AI summary · arXiv: 2610.40598v1 · cs.DS
On Zeros and Algorithms for Disordered Systems II: The Antiferromagnetic Ising Model up to Kesten-Stigum
The essentials
The paper proves zero-freeness and deterministic polynomial-time partition-function approximation for the antiferromagnetic Ising model on random regular graphs at every fixed inverse temperature below Kesten–Stigum.
Question
Can the partition function of the antiferromagnetic Ising model on uniformly random regular graphs be approximated to arbitrarily high accuracy throughout the replica-symmetric regime? The paper also asks whether Fisher zeros remain away from the corresponding real inverse-temperature interval.
Method
The authors analyze uniformly random d-regular graphs for fixed d ≥ 3 through the configuration model, combining Jensen’s formula, complex moment estimates, cycle-based analytic reweighting, and truncation of atypical contributions. For any fixed 0 < δ < 1 and inverse temperature between 0 and (1 − δ) times the Kesten–Stigum threshold, they prove a constant-width zero-free strip with probability 1 − o(1). Barvinok interpolation then uses O(log(n/ε)) Taylor terms to obtain multiplicative error between exp(−ε) and exp(ε) in time (n/ε)^C, where C depends on d and δ.
Findings
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Result
A deterministic polynomial-time algorithm approximates the partition function to arbitrarily high accuracy with high probability over the random graph, for every fixed inverse temperature strictly below Kesten–Stigum.
See the passage in the paper
In this paper, we make progress on the high-temperature (small $\beta$) side of the aforementioned conjecture by giving the first polynomial-time approximate counting algorithm for all $\beta$ up to $\beta_{\mathsf{KS}}(d)$.
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Result
With high probability, the partition function has no Fisher zeros in a constant-width complex neighborhood of any real interval ending a fixed distance below Kesten–Stigum.
See the passage in the paper
The key to guaranteeing correctness of our algorithm is the absence of zeros in a constant-width strip around the interval $[0,(1-\delta)\cdot\beta_{\mathsf{KS}}(d)]$ for any $\delta>0$.
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Result
The interpolation algorithm obtains the required multiplicative accuracy by retaining only logarithmically many Taylor terms.
See the passage in the paper
To approximate $$q_{G}(p(1))=\tfrac{1}{2^{|V|}}Z_{G}(\beta)$$ up to a multiplicative factor $e^{\varepsilon}$, it suffices to truncate the Taylor series of $\log(q_{G}(p(z)))$ after $O(\log(n/\varepsilon))$ terms (see [5, Lemma 2.2.1]).
Limitations
- The counting algorithm does not directly provide an approximate sampling algorithm because the model without an external field is not self-reducible.
See the passage in the paper
Our approximate counting algorithm does not immediately imply an approximate sampling algorithm for the Gibbs measure $\mu_{G,\beta}$. This is because we only work with the antiferromagnetic Ising model without external field, which is not self-reducible in the sense of [30].
- The authors do not know how to efficiently certify the approximation guarantee on a given input graph.
See the passage in the paper
Unfortunately, we do not know how to show that our algorithm is certifiable in this sense. In particular, we do not know how to certify the requisite zero-freeness of $Z_{G}(\beta)$ given $G$.
- The theorems require a fixed positive gap below Kesten–Stigum and do not establish the endpoint itself.
Why it matters
The result extends high-accuracy average-case approximate counting to every fixed inverse temperature below the replica-symmetry-breaking threshold, beyond the range reached by the prior sampling methods discussed in the paper. It establishes the counting and zero-freeness sides of the proposed coincidence of average-case phase transitions, without resolving sampling or rapid mixing throughout that regime.
Written by AI from the paper. Passages are checked word for word against the text we analysed; the rest may contain errors.
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