Luminogenesis from Inflationary Dark Matter
Paul H. Frampton, Pham Q. Hung

TL;DR
This paper proposes a cosmological model where dark matter dominates early universe evolution, unifies gauge groups, and explains the origin of luminous matter and matter asymmetry, challenging traditional grand unification theories.
Contribution
It introduces a novel dark matter-centric cosmological model with a specific gauge group unification, explaining luminous matter generation and matter asymmetry.
Findings
Dark matter dominates for T > 10^9 GeV
Luminous matter is generated at T ~ 10^9 GeV
Challenges grand unification theories involving only luminous matter
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 GeV. The gauge group is and unifies in such a way that luminous matter is generated at 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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Taxonomy
TopicsDark Matter and Cosmic Phenomena · History and Developments in Astronomy · Atomic and Subatomic Physics Research
