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Bootstrapping the $R$-matrix

by Zhao Zhang

Submission summary

Authors (as registered SciPost users): Zhao Zhang
Submission information
Preprint Link: https://arxiv.org/abs/2504.17773v5  (pdf)
Date submitted: Oct. 3, 2025, 9:40 a.m.
Submitted by: Zhao Zhang
Submitted to: SciPost Physics
Ontological classification
Academic field: Physics
Specialties:
  • High-Energy Physics - Theory
  • Mathematical Physics
Approach: Theoretical

Abstract

A bootstrap program is presented for algebraically solving the $R$-matrix of a generic integrable quantum spin chain from its Hamiltonian. The Yang-Baxter equation contains an infinite number of seemingly independent constraints on the operator valued coefficients in the expansion of the $R$-matrices with respect to their spectral parameters, with the lowest order one being the Reshetikhin condition. These coefficients can be solved iteratively using Kennedy's inversion formula, which reconstructs the $R$-matrix after an infinite number of steps. For a generic Hamiltonian, the procedure could fail at any step, making the conditions useful as an integrability test. However in all known examples they all turn out to be satisfied whenever the lowest order condition is. It remains to be understood whether they are all implied by the Reshetikhin condition.

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
Current status:
Awaiting resubmission

Reports on this Submission

Report #2 by Anonymous (Referee 2) on 2025-12-15 (Invited Report)

Strengths

  1. Interesting submission dealing with the characterisation of integrability in one-dimensional spin chains (also applicable to fermion models) with nearest-neighbour interaction.
  2. Accessible to a wider audience, not only experts in the field.

Weaknesses

  1. Improved clarity required in part of the discussion.

Report

The problem revisits a topic that was the subject of a lot of interest late last century, and has been revived in the last five years or so. The fundamental question is whether the so-called Reshetikhin condition, a necessary condition for models derived as the logarithmic derivative of the transfer matrix with periodic boundary conditions for regular solutions of the Yang-Baxter equation, is also sufficient for existence of the Yang-Baxter equation solution. The author's analysis supports this conjecture. It is argued that if the Reshetikhin condition is shown to hold, it follows in principle (not necessarily in practice) that there exists a recursive means to generate the operator coefficients of the series expansion of the solution of the Yang-Baxter equation.

I found the presentation to reasonably clear and accessible. The topic has been unresolved for some decades and for this reason I believe that there is a case to argue that the results warrant publication in SciPost The author includes welcomed discussion about connections to a lattice version of the Poincare group. The appendix contains some examples to illustrate the process.

Requested changes

  1. I have some reservations about the clarity of Sect. 7, and I request that modifications are made before the manuscript can be accepted. In this section, the solution of the Yang-Baxter equation is assumed to have non-difference form, satisfying

\begin{align} &R_{x,x+1}(\nu,\lambda) R_{x-1,x}(\nu,\mu) R_{x,x+1}(\lambda,\mu) \ &\qquad = R_{x-1,x}(\lambda,\mu) R_{x,x+1}(\nu,\mu) R_{x-1,x}(\nu,\lambda). \end{align} In the author's analysis, the solution is expanded as \begin{align} R_{x,x+1}(\mu,\nu)=1_{x,x+1}+\sum_{n=1}^\infty\frac{(\mu-\nu)^n}{n!} R_{x,x+1}^{(n)}(\nu). \end{align}

The author makes the comment

"If there is a solution of $h'$ that makes the LHS of (32) decompose into the difference of two bi-local operators, then the generalized Reshetikhin condition is satisfied, and the Hamiltonian would likely turn out integrable."

where Eq. (32) is given by

\begin{align} &[h_{12}(\mu)+h_{23}(\mu) ,[h_{12}(\mu),\,h_{23}(\mu)]+[h_{12}(\mu),h_{23}'(\mu)] +[h_{23}(\mu),h_{12}'(\mu)] \ &\qquad \frac{1}{2}[h_{12}(\mu),h_{12}'(\mu)] +\frac{1}{2}[h_{23}(\mu),h_{23}'(\mu)] = X_{12}(\mu)-X_{23}(\mu).
\end{align
}

It has recently been proposed in

A. Hokkyo Integrability from a single conservation law in quantum spin chains, doi:10.48550/arXiv.2508.20713

that the relation above indeed implies the existence of an infinite sequence of conserved charges in involution. This reference should be included.

Then, the author goes on to make the following claim, regarding integrability of the Hubbard model, in a footnote:

"This serves as a way to determine $h'(0)$ without knowledge of the $R$-matrix, which was believed impossible according to Ref. [31]."

I am happy if the author can prove otherwise, but I do not see any reason to assume that there is a unique solution $h'(0)$ to the following equation \begin{align} &[h_{12}(0)+h_{23}(0),[h_{12}(0),\,h_{23}(0)]]+[h_{12}(0),h_{23}'(0)] +[h_{23}(0),h_{12}'(0)] \ &\qquad \qquad +\frac{1}{2}[h_{12}(0),h_{12}'(0)] +\frac{1}{2}[h_{23}(0),h_{23}'(0)]= X_{12}(0)-X_{23}(0).
\qquad\qquad (
) \end{align*} where $X(0)$ and the parametric form $h(\mu)$ are both unknown. The operators $X_{jk}(\mu)$ are, apparent in the generalised Reshetikhin condition derivation, functions of $h'(\mu)$, $h''(\mu)$, and $R_{x,x+1}^{(3)}(\mu)$. That these three functions could be bootstrapped from Eq. $(*)$, without explicit knowledge of the dependence on $\mu$, is very speculative.

To be clear, for the Hubbard model the spectral parameter dependence $\mu$ of the local Hamiltonian $h_{x,x+1}(\mu)$ is not in any way related to the familiar coupling parameter $U$ that appears in the Hubbard Hamiltonian; i.e., $U$ is genuinely a constant parameter in the $R$-matrix, (much like $\Delta$ in the $XXZ$ chain) and the spectral parameter $\mu$ provides a two-parameter generalisation of the Hubbard model. By contrast, for example, the two coupling parameters in the Hubbard model analogue described in

J. Links, Extended integrability regime for the supersymmetric $U$ model, J. Phys. A: Math. Gen. 32 (1999) L315 doi:10.1088/0305-4470/32/27/104

are related to two independent spectral parameters.

It appears there is some confusion about the subtle issue of the origin of parameters in integrable models. This needs to be clarified.

Continuing, the reason for the author's comment

"as we have not solved $h'(\mu)$ from Kennedy’s method, or even $h''(0)$ for that matter. "

is puzzling with regard to the significance of $h''(0)$. In general, given a solution $R_{x,x+1}(\mu,\nu)$ and any differentiable function $f$ then $R_{x,x+1}(\tilde{\mu},\tilde{\nu})$ with $\tilde{\mu}=f(\mu)$, $\tilde{\nu}=f(\mu)$, also solves the Yang-Baxter equation without difference property. There is no requirement that $f(0)=0$. Only when the difference property holds is it required that $f$ be a linear function in order to maintain the difference property. So I do not understand the significance in $h''(0)$, over $h''(\mu_0)$ generally for some constant $\mu_0$. I request that the author explains this aspect.

Recommendation

Ask for minor revision

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Author:  Zhao Zhang  on 2026-01-06  [id 6201]

(in reply to Report 2 on 2025-12-15)

I thank the referee for the positive assessment and the valuable feedback.

Here are my responses to the issues raised preceding the changes made in a forth-coming resubmission:

  1. I was not aware that A.Hokkyo addressed the non-fundamental integrable models in his latest update. So this reference will be added here.

  2. Of course, Eq. (32) does not have a closed form solution, but h'(0) could be solved in the following way. Given a matrix representation of h in a specific model, one can parameterize h'(0) element-wise using a set of unknown variables. Then Kennedy's inversion method can be used to express X_12 in terms of these unknowns. Next, following the same procedure detailed in Sec. 3, the (candidate) X_12 solved from Kennedy's method are not necessarily satisfying Eq. (32). So actually requiring the X_12 obtained like that indeed is a solution of Eq. (32) would result in a set of equations on those unknown variables, solving which specifies the matrix h'(0). In a way, it is like a self-consistency solution.

  3. That being said, Eq.(32) contains no spectral parameter, so it is not enough to determine h(mu) as a function. And in the text, I only mentioned h''(0) to emphasize that point. Upon hindsight, the confusion it brought was not worth it. So i will remove that comment. But there was no misunderstanding of the origin of parametrization on my part in the first place, as I was not even familiar with the example that the referee kindly mentioned.

In summary, Sec. 7 contains nothing new to Ref. 31 other than putting Eq. 32 in a symmetric form that generalizes Eq. 9, and that h'(0) can be solved in a similar manner as the integrability test/R-matrix bootstrap in Sec. 3. But this is not significant, as it does not help either purpose for the models in question in Sec. 7.

I would appreciate if referee could let me know if the explanation is unsatisfactory.

Report #1 by Anonymous (Referee 1) on 2025-12-7 (Invited Report)

Strengths

  1. The results that the author is trying to prove are particularly interesting and would be useful for the community. However, the arguments he uses are not very clear and require clarification.

Weaknesses

  1. The bootstrap program is not properly explained; more steps in the proof are needed, as well as further clarification in the examples of Appendix B.
  2. The author is ignoring a recent result concerning the proof of the necessary and sufficient condition of the Reshetikhin condition (arXiv:2508.20713).

Report

Even though the potential results of the paper would be particularly interesting, I believe that, in its current form, the paper does not prove the main claims stated in the abstract and introduction. A major revision is recommended.

I will first mention the points where I believe the proof contains gaps, and afterward suggest some minor and stylistic changes (in Requested changes).

Since Section 3 contains the main result of the paper, I recommend several clarifications here:

1) Equation (9) is the main result, however I do not understand how to obtain an expression siminal to (4) for R^{(2m+1)}. Can the author please comment on this? 2) how to see that (9) is the microscopic reason behind the conservation of higher local charges Q^{(2m+1)}? 3) It is not clear what the purpose of the bootstrapping method is. According to the abstract, it should provide a way to reconstruct the R-matrix starting from an integrable Hamiltonian (which would indeed be an interesting result). However, in the text, the author states that it can also be used as a way to check integrability. This second approach has already been addressed in several previous papers: 2206.08390, 2206.08679, 2501.18400, and 2508.20713. The author can for example explain how the R matrix of the models in Appendix B can be constructed. 4) The author mentions that the even coefficient of the R can be read from (4) and the odd from (9) by using the Kennedy's inversion formula. This method is not explained properly. Can the author provides the first several coefficients explicitly? 5) at page 5, the author claims: "These identities are expressed in terms of many new operators... input for an integrability test". How this test wold work since the expression (9) contains infinite terms? As I mentioned, according to A.Hokkyo, (6) is enough to show integrability or non integrability. But supposing this is not correct, how would you use (9)? Even if it works up to some coefficient n, how is it guaranteed that it works always? Section 4. 1) The sentence "Unlike the definitions of classical integrability..." is not clear. 2) As before, "Hence the Reshetikhin condition has been conjectured...". Recently it has been proved by A. Hokkyo. Section 7. 1) About footnote 9: In which step of ref 31. it is believed impossible to determine h'(0) without knowing R? Appendix A. 1) Can the author please comment on how to use eq. (4) to rewrite the LHS of Eq A.1 to obtain (9)? Appendix B. 1) I would put more emphasis on the examples. I think a,b operators (without the superscript) have not been defined. Can you use this relations to obtain coefficients in the R? What is the Kennedy's inversion formula explicitly?

Requested changes

The major changes are discussed in the Report. Here I list the minor and stylistic changes: 1. After equation (1), you could just say that the YBE remains satisfied up to a different normalization of the R-matrix (which corresponds to a shift by a constant term in the Hamiltonian) 2. In the equation (9), I would write some brackets in (a<->b) to make the expression easier to read 3. Appendix A. I believe it would be clearer to manipulate each term on the right-hand side separately and then equate them afterward.

Recommendation

Ask for major revision

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Author:  Zhao Zhang  on 2026-01-06  [id 6202]

(in reply to Report 1 on 2025-12-07)

I thank the referee for the helpful suggestions. Let me try to clarify some of the questions before a resubmission is made accordingly.

Section 3: 1) There is no closed form equation for odd order coefficients. Each of them is instead an independent input that can only be solved self-consistently (in the case that the model is indeed integrable) using Kennedy's Eq. (10). 2) I have not been able to establish the eq. (9) as the symmetry current correspondence of the conserved charges other than observing that the number of additional constraints that are referred to here as higher order Reshetikhin conditions is the same as independent commutation relations of the conserved charges (the triangles in Fig. 1). So I should have been more careful about that statement. 3) The purpose is primarily to point out the nice structure of eq. (9). The following two usages can be considered by-products along the way. First, for generic Hamiltonians, it serves as an integrability check, as there may or may not be a self-consistent solution for the odd order coefficients. Second, for the models that do satisfy the test, namely integrable ones, repeating this procedure reconstructs the R-matrix purely from the Hamiltonian either after infinite steps, or by making an educated guess after a just a few. The appearance of 2508.20713 does make the first purpose irrelevant, as the Reshetikhin condition itself is nothing new. But it is still not obvious at all that they are all implied by Reshetikhin condition. So a more physical proof than 2508.20713 would still need to address this apparent contradiction. Regarding Appendix B, I can give explicitly the first few lowest order coefficients, but obtaining the full R-matrix this way would either require iterating infinite steps or guesswork done element-wise for the matrix representation of the R-matrix, which is neither so illuminating, nor leading to anything new for these known examples. 4) The Kennedy's formula refers to Lemma 1 (eq. 16) or Ref. 3, which is recast in the form of my eq. (11) (and later generalized to eq. 24). Knowing this mathematical property, the extensive explanation in Sec.3 should be understandable. I can provide the first few coefficient, which I already implicitly did in parts of Appendix B, but they are obtained from symbolic calculation softwares, where the procedure is easy to implement. I do not think this is a suitable calculation to do by hand. I am happy to provide my Mathematica code, but this is really elementary manipulation. 5) I agree with the referee that this is not so practical as a test. I mention this just to remind the readers that the attempt to construct the R-matrix iteratively could (at least in principle) fail at any step. The whole point of this approach is that we can try to construct the R-matrix of any Hamiltonian assuming it is integrable, which may or may not turn out to be true. Hokkyo's result also can only show integrability, not non-integrability, as models like Hubbard do not pass the test.

Section 4: 1) In classical integrability, sometimes the conserved charges do not have to commute with each other. This is different from the definition in quantum context. I can explain in more detail listing some references. 2) At the time of writing, I did not feel comfortable citing Hokkyo's proof as it is not peer-reviewed, and I could not follow the technical details of his appendices, where all the new treatments were hidden. In any case, it does not explain why eq. (9) are not independent. But if both referees have vetted that proof, I am happy reflect that result in my writing.

The rest of the requests are quite straightforward, which will be directly addressed in the resubmission.

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