The gravity-induced quasi-Gaussian correlation hierarchy

Details The gravity-induced quasi-Gaussian correlation hierarchy The gravity-induced quasi-Gaussian correlation hierarchy

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...392....1b&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 392, no. 1, June 10, 1992, p. 1-14.

Astronomy and Astrophysics

Astrophysics

159

Astronomical Models, Cosmology, Spatial Distribution, Correlation, Equations Of Motion, Gravitational Effects, Universe, Voids

Scientific paper

The hierarchy that first emerges from a Gaussian field, with a given initial spectrum, owing to the nonlinearities of the dynamics in an expanding universe, is calculated. The density distribution is significantly different from a Gaussian distribution, and is found to be asymmetrical, always with a positive density, and with an extended large tail for the large overdensities. Extrapolations toward high nonlinear regimes are also discussed.

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