal {C}}_0 \times {\mathcal {C}}_{\frac{N}{2}} = ({\mathcal {Z}}_N)_N \,{\mathcal {C}}_{\frac{N}{2}}\). One can also verify that the two condensation defects commutes, and we obtain \({\mathcal {C}}_0 \times {\mathcal {C}}_{\frac{N}{2}} = {\mathcal {C}}_{\frac{N}{2}} \times {\mathcal {C}}_0 =({\mathcal {Z}}_N)_N \,{\mathcal {C}}_0 = ({\mathcal {Z}}_N)_N \,{\mathcal {C}}_{\frac{N}{2}}\). Finally, consider

    $$\begin{aligned} {\mathcal {C}}_{\frac{N}{2}} \times {\mathcal {C}}_{\frac{N}{2}} :{\mathcal {L}}[b_1] + \frac{2\pi i}{N} \left( b_1 \cup b_2 + \frac{1}{2} q(b_1) -b_2 \cup b_3 +b_3 \cup b_4 - b_4 \cup B - \frac{1}{2} q(B) \right) .\nonumber \\ \end{aligned}$$
    (B.14)

    Let \(b'_4 \equiv b_4 - b_2\), then this reduces to

    $$\begin{aligned}{} & {} {\mathcal {C}}_{\frac{N}{2}} \times {\mathcal {C}}_{\frac{N}{2}} :\frac{2\pi i}{N} b'_4 \cup (b_3 - B)\nonumber \\ {}{} & {} + \left( {\mathcal {L}}[b_1] + \frac{2\pi i}{N} \left( b_1 \cup b_2 + \frac{1}{2} q(b_1) -b_2 \cup B -\frac{1}{2} q(B) \right) \right) , \end{aligned}$$
    (B.15)

    which gives \({\mathcal {C}}_{\frac{N}{2}} \times {\mathcal {C}}_{\frac{N}{2}} = ({\mathcal {Z}}_N)_0 \,{\mathcal {C}}_{\frac{N}{2}}\). To summarize, we have derived \({\mathcal {C}}_{\frac{N\ell _1}{2}} \times {\mathcal {C}}_{\frac{N\ell _2}{2}} = ({\mathcal {Z}}_N)_{N(\ell _1 + \ell _2)} {\mathcal {C}}_{\frac{N\ell _1}{2}} =({\mathcal {Z}}_N)_{N(\ell _1 + \ell _2)} {\mathcal {C}}_{\frac{N\ell _2}{2}}\) for general \(\ell _1\) and \(\ell _2\). The same fusion rules can also be derived from the definition of condensation defects given in Eq. (2.5) although we will not do so explicitly.

  • \({\mathcal {D}}_3 \times {\mathcal {D}}_3 \times {\mathcal {D}}_3\): We have

    $$\begin{aligned} \begin{aligned} {\mathcal {D}}_3 \times {\mathcal {D}}_3 \times {\mathcal {D}}_3 :&{\mathcal {L}}[b_1] + \frac{2\pi i}{N} \left( b_1 \cup b_2 + \frac{1}{2} q(b_1) + b_2 \cup b_3 + \frac{1}{2} q(b_2) + b_3 \cup B + \frac{1}{2} q(b_3) \right) \\&= \frac{2\pi i}{2N} q({\tilde{b}}) + \left( {\mathcal {L}}[b_1] + \frac{2\pi i}{N} \left( b_1 \cup b'_3 - b'_3 \cup B \right) \right) , \end{aligned}\nonumber \\ \end{aligned}$$
    (B.16)

    where we performed field redefinitions \({\tilde{b}} \equiv b_1 + b_2 + b_3\) and \(b'_3 \equiv - b_3\). The first term reduces to a 2+1d \(U(1)_{N}\) Chern-Simons theory on the defect [1, 79], and the remaining terms define the condensation defect \({\mathcal {C}}_0\). Thus, \({\mathcal {D}}_3 \times {\mathcal {D}}_3 \times {\mathcal {D}}_3 = U(1)_{N} \,{\mathcal {C}}_0\). Alternatively, one can also define , in which case we obtain

    (B.17)

    from which we can deduce \({\mathcal {D}}_3 \times {\mathcal {D}}_3 \times {\mathcal {D}}_3 = U(1)_{N} \,{\mathcal {C}}_{\frac{N}{2}}\). Combining the above, we conclude \({\mathcal {D}}_3 \times {\mathcal {D}}_3 \times {\mathcal {D}}_3 = U(1)_{N} \,{\mathcal {C}}_0 = U(1)_{N} \,{\mathcal {C}}_{\frac{N}{2}}\).

B.2. Odd N Here we derive the fusion rule in Sect. 3.3 for the triality defect \({{{\mathcal {D}}}}_3\) and the condensation defects \({{{\mathcal {C}}}}_{0}\) in any 3+1d QFT \({{\mathcal {Q}}}\) invariant under the ST gauging in the sense of (2.16) for the odd N case.

  • \(\overline{{\mathcal {D}}}_3 \times {\mathcal {D}}_3\) and \({\mathcal {D}}_3 \times \overline{{\mathcal {D}}}_3\): First, we have

    $$\begin{aligned} \begin{aligned} \overline{{\mathcal {D}}}_3 \times {\mathcal {D}}_3 :&{\mathcal {L}}[b_1] + \frac{2\pi i}{N}\left( -b_1 \cup b_2 - \frac{N+1}{2} b_2 \cup b_2 + b_2 \cup B + \frac{N+1}{2} b_2 \cup b_2 \right) \\ =&{\mathcal {L}}[b_1] + \frac{2\pi i}{N} \left( -b_1 \cup b_2 + b_2 \cup B \right) \,. \end{aligned} \end{aligned}$$
    (B.18)

    By flipping the sign of \(b_2\), we obtain \(\overline{{\mathcal {D}}}_3 \times {\mathcal {D}}_3 = {\mathcal {C}}_0\). Next,

    $$\begin{aligned} \begin{aligned} {\mathcal {D}}_3 \times \overline{{\mathcal {D}}}_3 :&{\mathcal {L}}[b_1] + \frac{2\pi i}{N}\left( b_1 \cup b_2 + \frac{N+1}{2} b_1 \cup b_1 - b_2 \cup B - \frac{N+1}{2} B \cup B \right) \\ =&{\mathcal {L}}[b_1] + \frac{2\pi i}{N} \left( b_1 \cup (b'_2 + \frac{N+1}{2} B) - (b'_2 + \frac{N+1}{2} B) \cup B \right) \,, \end{aligned} \end{aligned}$$
    (B.19)

    where we have defined \(b'_2 \equiv b_2 + \frac{N+1}{2} b_1\). The resulting defect obeys the same parallel fusion rule with \(\eta \) as \({\mathcal {C}}_0\) (see Sect. 4.3). Thus, if we ignore the transverse junctions, we can further shift \(b'_2\) by \(\frac{N+1}{2} B\). This gives \({\mathcal {D}}_3 \times \overline{{\mathcal {D}}}_3 = {\mathcal {C}}_0\).

  • \({\mathcal {D}}_3 \times {\mathcal {D}}_3\): We have

    $$\begin{aligned} \begin{aligned} {\mathcal {D}}_3 \times {\mathcal {D}}_3 :&{\mathcal {L}}[b_1] + \frac{2\pi i}{N}\left( b_1 \cup b_2 + \frac{N+1}{2} b_1 \cup b_1 + b_2 \cup B + \frac{N+1}{2} b_2 \cup b_2 \right) \\ =&\frac{2\pi i}{N} \frac{N+1}{2} ({\tilde{b}}+B)^2 + \left( {\mathcal {L}}[b] + \frac{2\pi i}{N} \left( -b \cup B - \frac{N+1}{2} B \cup B \right) \right) \,, \end{aligned} \end{aligned}$$
    (B.20)

    where we have defined \(b \equiv b_1\) and \({\tilde{b}} \equiv b_1 + b_2\). The first term is a 3+1d invertible field theory living in \(x>0\) with Dirichlet boundary condition \({{\tilde{b}}}|=0\) imposed at \(x=0\). This gives the 2+1d \(SU(N)_{-1}\) Chern-Simons theory living on the defect [79]. The remaining terms define \(\overline{{\mathcal {D}}}_3\). Thus, we have \({\mathcal {D}}_3 \times {\mathcal {D}}_3 = SU(N)_{-1} \,\overline{{\mathcal {D}}}_3\). From this and the earlier fusion rule, we also find \({\mathcal {D}}_3 \times {\mathcal {D}}_3 \times {\mathcal {D}}_3 = SU(N)_{-1} \,{\mathcal {C}}_0\).

  • \({\mathcal {D}}_3 \times {\mathcal {C}}_0\) and \({\mathcal {C}}_0 \times {\mathcal {D}}_3\): We have

    $$\begin{aligned} \begin{aligned} {\mathcal {D}}_3 \times {\mathcal {C}}_0 :&{\mathcal {L}}[b_1] + \frac{2\pi i}{N}\left( b_1 \cup b_2 + \frac{N+1}{2} b_1 \cup b_1 + b_2 \cup b_3 - b_3 \cup B \right) \\ =&\frac{2\pi i}{N} (b_2 - B) \cup b'_3 + \left( {\mathcal {L}}[b] + \frac{2\pi i}{N} \left( b \cup B + \frac{N+1}{2} b \cup b \right) \right) \,, \end{aligned} \end{aligned}$$
    (B.21)

    where \(b \equiv b_1\) and \(b'_3 \equiv b_3 + b_1\). The first term gives us the 2+1d \(({\mathcal {Z}}_N)_0\) gauge theory living on the defect, and the remaining terms define \({\mathcal {D}}_3\). Thus, \({\mathcal {D}}_3 \times {\mathcal {C}}_0 = ({\mathcal {Z}}_N)_0 \, {\mathcal {D}}_3\). Similarly, we have

    $$\begin{aligned} \begin{aligned}&{\mathcal {C}}_0 \times {\mathcal {D}}_3 :{\mathcal {L}}[b_1] + \frac{2\pi i}{N}\left( b_1 \cup b_2 - b_2 \cup b_3 + b_3 \cup B + \frac{N+1}{2} b_3 \cup b_3 \right) \\&\quad = \frac{2\pi i}{N} (b'_2 + B) \cup b'_3 + \left( {\mathcal {L}}[b] + \frac{2\pi i}{N} \left( b \cup B + \frac{N+1}{2} b \cup b \right) \right) \,, \end{aligned} \end{aligned}$$
    (B.22)

    where \(b \equiv b_1\), \(b'_2 \equiv \frac{N+1}{2}b_1 -b_2 +\frac{N+1}{2}b_3\), and \(b'_3 \equiv b_3 - b_1\). We see that \({\mathcal {C}}_0 \times {\mathcal {D}}_3 = ({\mathcal {Z}}_N)_0 \, {\mathcal {D}}_3\).

N-ality Defects From Mixed Anomalies

The Kramers-Wannier duality defect in 1+1d Ising model can be obtained from the invertible chiral symmetry defect in Majorana fermion by gauging the fermion parity symmetry [31, 101]. The chiral symmetry has a mixed anomaly with the fermion parity symmetry, and thus gauging the fermion parity symmetry “extends” the chiral symmetry to be a non-invertible symmetry generated by the Kramers-Wannier duality defect. Conversely, the Majorana fermion can be obtained from the Ising model by gauging a \({\mathbb {Z}}_2\) zero-form symmetry with a local counterterm [31, 102, 103].

We would like to understand whether the non-invertible N-ality defects discussed here can be obtained from invertible zero-form symmetry by gauging a one-form symmetry in a “parent theory”, generalizing the algorithm in [49]. In other words, we would like to understand whether the non-invertible symmetry defect becomes an invertible symmetry when we gauging a one-form symmetry with suitable local counterterm. As we will show in this appendix, this is in general not the case. Thus the non-invertible defect discussed here in general cannot be obtained from an invertible zero-form symmetry that has mixed anomaly with one-form symmetry by gauging the one-form symmetry. The condition that the non-invertible symmetry can be realized as an invertible symmetry upon gauging a discrete symmetry coincides with the condition that such non-invertible defect can be realized by invertible phases discussed in Sect. 5.

We define the codimension-one non-invertible defect in the same way as in Sect. 2 by gauging in half of the spacetime. On one side of the defect the theory has partition function Z[B] with the background two-form gauge field B. On the other side the partition function is \(\sum _b Z[b]e^{iS[b,B]}\), whereFootnote 31

$$\begin{aligned} \begin{aligned} S[b,B]= {\left\{ \begin{array}{ll} {2\pi \over N}\int b\cup B+\frac{p}{2}q(b) &{} \text {even }N\\ \frac{2\pi }{N}\int b\cup B+ 2^{-1}p \, b\cup b &{} \text {odd }N \end{array}\right. } \end{aligned} \end{aligned}$$
(C.1)

where \(2^{-1}=(N+1)/2\) is the inverse in \({\mathbb {Z}}_N\) for odd N.

Next, we gauge the one-form symmetry by promoting B to be dynamical, and add an additional local counterterm \(S'[B,B']\) with a new background two-form gauge field \(B'\),

$$\begin{aligned} S'[B,B']= \left\{ \begin{array}{ll} \frac{2\pi }{N}\int r B\cup B'+\frac{p'}{2}q(B)&{} \text {even }N\\ \frac{2\pi }{N}\int r B\cup B'+ p' B\cup B &{} \text {odd }N \end{array} \right. ~. \end{aligned}$$
(C.2)

The theories on the two sides of the defect are now

$$\begin{aligned}&\text {LHS}: \sum _B Z[B] e^{iS'[B,B']} \nonumber \\&\text {RHS}:\sum _{b,B}Z[b]e^{iS[b,B]+iS'[B,B']}~. \end{aligned}$$
(C.3)

If there is a choice of \(S'\) such that we can integrate out B on the right hand side to obtain \(\sum _b Z[b]e^{iS'[b,\ell B']}\) for some integer \(\ell \) that is coprime with N and up to a local counterterm of the background field \(B'\), then the defect becomes an invertible defect that generates zero-form symmetry in the theory with partition function \(\sum _B Z[B]e^{iS'[B,B']}\). More specifically, this invertible symmetry acts on the dual \({\mathbb {Z}}_N\) one-form symmetry by \(n\rightarrow n\ell \) for \(n\in {\mathbb {Z}}_N\). If we gauge the dual symmetry generated by \(\exp (i \oint B)\), such invertible zero-form symmetry becomes the non-invertible defect.

C.1. Duality Defect. Consider the Kramers-Wannier duality defect with \(p=0\). We will take \(\gcd (p',N)=1\).

C.1.1. Even N The partition function \(\sum _{b,B}Z[b]e^{iS[b,B]+iS'[B,B']}\) is

$$\begin{aligned}&\sum _{b,B}Z[b]\exp \left( {2\pi i\over N}\int \left( b\cup B+r B\cup B'+\frac{p'}{2}q(B)\right) \right) \nonumber \\&\quad =\sum _{{{\tilde{b}}}=B+p'^{-1}(b+rB'), b} Z[b] \exp \left( \frac{2\pi i p'}{2N}\int q(\tilde{b})+\frac{2\pi i}{N}\int \right. \nonumber \\&\qquad \left. \left( -\frac{p'^{-1}}{2}q(b)-p'^{-1} r b\cup B'-\frac{p'^{-1}r^2}{2}q(B')\right) \right) ~. \end{aligned}$$
(C.4)

Thus we need to solve

$$\begin{aligned} p'^2=-1\text { mod }2N\quad (\text {bosonic});\quad p'^2=-1\text { mod }N\quad (\text {fermionic})~, \end{aligned}$$
(C.5)

for bosonic and fermionic theories, respectively.

The solutions are discussed in [22], in a different context of invertible phases that possess Kramers-Wannier duality defect. For instance, if the theory is bosonic, then the first equation does not have a solution and the Kramers-Wannier duality defect cannot be obtained from an invertible symmetry by gauging one-form symmetries.

On the other hand, if the theory is fermionic, and for instance take \(N = 2\), then the equations have solution \(p' = 1\). Thus the Kramers-Wannier duality non-invertible defect can be obtained from an invertible zero-form symmetry in the theory \(\sum _B Z[B]e^{{\pi i\over 2} \int q(B)}\) by gauging the dual symmetry generated by \(\exp (i\oint B)\). The dual symmetry and the invertible zero-form symmetry has a mixed anomaly: in the presence of the background gauge field \(B'\) for the dual symmetry, the two sides of the defect differ by

$$\begin{aligned} -2\pi \frac{p'^{-1}r^2}{2N}\int q(B')~. \end{aligned}$$
(C.6)

The invertible symmetry acts on the one-form symmetry by multiplying the \({\mathbb {Z}}_N\) element with \(\ell =-(p')^{-1}\).

C.1.2. Odd N From a similar discussion, we need to solve

$$\begin{aligned} 4p'^2=-1\text { mod }N~. \end{aligned}$$
(C.7)

The solutions are discussed in [22], in a different context of invertible phases that possess Kramers-Wannier duality defect. When the equation is solvable, the Kramers-Wannier duality defect can be obtained by gauging one-form symmetry in a theory with invertible symmetry. The invertible symmetry has mixed anomaly with the dual one-form symmetry: in the presence of background gauge field \(B'\) for the dual one-form symmetry, the two sides of the defect differ by

$$\begin{aligned} -2\pi \frac{2^{-1}(2p')^{-1}r^2}{N}\int B'\cup B'~. \end{aligned}$$
(C.8)

The invertible symmetry acts on the one-form symmetry by multiplying the \({\mathbb {Z}}_N\) element with \(\ell =-(2p')^{-1}\).

C.2. Triality Defect.

C.2.1. Even N We have \(p=1\) and take \(\gcd (p',N)=1\). The partition function \(\sum _{b,B}Z[b]e^{iS[b,B]+iS'[B,B']}\) is

$$\begin{aligned}&\sum _{b,B}Z[b]\exp \left( {2\pi i\over N}\int \left( \frac{1}{2}q(b)+ b\cup B+r B\cup B'+\frac{p'}{2}q(B)\right) \right) \nonumber \\&\quad =\sum _{{{\tilde{b}}}=B+p'^{-1}(b+rB'), b} Z[b]\exp \left( \frac{2\pi i p'}{2N}\int q({{\tilde{b}}}) +\frac{2\pi i}{N}\right. \nonumber \\&\qquad \left. \int \left( \frac{1-p'^{-1}}{2}q(b)-p'^{-1} r b\cup B'-\frac{p'^{-1}r^2}{2}q(B')\right) \right) . \end{aligned}$$
(C.9)

Thus we need to solve

$$\begin{aligned} p'(p'-1)+1=0\text { mod }2N\quad (\text {bosonic});\quad p'(p'-1)+1=0\text { mod }N\quad (\text {fermionic}).\nonumber \\ \end{aligned}$$
(C.10)

Since \(p'(p'-1)\) is even, and the above equation has definite even/odd parity, there is no solution. Thus the triality defect cannot be obtained from an invertible symmetry by gauging a one-form symmetry.

C.2.2. Odd N Here \(p=N+1\) and we take \(\gcd (p',N)=1\). The partition function \(\sum _{b,B}Z[b]e^{iS[b,B]+iS'[B,B']}\) is

$$\begin{aligned}&\sum _{b,B}Z[b]\exp \,\left( {2\pi i\over N}\int \left( \frac{N+1}{2} (b\cup b)+ b\cup B+r B\cup B'+p'(B\cup B)\right) \right) \nonumber \\&\quad =\sum _{{{\tilde{b}}}=B+(2p')^{-1}(b+rB'), b} Z[b]\exp \left( \frac{2\pi ip'}{N}\int ({{\tilde{b}}}\cup {{\tilde{b}}}) \right) \nonumber \\&\qquad \times \exp \left( \frac{2\pi i}{N}\int \left( \left( \frac{N+1}{2}-2^{-1}(2p')^{-1}\right) \right. \right. \nonumber \\&\qquad \left. \left. (b\cup b)-(2p')^{-1} r b\cup B'-2^{-1}(2p')^{-1}r^2(B'\cup B')\right) \right) ~. \end{aligned}$$
(C.11)

Thus we need to solve

$$\begin{aligned} (2p')^2-2p'+1=0\text { mod }N~. \end{aligned}$$
(C.12)

There exits solution if and only if \(N\in {{{\mathcal {X}}}}\) as defined in (5.12).

When \(N\in {{{\mathcal {X}}}}\) and thus a solution exists, the coupling to \(B'\) on the two sides of the invertible wall is r and \(-(2p')^{-1}r\). The invertible symmetry has mixed anomaly with the dual symmetry: in the presence of background \(B'\) for the dual symmetry generated by \(\exp (i \oint B)\), the two sides of the defect differ by a local counterterm (take \(r =1\))

$$\begin{aligned} -\frac{\pi (N+1)(2p')^{-1}}{N}\int (B'\cup B')~. \end{aligned}$$
(C.13)

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Choi, Y., Córdova, C., Hsin, PS. et al. Non-invertible Condensation, Duality, and Triality Defects in 3+1 Dimensions. Commun. Math. Phys. 402, 489–542 (2023). https://doi.org/10.1007/s00220-023-04727-4

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