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How to estimate Fisher information matrices from simulations

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arxiv 2305.08994 v3 pith:TJTGJD7O submitted 2023-05-15 stat.ME astro-ph.COastro-ph.IMphysics.data-an

classification stat.MEastro-ph.COastro-ph.IMphysics.data-an
keywords informationfisherusedcarloestimateestimatesmethodsmonte
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The Fisher information matrix is a quantity of fundamental importance for information geometry and asymptotic statistics. In practice, it is widely used to quickly estimate the expected information available in a data set and guide experimental design choices. In many modern applications, it is intractable to analytically compute the Fisher information and Monte Carlo methods are used instead. The standard Monte Carlo method produces estimates of the Fisher information that can be biased when the Monte-Carlo noise is non-negligible. Most problematic is noise in the derivatives as this leads to an overestimation of the available constraining power, given by the inverse Fisher information. In this work we find another simple estimate that is oppositely biased and produces an underestimate of the constraining power. This estimator can either be used to give approximate bounds on the parameter constraints or can be combined with the standard estimator to give improved, approximately unbiased estimates. Both the alternative and the combined estimators are asymptotically unbiased so can be also used as a convergence check of the standard approach. We discuss potential limitations of these estimators and provide methods to assess their reliability. These methods accelerate the convergence of Fisher forecasts, as unbiased estimates can be achieved with fewer Monte Carlo samples, and so can be used to reduce the simulated data set size by several orders of magnitude.

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Cited by 3 Pith papers

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    astro-ph.CO 2026-07 accept novelty 7.0 of 10

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  2. Climbing the $N$-point Ladder Part I: Information in the Higher-Order Configuration-Space Clustering of Dark Matter Halos

    astro-ph.CO 2026-07 conditional novelty 6.0 of 10

    On Quijote halos the config-space 3PCF supplies most higher-order Fisher information (especially on σ8 and Mν) while the connected 4PCF adds a robust further ~1.4–1.5× tightening.

  3. Cosmological information content of Betti curves and $k$-nearest neighbor distributions

    astro-ph.CO 2025-02 conditional novelty 6.0 of 10

    Betti curves and kNN distributions give similar cosmological constraints in Quijote simulations, with beta0/beta1 dominating Betti information and the two statistics only partially redundant.

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