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Mixed Dark Matter from Axino Distribution

S. A. Bonometto, F. Gabbiani, A. Masiero

astro-pharXiv:astro-ph/9305010

Abstract

We study the possibility of mixed dark matter obtained through the phase space distribution of a single particle. An example is offered in the context of SUSY models with a Peccei-Quinn symmetry. Axinos in the 100 keV range can naturally have both thermal and non-thermal components. The latter one arises from the lightest neutralino decays and derelativizes at z ~ 104.

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