Gravitational clustering of galaxies - The probability distribution function

Details Gravitational clustering of galaxies - The probability distribution function Gravitational clustering of galaxies - The probability distribution function

May 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...340...23z&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 340, May 1, 1989, p. 23-28. Research supported by the University of Toronto

Statistics

Computation

19

Computational Astrophysics, Galactic Clusters, Gravitational Effects, Many Body Problem, Probability Distribution Functions, Astronomical Models, Computerized Simulation, Perturbation Theory

Scientific paper

The evolution of the probability distribution function, f(N), for finding N particles in a given volume for an infinite, homogeneous gravitating system with a Poissonian initial space distribution and a zero initial velocity distribution is determined. The evolution of f(N) was found to be consistent with the results of N-body simulations. The method is used to find f(N) for the same system, but with a nonzero initial velocity distribution.

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