Pregalactic inhomogeneity in hot dark matter model of the universe

Details Pregalactic inhomogeneity in hot dark matter model of the universe Pregalactic inhomogeneity in hot dark matter model of the universe

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990esasp.311..283k&link_type=abstract

In ESA, Plasma Astrophysics p 283-285 (SEE N91-15046 06-90)

Astronomy and Astrophysics

Astrophysics

Boltzmann Transport Equation, Dark Matter, Galactic Evolution, Transfer Functions, Universe, Algorithms, Cosmology, Gravitational Fields, Inhomogeneity, Mathematical Models

Scientific paper

The development of small potential perturbations of the gravitational field and matter of a hot dark matter model in the presence of light weakly interacting particles is considered. Transfer functions and their dependence on the number of massive collisionless particles which today are the dynamical dark matter are found. Effective algorithms for building numerical simulation of the development of small inhomogeneities in this model are investigated.

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