SciPost Submission Page
Solitonic symmetry as non-invertible symmetry: cohomology theories with TQFT coefficients
by Shi Chen, Yuya Tanizaki
Submission summary
Authors (as registered SciPost users): | Shi Chen · Yuya Tanizaki |
Submission information | |
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Preprint Link: | scipost_202503_00063v1 (pdf) |
Date submitted: | 2025-03-31 14:45 |
Submitted by: | Chen, Shi |
Submitted to: | SciPost Physics |
Ontological classification | |
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Academic field: | Physics |
Specialties: |
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Approach: | Theoretical |
Abstract
Originating from the topology of the path-integral target space Y, solitonic symmetry describes the conservation law of topological solitons and the selection rule of defect operators. As Ref.~\cite{Chen:2022cyw} exemplifies, the conventional treatment of solitonic symmetry as an invertible symmetry based on homotopy groups is inappropriate. In this paper, we develop a systematic framework to treat solitonic symmetries as non-invertible generalized symmetries. We propose that the non-invertible solitonic symmetries are generated by the partition functions of auxiliary topological quantum field theories (TQFTs) coupled with the target space Y. We then understand solitonic symmetries as non-invertible cohomology theories on Y with TQFT coefficients. This perspective enables us to identify the invertible solitonic subsymmetries and also clarifies the topological origin of the non-invertibility in solitonic symmetry. We finally discuss how solitonic symmetry relies on and goes beyond the conventional wisdom of homotopy groups. This paper is aimed at a tentative general framework for solitonic symmetry, serving as a starting point for future developments.
Author indications on fulfilling journal expectations
- Provide a novel and synergetic link between different research areas.
- Open a new pathway in an existing or a new research direction, with clear potential for multi-pronged follow-up work
- Detail a groundbreaking theoretical/experimental/computational discovery
- Present a breakthrough on a previously-identified and long-standing research stumbling block
Author comments upon resubmission
Best regards,
Shi Chen, Yuya Tanizaki
List of changes
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Reply to Referee 1
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Thanks very much for reviewing our paper with saying "this is a timely and important paper." We made corrections to clarify the point you raised.
(1) and (4) The typos were already corrected in the arXiv version (namely v2) in our first submission.
(2) Eq. (2.8) is correct in the current form. As an example, let us consider the U(1) gauge theory. The magnetic monopole chagre ∫M12πda is always defined on a 2-manifold M in any spacetime dimension. Because of this independence from the ambient spacetime, we can develop the theory of solitonic symmetries just focusing on the target space Y.
(3) We removed E-orientable following your suggestion.
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Reply to Referee 2
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Thanks very much for reviewing our paper with saying "I recommend to publish it in SciPost." We made corrections to clarify the points you raised.
# On Major points:
1. Thanks for raising this point.
We now think that the structure type on the operator manifold M may be chosen independently from the tangential structure of the spacetime manifolds. We thus modified a lot of contents in the paper to address the problems raised by this issue. Most of them are minor wording changes, and the major modifications are the following.
i) We added one sentence to the last of the paragraph below Eq.(3.2).
ii) We removed the leading paragraph of Sec. 3.3 and instead added a new paragraph.
2. We agree that chiral Chern-Simons theories are not included in our general formal framework, and our discussions here were actually incomplete.
Hence we are pleased to follow the referee's suggestion.
i) We first added a new paragraph to the end of Sec. 4.2.2 to explain that our general framework precludes chiral TQFTs.
ii) We then modified the construction of topological functional of our primary example of 4d CP1 sigma model in Sec. 5.2.2 using non-chiral Chern-Simons theories. Explicitly, we replaced the last two paragraphs of Sec. 5.2.2 with three new paragraphs.
3.
- Issues about Sec. 4.2.2:
Freed and Hopkins discussed about the topology on C× in their Sec. 5.3. In the paragraph above Remark 5.16, they said that ΣnIC× corresponds to discrete topology on C×. In the paragraph above Eq. 5.17, they said that Σn+1IZ(1) correpsonds to continuous topology on C×. Intuitively, continuous topology allows us to deform one theory to another, whereas discrete topology isolates each individual theory. Therefore, the use of continuous topology classifies the isomorphism classes, while the use of discrete topology classifies the deformation classes. We added Footnote 11 to clarify this point and cited Sec. 5.3 of Freed-Hopkins for readers who are interested in.
- Issues about Sec 4.3.2:
Vect× and sVect× are the 0-truncation and the 1-truncation of IC×, respectively. The former fact is trivial, and we explained the latter fact around Eq. 4.28 in the present version. Meanwhile, Vect× and sVect× are also the 0-truncation and the 1-truncation of IC×MSpin, respectively. This is because the spin Thom spectrum MSpin is 1-connected. As for our SU, it is an alternative of sVect× when the target space is finite, and it is not the 1-truncation of IC×MSpin on its own. We rewrote many sentences in Sec. 4.3.2, to refine the descriptions of the relevant spectra; this passingly includes a reply to Minor Point 10.
# On Minor points:
1. We added some related references and changed the sentence accordingly.
2. Here, we are not discussing the continuous deformation of the submanifolds. Rather, what we are discussing the continuous deformation of the field configurations on a fixed submanifold. We note that this is roughly equivalent to consider the continuous deformation of the base manifold while keeping its topology fixed. In this sense, we can answer your question that our continuous deformation excludes the case when the sphere is retracted to a point. As we are just mentioning the sufficient condition (not the necessary condition) for the values of topological functionals being nontrivial, we think "as long as" is the right word.
3. We added references.
4. We removed the leading paragraphs of Sec. 3.3 as we made a mistake due to our misunderstanding in the first version, as explained in the Major point 1.
5. We added a footnote to make the remark on the difference from the conventional definition.
6. Thanks for pointing it out. We added the following sentence: "For the claim of equivalence among several models, see Ref.~\cite{Barwick:2021}."
7. We moved the part of previous Footnote 17 (present Footnote 20) to the place you suggested in Sec. 4.2.1 to explain the notion of universe. We, however, left previous Footnote 17 (present Footnote 20) partly, because we have not introduced Repn(Y) in Sec. 4.2.1 yet.
8. We added a footnote for clarifications.
9. We added comments with the reference to Lurie's paper for clarifications.
10. We updated the discussion before Proposition 4.11 and clarified how we define SC (see also our answer for Major Point 3).
11. We made the correction as suggested.
12. As the referee pointed out, B3Z→X→B2Z→B4Z is a fragment of a homotopy fiber sequence, and each class ∈[B2Z,B4Z] prescribes a distinct space X (up to homotopy equivalence). Nevertheless, computing which class yields X≃π≤3CP1 requires additional work. We expanded the text and added a footnote to explain why the generator of [B2Z,B4Z]≃\Z yields X≃π≤3CP1.
13. We added several references on the condensation operators.
14. We agree with your point, but we also believe that the solitonic symmetry should be anomaly free even for continuous cases. We added a footnote there to justify our conjecture 6.1.
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Additional modification
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In addition to both referees' suggestions, we found other inappropreiate descriptions in the manuscript, and we also modfied them accordingly.
(1) We modified our speculation in present Footnote 17 (previous Footnote 14). The Brown-Comenetz dual of MSO or MSpin gives gravitational theta angles in terms of characteristic classes of tangent bundles (including Pontryagin, Stiefel-Whitney, and KO-theoretic classes). Our TQFTs are a priori defined on framed manifolds, and all the charactertic classes of a framed manifold have to be trivial. Hence our TQFTs do not cover those gravitational theta angles.
(2) In Sec. 3.1 "Example: spin structure", our previous decription of the f-action on ℓ was incorrect, and we now corrected it (see Eq. 3.9). We also added references about the mapping class group of S2×S1 there.