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Rejuvenating the matter power spectrum: restoring information with a logarithmic density mapping

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arxiv 0903.4693 v2 pith:BUZVDQY2 submitted 2009-03-27 astro-ph.CO

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keywords powerspectrumdensityinformationlogarithmicmappingproceduresmaller
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We find that nonlinearities in the dark-matter power spectrum are dramatically smaller if the density field first undergoes a logarithmic mapping. In the Millennium simulation, this procedure produces a power spectrum with a shape hardly departing from the linear power spectrum for k <~ 1 h/Mpc at all redshifts. Also, this procedure unveils pristine Fisher information on a range of scales reaching a factor of 2-3 smaller than in the standard power spectrum, yielding 10 times more cumulative signal-to-noise at z=0.

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  1. Detecting Modeling Bias with Continuous Time Flow Models on Weak Lensing Maps

    astro-ph.CO 2025-05 conditional novelty 6.0 of 10

    Continuous time flow models estimating full-field probability densities detect out-of-distribution weak lensing maps from baryonic effects with AUROC up to 0.95, outperforming feature-level normalizing flow baselines.

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