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Gravitational wave signals of dark matter freeze-out

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arxiv 2006.07313 v4 pith:SEDMJAT7 submitted 2020-06-12 hep-ph astro-ph.COhep-ex

classification hep-phastro-ph.COhep-ex
keywords darkmattergravitationalfreeze-outwavesabundanceaccompanybackground
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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.

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Cited by 1 Pith paper

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  1. Gravitational waves from supercooled phase transitions in conformal Majoron models of neutrino mass

    hep-ph 2024-12 conditional novelty 6.0 of 10

    A detailed scan of conformal U(1)' Majoron models finds that supercooled phase transitions produce gravitational waves detectable by LIGO, LISA, and ET, and that current null data already exclude part of the parameter space.

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