Cosmic structure from dark matter

Details Cosmic structure from dark matter Cosmic structure from dark matter

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...204....3o&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 204, no. 1-2, Oct. 1988, p. 3-9.

Astronomy and Astrophysics

Astrophysics

10

Astronomical Models, Dark Matter, Galactic Evolution, Cosmology, Luminosity

Scientific paper

The present distribution of galaxies is estimated based on the linear growth of primordial adiabatic fluctuation in flat universe models dominated by dark matter. On the large scales, the canonical Press-Schechter (1974) mechanism is found to provide good agreement with observational data derived from luminosity functions of galaxies and clusters for all models considered, regardless of their chemical composition. On the small scales, the pure warm model best fits the observational data.

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