Inflaton freeze-out
arXiv:2110.05488 · doi:10.1103/PhysRevD.106.043537
Abstract
We study the possibility that, after inflation, the inflaton reaches thermal equilibrium with the Standard Model thermal bath and eventually freezes-out in the non-relativistic regime. When the inflaton decay is the sole source of (non-thermal) dark matter, its relic density is automatically suppressed. We delineate parameter space leading to the correct dark matter abundance. The model allows for a significant Higgs-inflaton coupling which may lead to invisible Higgs decay into inflaton pairs at the LHC.
14 pages, 3 figures; v2: matches version published in PRD (extended discussions, fixed typos, updated references)
References in corpus (10)
- The Standard Model Higgs boson as the inflaton
- Gauge Singlet Scalars as Cold Dark Matter
- Power-counting and the Validity of the Classical Approximation During Inflation
- Inflation with Non-Minimal Coupling: Metric vs. Palatini Formulations
- Higgs-Palatini Inflation and Unitarity
- Inflation, dark matter and dark energy in the string landscape
- The Higgs Portal to Cosmology
- Spectator Dark Matter
- Challenges for Inflaton Dark Matter
- Dark matter production and reheating via direct inflaton couplings: collective effects