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Luminogenesis from Inflationary Dark Matter (1309.1723v4)

Published 6 Sep 2013 in hep-ph and astro-ph.CO

Abstract: A cosmological model is introduced in which dark matter plays a dominant role throughout the history of the universe, and is the only matter present for temperatures $T \gtrsim T_{15} \sim 109$ GeV. The gauge group is $SU(3) \times SU(6){DM} \times U(1)_Y$ and unifies in such a way that luminous matter is generated at $T \sim T{15}$ with the correct amount and eventual asymmetry. Construction of more highly sensitive direct detectors of dark matter (e.g. XENON1T) is encouraged. We offer a new explanation of why grand unification theories involving only luminous matter may be fatally flawed.

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