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This paper establishes tight bounds on the stochastic-gradient query complexity required to sample smooth, strongly log-concave distributions in fixed dimensions. The derived complexity scales logarithmically with the condition number and inversely with accuracy, while explicitly accounting for oracle noise variance. These theoretical limits are critical for understanding the fundamental efficiency of sampling algorithms used in variational inference and generative modeling.
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Tight Sampling Complexity with stochastic gradient oracles in Fixed Dimensions

arXiv2 min read

arXiv:2609.12590v1 Announce Type: cross Abstract: We investigate the stochastic-gradient query complexity of sampling smooth strongly log-concave distributions in any fixed Euclidean dimension. The potential is $\mu$-strongly convex and $L$-smooth, with an unknown mode in the ball of radius $\mu^{-1/2}$ about the origin. We have access to unbiased stochastic oracles with the variance at most $\sigma^2$. For every $\sigma^2\ge0$ and total variation (TV) accuracy $0<\varepsilon\le1/10$, we prove that the tight complexity of sampling a distribution within $\epsilon$-TV distance from the target distribution is \[ N^\star_{\text{TV}}=\Theta\!\left(\log(1+\kappa)+ \frac{\sigma^2}{\mu\epsilon}\right), \] where $\kappa:=\frac L\mu$ is the condition number. Note that this complexity bound is simultaneously tight for the condition number $\kappa$ and accuracy $\epsilon$. Besides, our tight complexity bound is adaptive to noiseless setting $\sigma=0$, which is $ N^\star_{\text{TV}}=\Theta\!\left(\log(1+\kappa)\right)$.

Abstract:We investigate the stochastic-gradient query complexity of sampling smooth strongly log-concave distributions in any fixed Euclidean dimension. The potential is $\mu$-strongly convex and $L$-smooth, with an unknown mode in the ball of radius $\mu^{-1/2}$ about the origin. We have access to unbiased stochastic oracles with the variance at most $\sigma^2$. For every $\sigma^2\ge0$ and total variation (TV) accuracy $0<\varepsilon\le1/10$, we prove that the tight complexity of sampling a distribution within $\epsilon$-TV distance from the target distribution is \[ N^\star_{\text{TV}}=\Theta\!\left(\log(1+\kappa)+ \frac{\sigma^2}{\mu\epsilon}\right), \] where $\kappa:=\frac L\mu$ is the condition number. Note that this complexity bound is simultaneously tight for the condition number $\kappa$ and accuracy $\epsilon$. Besides, our tight complexity bound is adaptive to noiseless setting $\sigma=0$, which is $ N^\star_{\text{TV}}=\Theta\!\left(\log(1+\kappa)\right)$.

Statistics Theory (math.ST); Machine Learning (cs.LG); Probability (math.PR)

arXiv:2609.12590 [math.ST]

(or arXiv:2609.12590v1 [math.ST] for this version)

https://doi.org/10.48550/arXiv.2609.12590 Focus to learn more arXiv-issued DOI via DataCite (pending registration)

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Full text under the publisher's open licence · 218 words

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