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Self-congruent point in critical matrix product states: An effective field theory for finite-entanglement scaling

by Jan T. Schneider, Atsushi Ueda, Yifan Liu, Andreas M. Läuchli, Masaki Oshikawa, Luca Tagliacozzo

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Submission summary

Authors (as registered SciPost users): Yifan Liu · Andreas Läuchli · Jan Thorben Schneider · Atsushi Ueda
Submission information
Preprint Link: https://arxiv.org/abs/2411.03954v2  (pdf)
Date submitted: Feb. 26, 2025, 8:39 a.m.
Submitted by: Schneider, Jan Thorben
Submitted to: SciPost Physics
Ontological classification
Academic field: Physics
Specialties:
  • Condensed Matter Physics - Theory
  • Condensed Matter Physics - Computational
  • Statistical and Soft Matter Physics
Approaches: Theoretical, Computational

Abstract

We set up an effective field theory formulation for the renormalization flow of matrix product states (MPS) with finite bond dimension, focusing on systems exhibiting finite-entanglement scaling close to a conformally invariant critical fixed point. We show that the finite MPS bond dimension χ is equivalent to introducing a perturbation by a relevant operator to the fixed-point Hamiltonian. The fingerprint of this mechanism is encoded in the χ-independent universal transfer matrix's gap ratios, which are distinct from those predicted by the unperturbed Conformal Field Theory. This phenomenon defines a renormalization group self-congruent point, where the relevant coupling constant ceases to flow due to a balance of two effects; When increasing χ, the infrared scale, set by the correlation length ξ(χ), increases, while the strength of the perturbation at the lattice scale decreases. The presence of a self-congruent point does not alter the validity of the finite-entanglement scaling hypothesis, since the self-congruent point is located at a finite distance from the critical fixed point, well inside the scaling regime of the CFT. We corroborate this framework with numerical evidences from the exact solution of the Ising model and density matrix renormalization group (DMRG) simulations of an effective lattice model.

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Author comments upon resubmission

We thank the referees for their time and effort in carefully reading our manuscript, resulting in constructive criticism. In this second version, we have implemented their remarks, which improved our manuscript.

List of changes

- Page 3, removed the sentence “This has been the subject of several studies.”

- Beginning of Section 2: We have made the distinction of thermodynamic limit and
infinite degrees of freedom

- Page 6, added sentence on further details on the scaling hypothesis and reference.

- Page 5, thus affecting thus affecting the ratio of the gap ratios'' to thus affecting the ratio of the gaps''

- Beginning of Section 2.1: Added a paragraph on introduction on the transfer matrix and motivation of studying MPS TMs.

- Fig 2 description: symmetry-broken to non-conserving

- Figure 3(b): x-axis label changed from L/ξ0χκ to L/ξ(χ), label for dashed green line changed from L15/4 to (L/ξ)15/4

- Below Eq.~(13) and describing Fig.~3(a) correction of quantity explained from this relation is shown'' (i.e. δE0) to E0ϵL'' and in the sentence referencing Fig.~3(a), a clarification and definition of ϵ0

- Page 12. This result aligns with our numerical observations shown in Fig.~3(b) [added:] when replacing the renormalization scale L with L/ξ(χ), being the relevant length scale in the crossover regime from finite-size to finite-entanglement scaling.

- Below Eq.~(34) add spontaneous:
However, in the spontaneous symmetry-breaking phase (SSB), the quasi-particle excitations are domain walls. Add also sentence and reference to algebraic Bethe ansatz with its analytical solutions.

- On page 13, changed transitionally'' into translationally''.

- Typo in the caption of Fig 6, 11/ξ instead of 11/L.

- Page 21, added clarification below Eq. (40) on the confinement of the theory

- Page 17, Eqs. (34) and (35), added expression in terms of the perturbation δ.

- Page 17, define acronym SSB as spontaneous symmetry-breaking phase''

- Page 18, adding further clarification for why the SSB phase is selected by iDMRG.

- On page 22, added subclause specifying that the relevant operator is rendered marginal in combination with its scale dependent coupling (twice)

- Right before A.11, corrected \ketψ to be \ketψ0, and e to e0.

- Below (B.1) updated the self-duality mapping to the correct one from the original reference.

- Below Eq.~(34): moved the sentence from before Eq.~(35) about the two elementary excitations needed to create any correlation

- Several minor orthographic corrections

Current status:
Has been resubmitted

Reports on this Submission

Report #1 by Anonymous (Referee 2) on 2025-3-25 (Invited Report)

  • Cite as: Anonymous, Report on arXiv:2411.03954v2, delivered 2025-03-25, doi: 10.21468/SciPost.Report.10906

Report

I thank the authors for their careful, point-by-point reply to my report. I understand the work more clearly now and I support its publication. I attach a series of comments from my second reading of the manuscript as well as of the author's reply.

- The explanation of why we are interested in the spectrum of the transfer matrix makes sense. I would make a bit more emphasis on the fact that the correspondence between the spectra of the TM and the effective Hamiltonian is a numerical observation (unless there is a proof of it in some reference). I would suggest also adding is a comment about the fact whether the transfer matrix is Hermitian, since it feels like it need not be, yet its spectrum is real anyway.

- In Fig. 3(a), the reader is not given an explanation for the appearance of νc in the cyan dotted line, the expansion of the Eexact(L) only gives π/6L.

- At the end of the first paragraph of page 14, it reads "Their distance from the unstable CFT fixed point increases logarithmically as we increase the system size." What distance measure are we talking about?

- Above Eq. 25, I would use a different letter to count the number of fermionic modes, since m already means something else.

- If I have now understood the Eqs. (33)-(35) argument correctly, the statement is that we can compute the correlation length exactly at both sides of the phase transition, thanks to (33) (which, I'd say, is a nontrivial result, as opposed to the author's reply saying that correlation length and single particle gap are inversely proportional "by definition"), and we pick the value of m so that ξ=L/2. Is this the case?

- On the sixth line of page 19, I would advise against using footnotes that can be mistook for exponents. Also, is there a reference for the information in the footnote (the bias of the variational energy) or is it an observation of the authors?

- Towards the end of 5.2.2. there is a reference to Fig. 8(c) which does not exist.

- I find the explanation for the influence of the choice of symmetric vs. nonsymmetric tensors on the spectrum of the TM is a bit rushed and sandwiched in the discussion of a different spectrum (the entanglement Hamiltonian spectrum, last paragraphs before Section 6), making it easy to miss. It would be nice to give it some more entity and discuss whether the relevant boundary conditions can be implemented in the toy model of the paper.

- I appreciate the explanation about Appendix A, although I believe it does not match what is done in the Appendix. Having checked the references, it seems like Appendix A uses the argument of Pollmann et al., while the reply to my report features the argument of Pirvu et al. I think I understand now that the argument in the Appendix is to find the state, among the family of states with all possible correlation lengths, that minimizes the energy upon truncation to a given bond dimension w.r.t. the gapless Hamiltonian, and my confusion is why do we assume that the Schmidt values follow the distribution of a critical state also for states with finite correlation length, i.e., why (A.7) should follow (A.1), and why do we seem to use the gap of the perturbed Hamiltonian in (A.11) in order to determine the energy with respect to the gapless Hamiltonian. In any case, since this is based on previous published works, I guess it does not really affect this work that much.

- Regarding my comment about Appendix B, I would say the transformation is indeed the original Kramers-Wannier. I guess the confusion was just that I was thinking self-duality as the Hamiltonian mapping back to itself under the duality (which only holds when g=1), while the authors are referring to the Hamiltonian mapping back to one in the same family (i.e. self-duality of the entire class).

Recommendation

Publish (easily meets expectations and criteria for this Journal; among top 50%)

  • validity: high
  • significance: high
  • originality: high
  • clarity: good
  • formatting: perfect
  • grammar: excellent

Author:  Jan Thorben Schneider  on 2025-04-07  [id 5349]

(in reply to Report 1 on 2025-03-25)
Category:
answer to question
correction

We thank the referee for their positive evaluation of our previous feedback and for the careful critique of our revised second version. Below, we intend to respond satisfactorily to all points raised by the referee.

The explanation of why we are interested in the spectrum of the transfer matrix makes sense. I would make a bit more emphasis on the fact that the correspondence between the spectra of the TM and the effective Hamiltonian is a numerical observation (unless there is a proof of it in some reference). I would suggest also adding is a comment about the fact whether the transfer matrix is Hermitian, since it feels like it need not be, yet its spectrum is real anyway.

A: We have added the clarification of the numerical observation of the mapping of the TM spectrum to the effective Hamiltonian spectrum. On the second point, indeed the TM spectrum does not need to be real as the transfer matrix is not Hermitian in general. In the Ising model, everything is real-valued because the Ising model has not just a Hermitian Hamiltonian but indeed a symmetric real Hamiltonian. The ground state of the Ising model is thus real-valued, and therefore so is the transfer matrix. We added a note stating that this is generally not true.

In Fig. 3(a), the reader is not given an explanation for the appearance of νc in the cyan dotted line, the expansion of the Eexact(L) only gives π/6L

A: On page 11, in the main text discussing Fig. 3(a), we cite Refs. [53, 54], the relevant references which give the definition of the Casimir energy in the context of a CFT given the features of the model, i.e., speed of sound v=2, and conformal charge c=1/2. Note that the referee mistakenly read the cursive Latin letter v as the cursive Greek letter ν, possibly mistaking it for the critical exponent ν=1. We have added a footnote to warn the reader. We have made the formula explicit in the main text in the new version, explaining the contributing factors in the Ising model. Essentially, vc=1 as v=2 and c=1/2 in the Ising model, which hopefully should resolve the confusion.

At the end of the first paragraph of page 14, it reads "Their distance from the unstable CFT fixed point increases logarithmically as we increase the system size." What distance measure are we talking about?

The logarithmic distance originates from the RG flow equations which are always Ordinary Differential Equations (ODEs) in the logarithm of the system size, as in Eq. (15). Thus, the "flow" in the RG sense happens in a space of couplings with a notion of distance (or time if you want) given by the logarithm of the ratios of two system sizes, log(L2/L1), which are given by the initial and final point of the flow, L1 and L2, respectively. The maximum distance RG can flow in a physical system with system size L is log(L/1), that is, from the microscopic definition of a single site (or unit cell), L1=1, up to the notion of the complete system, L2=L. The distance of the initial coupling flowing due to RG to its final point hence grows logarithmically with the size of the system and approaches the fixed point in the thermodynamic limit.

Above Eq. 25, I would use a different letter to count the number of fermionic modes, since m already means something else.

A: Thank you for noticing the double notation. We have adapted the label for the number of fermion modes.

If I have now understood the Eqs. (33)-(35) argument correctly, the statement is that we can compute the correlation length exactly at both sides of the phase transition, thanks to (33) (which, I'd say, is a nontrivial result, as opposed to the author's reply saying that correlation length and single particle gap are inversely proportional "by definition"), and we pick the value of m so that ξ=L/2. Is this the case?

A: We have restructured the arguments slightly and taken out the previous Eq. (33), which only served to give the speed of sound (or speed of light) v the entrance as a necessary proportionality constant into the well-known inverse proportionality relation of the correlation length to the gap, for dimensional reasons. In addition to the dimensional argument, i.e., ξv|Δ1|1, there is a dimensionless factor of 2 arising from the domain-wall nature of the quasi-particle excitations. Furthermore, we have argued above Eq. (23), the definition of the lattice model, that we expect a factor of 2 between the correlation length and the system size, since the correlation of the effective Hamiltonian is mediated through the finite bond dimension tensors on both sides. As the induced spatial dimension of the finite bond dimension is given by the correlation length, this gives rise to a notion of the total system size given by twice the correlation length, L=2ξ. We furthermore numerically verify our thusly constructed model, giving rise to the correct behavior. This consequently fixes |m|=1 according to Eq. (37). The only ambiguity left is the sign of m, which is equivalent to which side of the phase transition does δ settle, i.e., in the SSB or the PM phase. We show that statement with the same arguments as before, which also prompted us to include the graphic showing the approximate symmetry of the variational ground state error w.r.t. the coupling δ. This additionally yields the reference to the claim in the footnote the referee was asking for in the next question just below. We will resubmit this manuscript with the reference to this comment and its attachment and acknowledge Referee 2 for their constructive, clarifying, and helpful critique.

On the sixth line of page 19, I would advise against using footnotes that can be mistook for exponents. Also, is there a reference for the information in the footnote (the bias of the variational energy) or is it an observation of the authors?

A: Thank you for suggesting this clearer typographic choice. We have swapped the footnote marker to symbols. We do not have a direct source for the bias of the variational energy. We computed it numerically exactly through the free fermion framework and the numerical packages of Ref. [64]. We have attached a plot to this comment, which shows the variational ground state energy error as a function of the perturbative coupling δ. We hope this plot clears things up.

Towards the end of 5.2.2. there is a reference to Fig. 8(c) which does not exist.

A: Thank you for spotting that typo. The label is now corrected to Fig. 8(a).

I find the explanation for the influence of the choice of symmetric vs. nonsymmetric tensors on the spectrum of the TM is a bit rushed and sandwiched in the discussion of a different spectrum (the entanglement Hamiltonian spectrum, last paragraphs before Section 6), making it easy to miss.

A: We appreciate the remark and acknowledge the brevity with which we go over this specialized detail. We have expanded the explanations and added a discussion of the matter in Section 2 and 3. Furthermore, at the very end of Section 2, when we previously talked about shedding more light onto the puzzle of the different spectra of the TM when enforcing the Z2-symmetry or not, we have added the cross-reference to the section (Section 5.2.3) where we discuss this in more detail.

It would be nice to give it some more entity and discuss whether the relevant boundary conditions can be implemented in the toy model of the paper.

A: On the implementation of the boundary conditions in the toy model of our paper: Indeed, it remains open to further investigations to incorporate other boundary conditions in our toy model which could correspond to different spectra.

Attachment:

MPS-TFM-attachement-plot.pdf

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