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"
Galaxy formation, International School of Physics "Enrico Fermi"
File in questo prodotto:
Non ci sono file associati a questo prodotto.
Pubblicazioni consigliate

I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.

Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11577/172457
Citazioni
  • ???jsp.display-item.citation.pmc??? ND
  • Scopus ND
  • ???jsp.display-item.citation.isi??? ND
  • OpenAlex ND
social impact