The formation of the spectrum of pregalactic inhomogeneities in the CDM and HDM of the universe

Details The formation of the spectrum of pregalactic inhomogeneities in the CDM and HDM of the universe The formation of the spectrum of pregalactic inhomogeneities in the CDM and HDM of the universe

May 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990an....311..193k&link_type=abstract

Astronomische Nachrichten (ISSN 0004-6337), vol. 311, no. 3, 1990, p. 193-196.

Mathematics

Logic

Cosmic Plasma, Cosmology, Dark Matter, Galactic Evolution, Relativity, Galactic Clusters, Gravitational Fields, Perturbation Theory, Transfer Functions

Scientific paper

The evolution of large-scale cosmological density perturbations in CDM and HDM universe containing weakly interacting relativistic particles with number density to be the model free parameter is considered. The dependence of parameters of the large-scale structure on the collisionless particle numbers is discussed. A new cosmological test of the total number of light weakly interacting particles in the universe is proposed.

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