2013/09/06 by Paul H. Frampton, Frampton, Paul H., Phạm Quang Hưng +2
Physics and Astronomy · #Atomic and Subatomic Physics Research #Cosmology and Nongalactic Astrophysics (astro-ph.CO) #Dark Matter and Cosmic Phenomena #FOS: Physical sciences #High Energy Physics - Phenomenology (hep-ph) #History and Developments in Astronomy #astro-ph.CO #hep-ph
paper · pdf · doi:10.48550/arxiv.1309.1723
8 double-column pages. No figures. Typos corrected. Added comments. Improved version
openalex publication_date 2013/09/06 · arxiv created 2015/05/07 · arxiv updated 2015/05/08 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
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 T15 ∼ 109 GeV. The gauge group is SU(3) × SU(6)DM × U(1)Y and unifies in such a way that luminous matter is generated at T ∼ T15 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.