Abstract

Purely self-gravitating systems of point particles have been extensively studied inastrophysics and cosmology, mainly through numerical simulations, but understandingof their dynamics still remains extremely limited. We describe here results ofa detailed study of a simple class of cold quasi-uniform initial conditions, forboth finite open systems and infinite systems. These examples illustrate well thequalitative features of the quite different dynamics observed in each case, andalso clarify the relation between them. In the finite case our study highlightsthe potential importance of energy and mass ejection prior to virialization, aphenomenon which has been previously overlooked. We discuss for both cases thevalidity of a mean-field Vlasov–Poisson description of the dynamics observed, andspecifically the question of how particle number should be extrapolated to test forit.

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