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Entanglement asymmetry in periodically driven quantum systems
by Tista Banerjee, Suchetan Das and Krishnendu Sengupta
This is not the latest submitted version.
Submission summary
| Authors (as registered SciPost users): | Krishnendu Sengupta |
| Submission information | |
|---|---|
| Preprint Link: | scipost_202412_00038v2 (pdf) |
| Date submitted: | April 7, 2025, 10:54 a.m. |
| Submitted by: | Krishnendu Sengupta |
| Submitted to: | SciPost Physics |
| Ontological classification | |
|---|---|
| Academic field: | Physics |
| Specialties: |
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| Approach: | Theoretical |
Abstract
We study the dynamics of entanglement asymmetry in periodically driven quantum systems. Using a periodically driven XY chain as a model for a driven integrable quantum system, we provide semi-analytic results for the behavior of the dynamics of the entanglement asymmetry, $\Delta S$, as a function of the drive frequency. Our analysis identifies special drive frequencies at which the driven XY chain exhibits dynamic symmetry restoration and displays quantum Mpemba effect over a long timescale; we identify an emergent approximate symmetry in its Floquet Hamiltonian which plays a crucial role for realization of both these phenomena. We follow these results by numerical computation of $\Delta S$ for the non-integrable driven Rydberg atom chain and obtain similar emergent-symmetry-induced symmetry restoration and quantum Mpemba effect in the prethermal regime for such a system. Finally, we provide an exact analytic computation of the entanglement asymmetry for a periodically driven conformal field theory (CFT) on a strip. Such a driven CFT, depending on the drive amplitude and frequency, exhibits two distinct phases, heating and non-heating, that are separated by a critical line. Our results show that for $m$ cycles of a periodic drive with time period $T$, $\Delta S \sim \ln mT$ [$\ln (\ln mT)$] in the heating phase [on the critical line] for a generic CFT; in contrast, in the non-heating phase, $\Delta S$ displays small amplitude oscillations around it's initial value as a function of $mT$. We provide a phase diagram for the behavior of $\Delta S$ for such driven CFTs as a function of the drive frequency and amplitude
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Author comments upon resubmission
We resubmit as response to the comments by both the referees on our original submission.
All the changes from the earlier version in the main body of the manuscript is colored blue.
Your sincerely
Krishnendu Sengupta
on behalf of
Tista Banerjee, Suchetan Das, and Krishnendu Sengupta
List of changes
1) We have added a discussion in Sec 4 as response to second comment of Ref 1.
2) We have added a paragraph in the Introduction in response to first comment of Ref 1.
3) We have corrected a typo in Eq 38 of the draft in response to comment 4 of Ref 2
4) We have added Ref 27 in response to comment 5 of Ref 2.
5) We have added a clarification regarding computation of the CFT dynamics in Sec 4.
Current status:
Reports on this Submission
Report #2 by Anonymous (Referee 2) on 2025-5-18 (Invited Report)
- Cite as: Anonymous, Report on arXiv:scipost_202412_00038v2, delivered 2025-05-18, doi: 10.21468/SciPost.Report.11208
Report
In particular, regarding their reply to my question 2, the authors claim that their formula for the dimension of the composite twist operator,
\begin{equation}
\sum_{j=1}^n\frac{\Delta(\alpha_j)}{n^2}
\end{equation}
reduces to the expression by Goldstein and Sela,
\begin{equation}
\frac{\Delta(\alpha)}{n^2}
\end{equation}
when all $\alpha_j$ are equal, i.e. when $\alpha_j=\alpha/n$. However, assuming $\Delta(\alpha)=\alpha^2$ (as the authors do in the paper), we find from their expression
\begin{equation}
\alpha^2/n^3,
\end{equation}
while Goldstein and Sela's formula gives
\begin{equation}
\alpha^2/n^2.
\end{equation}
My proposed formula,
\begin{equation}
\Delta\left(\sum_{j=1}^n\alpha_j\right)/n^2,
\end{equation}
also gives $\alpha^2/n^2$. It predicts when $\sum_j\alpha_j=0$ that $\Delta(\sum_j\alpha_j)=0$, and the asymmetry is zero. This is consistent with the defect being topological. The core issue in Section 4.1 seems to be that the authors assume that the defects are topological in the bulk, but their calculation does not properly take into account that the symmetry is broken in the boundary. As a result, once the correct dimension of the composite twist fields is used, the asymmetry vanishes. To obtain a non-zero asymmetry in this framework, the breaking of the symmetry at the boundary must be explicitly incorporated.
I would also like to remark on a statement after Eq. (34), where the authors write: “In contrast, we demand $[\rho_A,Q_A]\neq 0$; this results in unequal weight of fluxes at every sheet as described in Eqs. 33 and 34.” This statement is, in my view, not correct: In the definition of the asymmetry (Eq. 33), different fluxes $\alpha_j$ are introduced in each replica, regardless of whether $Q_A$ commutes with $\rho_A$. If $\rho_A$ and $e^{i\alpha_jQ_A}$ commute, then the different fluxes cancel and the asymmetry is zero.
While I do not wish to insist further on this calculation, since it is not central to the main results of the manuscript, I would suggest that the authors reconsider this section carefully before the paper is accepted.
Recommendation
Ask for minor revision
Report
Recommendation
Publish (easily meets expectations and criteria for this Journal; among top 50%)
We thank the referee for their remark and for supporting publication.

Author: Krishnendu Sengupta on 2025-06-13 [id 5569]
(in reply to Report 2 on 2025-05-18)We thank the referee for a careful reading of our manuscript and pointing out some important issues. We have now rewritten parts of the draft to make our calculation method clear and added an appendix. We think that these additions will address referee's concerns. Below, We respond to their comments in details. \
The trace of $n^{\rm th}$ power of the symmetry projected reduced density matrix has the following expression: \begin{align} {\rm Tr}(\rho_{A,Q}^{n}) = \int^\pi_{-\pi} ..... \int^\pi_{-\pi} \frac{d\alpha_1 .... d\alpha_n}{(2\pi)^n} {\rm Tr} \Big[\prod_{j=1}^n \rho_A \exp[i\alpha'_j Q_A] \Big] \end{align} where $\alpha'_j$ =$ \alpha_j-\alpha_{j+1} $ and $\alpha_{n+1}=\alpha_{1}$ so that $\sum_{j=1}^{n}\alpha'_{j} = 0$. In our previous response, we have mistakenly stated that this would reduce to the Goldstein and Sela's answer. We apologize for the misleading statement. We do agree to the referee that our set-up is different to that used by Goldstein and Sela for computing symmetry resolved entanglement entropy. Below, we provide the reason for this. We have now corrected several statements in the manuscript in Secs. 1, 4.1 and 5 and added an appendix to show the details of our calculation.
In our work, we have implicitly assumed that the defect line is not topological. The main justification of this comes from the fact $[\rho,Q]\neq 0$ in our case ( and hence $[\rho_A, Q_A] \ne 0$) since we are working on a strip which hosts boundary state: \begin{align} (T(z)-\bar{T}(\bar{z}))|B\rangle=0 \; \text{at} \; z=\bar{z}. \end{align} A solution of the above equation is a conformal boundary state $|B\rangle$, which can be written in terms of linear combination of Ishibashi states. By definition, an Ishibashi state is constructed out of a primary and taking sum of all level Virasoro descendants acting on that primary with a specific holomorphic structure(for reference, see equation (2.8) of arXiv:1412.6226). This kind of state is expected to break the symmetry of the charge sector since $H|B\rangle \neq 0$. We have computed the Renyi asymmetry in this state. Note that computing $n$-point bulk correlation function in a boundary state is equivalent to $2n$-point holomorphic correlation function in the full complex plane without defect. This `method of image trick' is a consequence of the Ward identity in BCFT, where one need to impose $T(z)=\bar{T}(\bar{z})$ at the boundary(a review of this is given in appendix (D) of arXiv:1907.08763). This further implies in the presence of boundary defect, each Riemann sheet (dressed with $\exp[i \alpha'_j Q_A]$) will contribute to the stress tensor as shown in Eq. (36) of our work and we got (2) as the conformal dimension of composite twist operator.
Regarding how to ensure that the asymmetry vanishes for $[\rho_{A},Q_{A}]=0$, we note the following. As the Referee correctly pointed out, for a topological defect operator, it is possible to fuse the defect lines into the same Riemann sheet (For reference, see JHEP05 (2024) 059). In such a case, the composite twist dimension should reduce to the same as referee has suggested (this can also be seen from expression of $X_n$) and yield \begin{align} d_{n}=\frac{c}{24}(n-\frac{1}{n}) + \Delta(\sum_{j=1}^{n}\alpha'_{j})/n^2 ---- (2) \end{align} Since $\sum_{j=1}^n \alpha'_j=0$, $\Delta=0$ in this case; hence the asymmetry will vanish. This will happen if the initial (ground) state respects the symmetry: $[\rho,Q]=0$. In this case, by definition, $[\rho_{A},Q_{A}]=0$ and we can fuse the defect line into one sheet. Using (3), we can easily see the entanglement asymmetry will vanish in this case. We thank the referee for pointing this out.
We note that from Eqs. (36) and (37) of our work, we end up with \begin{align} d_{n}=\frac{c}{24}(n-\frac{1}{n}) + \sum_{j=1}^{n-1}\Delta(\alpha'_{j})/n^2 \end{align} where $\Delta$ is a function of $\alpha'_j$ i.e. $\Delta(\alpha'_{j})$= $K (\alpha'_{j})^{2}$= $K (\alpha_{j}-\alpha_{j+1})^{2}$ for a class of CFTS. This form is dictated by the fact that for us $[\rho_A, Q_A]\ne 0$. This is central to obtaining the final answer as we claimed in equation (39) and (40) of our work.
We hope that these changes will address referee's concern regarding the computations in Sec. 4.1.