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信息几何与功能方差分析的结合:一种精确的费舍尔信息分解及其在射电光度函数中的应用

Information Geometry meets Functional ANOVA: An Exact Fisher-Information Decomposition, with an Application to Radio Luminosity Functions

Marko Imbrišak, Krešimir Tisanić

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中文总结 AI 辅助

该研究将信息几何与功能方差分析结合,提出费舍尔信息的精确分解方法,并将其应用于射电光度函数模型的参数信息分解,还以植物CO2吸收实验作为示例验证方法。

中文摘要 AI 辅助

信息几何将拟合模型表示为一个流形,其度量为费舍尔信息。我们证明,对于非线性回归模型,该度量可在其协变量的Hoeffding-Sobol'(功能方差分析)通道上精确分解。将主效应和交互作用的得分贡献视为希尔伯特空间中的向量,它们的格拉姆矩阵精确再现了(高斯-牛顿)费舍尔信息度量,且该恒等式可扩展为费舍尔信息矩阵的精确加性分解,分解为主效应、交互作用和跨通道项:这是一种Sobol'式的参数信息而非输出方差的核算,等价于沿模型嵌入的环境费舍尔度量的通道分辨拉回。我们给出了带简短证明的精确分解定理(推导了中心化和非中心化费舍尔信息),定义了Sobol'指数的信息论类似物,表征了跨通道项的符号和有限样本行为,并描述了两种实用估计量。作为天体物理应用,我们分解了涵盖活动星系核(AGN)和恒星形成星系(SFG)的组合1.4 GHz射电光度函数模型的参数信息,该模型拟合于6dFGS-NVSS和VLA-COSMOS 3 GHz数据:该分解确定了每个星系种群和巡天在哪个光度处约束拟合,并揭示了光度函数 turnover附近的补偿性(“ sloppy”)通道组合。植物CO2吸收实验作为一个小型的全分类伴随示例。

英文摘要

Information geometry represents a fitted model as a manifold whose metric is the Fisher information. We show that, for a nonlinear regression model, this metric decomposes exactly across the Hoeffding-Sobol' (functional ANOVA) channels of its covariates. Treating the score contributions of main effects and interactions as vectors in a Hilbert space, their Gram matrix reproduces the (Gauss-Newton) Fisher information metric exactly, and this identity extends to an exact, additive decomposition of the Fisher information matrix into main-effect, interaction, and cross-channel terms: a Sobol'-type accounting for parameter information rather than output variance, and equivalently a channel-resolved pullback of the ambient Fisher metric along the model embedding. We give the exact decomposition theorem with a short proof (deriving both the centered and uncentered Fisher information), define information-theoretic analogues of Sobol' indices, characterize the sign and finite-sample behaviour of the cross-channel terms, and describe two practical estimators. As an astrophysical application we decompose the parameter information of a combined 1.4 GHz radio luminosity-function model spanning active galactic nuclei (AGN) and star-forming galaxies (SFG), fit to 6dFGS-NVSS and VLA-COSMOS 3 GHz data: the decomposition localizes where in luminosity each population and survey constrains the fit, and exposes the compensating ("sloppy") channel combinations near the luminosity-function turnover. A plant CO2-uptake experiment serves as a small, fully categorical companion example.

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