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三对角最大熵采样的更快动态规划

Faster dynamic programming for tridiagonal maximum-entropy sampling

Marcia Fampa, Jon Lee

arXiv 2610.08466首次发表:更新:

发表机构

Federal University of Rio de Janeiro; University of Michigan(里约热内卢联邦大学; 密歇根大学)

机构由 AI 辅助整理,请以论文原文为准。

AI 中文总结

本文针对三对角协方差矩阵的最大熵采样问题,提出更快的动态规划算法,将时间复杂度从O(n^5)降至O(ns^2)或O(ns),并给出闭式解,同时扩展至蜘蛛图结构。

AI 中文摘要

最大熵采样问题(MESP)旨在为阶数为$n$的协方差矩阵$C$寻找一个阶数为$s$且具有最大对数行列式的主子矩阵。为了方便起见,我们假设$C$是非奇异的。Al-Thani和Lee(2023)在$C$或$C^{-1}$为三对角矩阵时,以$O(n^5)$的时间复杂度解决了MESP。我们证明他们的递归中的内部最大化仅依赖于索引集的前缀,并且解的任何一部分的长度不超过$s$;这给出了一个$O(ns^2)$时间的算法,该算法为每个预算$t\le s$返回最优值。当$C^{-1}$为三对角矩阵时,$C$在缩放意义下是Ornstein--Uhlenbeck过程在不等间隔时间点观测到的协方差矩阵,此时MESP变为在一条直线上选择点,其凹间隙函数具有Monge性质;这给出了一个$O(ns)$时间的算法,并且在一阶自回归情形下,有闭式解。仅给定$C$,当$C$或$C^{-1}$为三对角矩阵(允许对称置换)时,我们在$O(n^2)$时间内求解MESP,并在相同界限内识别这些情形。对于蜘蛛图,我们明确并锐化了运行时间对腿数的依赖,并借鉴Ohsaka关于星图的困难性结果,我们观察到,除非$\mathrm{P}=\mathrm{NP}$,否则运行时间的指数必须随腿数增长。

英文摘要

The maximum-entropy sampling problem (MESP) seeks, for an order-$n$ covariance matrix $C$, a principal submatrix of order $s$ with maximum log-determinant. Mostly for convenience, we assume that $C$ is nonsingular. Al-Thani and Lee (2023) solved MESP in $O(n^5)$ time when $C$ or $C^{-1}$ is tridiagonal. We show that the inner maximization of their recursion depends only on a prefix of the index set and that no piece of a solution is longer than $s$; this gives an $O(ns^2)$-time algorithm that returns the optimal value for every budget $t\le s$. When $C^{-1}$ is tridiagonal, $C$ is, up to scaling, the covariance matrix of an Ornstein--Uhlenbeck process observed at unevenly spaced times, and MESP becomes choosing points on a line under a concave gap function with the Monge property; this gives an $O(ns)$-time algorithm and, in the first-order autoregressive case, a closed-form solution. Given only $C$, we solve MESP in $O(n^2)$ time whenever $C$ or $C^{-1}$ is tridiagonal, up to a symmetric permutation, and we recognize these cases within the same bound. For spiders, we make explicit, and sharpen, the dependence on the number of legs, and, drawing on a hardness result of Ohsaka for stars, we observe that, unless $\mathrm{P}=\mathrm{NP}$, the exponent of the running time must grow with the number of legs.

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