Gravitational clustering from scale-free initial conditions

Details Gravitational clustering from scale-free initial conditions Gravitational clustering from scale-free initial conditions

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988mnras.235..715e&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 235, Dec. 1, 1988, p. 715-748. Research supported by th

Astronomy and Astrophysics

Astronomy

432

Galactic Clusters, Gravitational Effects, Many Body Problem, Autocorrelation, Galactic Structure, Mass Distribution

Scientific paper

A series of N-body experiments have been performed in order to investigate gravitational clustering from scale-free initial conditions in an Einstein-de Sitter universe. The three-dimensional shapes, angular momenta, and internal velocity distributions of clumps are studied. It is shown that in general, although nonlinear clustering destroys the hierarchical arrangement of the initial conditions, their scaling properties still determine the scaling properties of the mass distribution at high density contrast.

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