Luminogenesis from Inflationary Dark Matter

preprint2015arXivOpen access

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≳T15∼109T \gtrsim T_{15} \sim 10^9 GeV. The gauge group is SU(3)×SU(6)DM×U(1)YSU(3) \times SU(6)_{DM} \times U(1)_Y and unifies in such a way that luminous matter is generated at T∼T15T \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.

Explore this paper’s authors, topics and related work.

Building this map preview

BZPEER is loading the nearby papers, people, topics and institutions for this page.

Reviews 0

Write a reviewWrite

No reviews yet.

Discussion 0

Add a commentWrite

No comments yet.