Summary
Sampling from complex high-dimensional data sets with very few positive elements (high magnetization) is challenging. The authors develop new methods that work efficiently for such data in statistical physics models called Ising models and in Bayesian sparse linear regression used in statistics. They show their sampling algorithms run in polynomial time even at very low temperatures and with certain constraints, improving on prior work. They also reduce the number of measurements needed to accurately infer sparse signals in noisy data. Their approach relies on exploiting sparsity and shared underlying mathematical structures in these problems.
sparsitysamplingIsing modelsSherrington–Kirkpatrick modelBayesian sparse linear regressionhigh-dimensional datamagnetizationannealingAlmeida–Thouless lineGaussian spike-and-slab posterior
Authors
Syamantak Kumar, Purnamrita Sarkar, Kevin Tian, Yusong Zhu
Abstract
Sparsity is a powerful structural resource in optimization and statistics. We develop frameworks for leveraging sparsity in sampling problems over the Hamming slice $\mathcal{X}_k^d:=\{\mathbf{x}\in\{\pm 1\}^d:|\{i:\mathbf{x}_i=1\}|=k\}$, in high-dimensional regimes where $k\ll d$ (i.e., where $\mathcal{X}_k^d$ is \emph{highly magnetized}). We use our frameworks to design improved samplers for canonical problems in the study of \emph{Ising models} and \emph{Bayesian sparse linear regression}. Our first main result considers the \emph{Sherrington--Kirkpatrick} (SK) model restricted to fixed-magnetization slices $\mathcal{X}_k^d$. We give a polynomial-time sampler for fixed-magnetization SK models at any inverse temperature $β>0$, under arbitrary external fields, provided that $k\le c_βd$ for an appropriate constant $c_β$. By combining this result with an annealing strategy for estimating normalizing constants, we obtain polynomial-time samplers for the SK model at arbitrarily low temperatures under a sufficiently strong external field of strength $h$. In the large-$β$ limit, our framework permits sampling at field strengths within constant factors of the \emph{Almeida--Thouless line} delineating the replica-symmetric and replica-symmetry-breaking regions ([dAT78]), improving polynomially over the field strength $h(β)$ required by the recent work of [BAR26]. Our second main result concerns the measurement complexity of polynomial-time Bayesian sparse linear regression. Recent work by [KSTZ25] shows how to sample from the canonical \emph{Gaussian spike-and-slab posterior} with expected sparsity $k$, at any signal-to-noise ratio, given $n\gtrsim k^3\log^3 d$ Gaussian measurements. We improve this requirement to $n\gtrsim k^{3/2}\log^2 d+k\log^3 d$, using a common sparsity-aware framework underlying both our results.