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Weakly Nonlinear Evolution of Topology of Large-scale Structure

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arxiv astro-ph/9501076 v1 pith:IEFKO2UN submitted 1995-01-20 astro-ph

classification astro-ph
keywords contoursevolutiongenusisodensitynonlinearperturbationstatisticstheory
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abstract

The gravitational evolution of the genus and other statistics of isodensity contours of the density field is derived analytically in a weakly nonlinear regime using second-order perturbation theory. The effect of final smoothing in perturbation theory on the statistics of isodensity contours is also evaluated. The resulting analytic expression for the genus is compared with $N$-body numerical simulations and exhibits a good agreement.

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  1. Non-Gaussian Expansion of Minkowski Tensors in Redshift Space

    astro-ph.CO 2025-07 conditional novelty 6.0 of 10

    A first derivation of the non-Gaussian, redshift-space ensemble averages of two rank-2 Minkowski tensors, with percent-level agreement against Quijote simulations for smoothing scales above 20 Mpc/h.

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