Statistics – Computation
Scientific paper
May 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991mnras.250..458w&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 250, May 15, 1991, p. 458-476.
Statistics
Computation
15
Astronomical Models, Computational Astrophysics, Galactic Clusters, Gravitational Collapse, Gravitational Fields, Universe, Computerized Simulation, Cosmology, Formalism
Scientific paper
The present adhesion model-based one-dimensional simulations of gravitational clustering have yielded bound-object catalogs applicable in tests of analytical approaches to cosmological structure formation. Attention is given to Press-Schechter (1974) type functions, as well as to their density peak-theory modifications and the two-point correlation function estimated from peak theory. The extent to which individual collapsed-object locations can be predicted by linear theory is significant only for objects of near-characteristic nonlinear mass.
Heavens Alan F.
Peacock John A.
Shandarin Sergei F.
Williams Brian G.
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