English

Luminogenesis from Inflationary Dark Matter

High Energy Physics - Phenomenology 2015-05-08 v4 Cosmology and Nongalactic Astrophysics

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 TT15109T \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 TT15T \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.

Keywords

Cite

@article{arxiv.1309.1723,
  title  = {Luminogenesis from Inflationary Dark Matter},
  author = {Paul H. Frampton and Pham Q. Hung},
  journal= {arXiv preprint arXiv:1309.1723},
  year   = {2015}
}

Comments

8 double-column pages. No figures. Typos corrected. Added comments. Improved version

R2 v1 2026-06-22T01:22:21.616Z