The formation of the spectrum of inhomogeneity of the dark matter in pregalactic cosmic plasma

Details The formation of the spectrum of inhomogeneity of the dark matter in pregalactic cosmic plasma The formation of the spectrum of inhomogeneity of the dark matter in pregalactic cosmic plasma

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989plap.work..359k&link_type=abstract

In ESA, Proceedings of an International School and Workshop on Plasma Astrophysics, Volume 1 p 359-362 (SEE N89-24910 18-75)

Astronomy and Astrophysics

Astrophysics

Cosmic Plasma, Cosmology, Dark Matter, Galactic Evolution, Collisionless Plasmas, Density Distribution, Perturbation Theory, Relativistic Particles, Transfer Functions, Universe

Scientific paper

The dynamics of large-scale cosmological perturbations of density in the Universe containing, together with ordinary interacting particles, both heavy nonbaryonic particles (which today are the dynamical dark matter) and weakly interacting relativistic particles with number density as the model free parameter. Transfer functions of the growing adiabatic and isothermal perturbation modes are obtained. The dependence of parameters of the large-scale structure of the Universe on the collisionless relativistic particle number is discussed. A cosmological test of the total number of light weakly interacting particles in the Universe is proposed.

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