An important theoretical issue in cosmology is to understand the physical processes that occured during the gravitational collapse of the matter which gave rise to the observed large-scale structure of the universe. We review here several well-motivated approximations for studying the dynamics of dark matter in non-linear regimes.

Non-Linear Evolution of Self-Gravitating Collisionless Matter

MATARRESE, SABINO;PANTANO, ORNELLA;LUCCHIN, FRANCESCO;
1994

Abstract

An important theoretical issue in cosmology is to understand the physical processes that occured during the gravitational collapse of the matter which gave rise to the observed large-scale structure of the universe. We review here several well-motivated approximations for studying the dynamics of dark matter in non-linear regimes.
1994
Galaxy formation, International School of Physics "Enrico Fermi", Proceedings of the International School of Physics "Enrico Fermi"
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11577/172457
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