Gravitational wave signals of dark matter freeze-out
arXiv:2006.07313 · doi:10.1007/JHEP02(2021)022
Abstract
We study the stochastic background of gravitational waves which accompany the sudden freeze-out of dark matter triggered by a cosmological first order phase transition that endows dark matter with mass. We consider models that produce the measured dark matter relic abundance via (1) bubble filtering, and (2) inflation and reheating, and show that gravitational waves from these mechanisms are detectable at future interferometers.
17 pages, 6 figures, 2 tables. Version to appear in JHEP
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- Probing superheavy dark matter with gravitational waves
- Electroweak phase transition and gravitational waves in a two-component dark matter model
- Dark Matter Candidates and Searches
- Correlated signals of first-order phase transitions and primordial black hole evaporation
- Finite-temperature bubble nucleation with shifting scale hierarchies
- Heavy dark matter and Gravitational waves
- Boosted dark matter from primordial black holes produced in a first-order phase transition
- Gravitational Waves From Dark Sectors, Oscillating Inflatons, and Mass Boosted Dark Matter
- Annihilogenesis
- Hydrodynamic effects on the filtered dark matter produced by a first-order phase transition
- Gravitational wave effects and phenomenology of a two-component dark matter model
- Sub-GeV dark matter and nano-Hertz gravitational waves from a classically conformal dark sector
- Non-thermal production of heavy vector dark matter from relativistic bubble walls
- Gravitational waves from supercooled phase transitions in conformal Majoron models of neutrino mass
- Reconstructing early universe evolution with gravitational waves from supercooled phase transitions
- Correlated gravitational wave and microlensing signals of macroscopic dark matter
- Detectability of the Phase Transition Gravitational Waves in the DFSZ axion Model