N-body simulations of non-Gaussian distributions - Topological analysis and evolution

Details N-body simulations of non-Gaussian distributions - Topological analysis and evolution N-body simulations of non-Gaussian distributions - Topological analysis and evolution

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.171...17m&link_type=abstract

(IAU, European Regional Astronomy Meeting, 11th, La Laguna, Spain, July 3-8, 1989) Astrophysics and Space Science (ISSN 0004-640

Astronomy and Astrophysics

Astrophysics

Astronomical Models, Galactic Evolution, Many Body Problem, Algorithms, Statistical Tests, Topology, Velocity Distribution, White Noise

Scientific paper

With N-body simulations, the evolution of the large-scale structure of
the universe is studied, assuming non-Gaussian initial conditions. In
addition, the sensitivity of different statistical tests to the change
of the initial conditions is discussed.

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