A mixed dark matter model with a non-thermal volatile component: theory versus observation.

Details A mixed dark matter model with a non-thermal volatile component: theory versus observation. A mixed dark matter model with a non-thermal volatile component: theory versus observation.

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996apl%26c..33...41p&link_type=abstract

Astrophysical Letters and Communications, Vol. 33, Nos. 1 - 5, p. 41 - 47

Mathematics

Logic

Universe: Dark Matter

Scientific paper

The author investigates the properties of a particular type of MDM model in which the hot component derives from the decay of a heavier particle. She briefly presents the particle model which gives rise to such a cosmological scenario and then she calculates the linear evolution of the perturbations for a set of Cold + Volatile DM models. After normalizing the outcoming spectra to the COBE data the author discusses the properties of large structure such as bulk velocities, abundances of high redshift objects and mass variance.

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