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arXiv · 2407.10123

Gravitational wave signatures of first-order phase transition in two-component dark matter model

Seyed Yaser Ayazi·Mojtaba Hosseini·Rouzbeh Rouzbehi
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Abstract

Here, we consider a classically scale-invariant extension of the Standard Model (SM) with two-component dark matter (DM) candidates, including a Dirac spinor and a scalar DM. We probe the parameter space of the model, constrained by relic density and direct detection, and investigate the generation of gravitational waves (GWs) produced by an electroweak first-order phase transition. The analysis demonstrates that there are points in the parameter space, leading to a detectable GW spectrum arising from the first-order phase transition, which is also consistent with the DM relic abundance and direct detection bounds. These GWs could be observed by forthcoming space-based interferometers such as the Big Bang Observer, Decihertz Interferometer Gravitational-wave Observatory, and Ultimate-Decihertz Interferometer Gravitational-wave Observatory.

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Seyed Yaser Ayazi, Mojtaba Hosseini, Rouzbeh Rouzbehi. 2024-07-14. Gravitational wave signatures of first-order phase transition in two-component dark matter model. https://doi.org/10.1103/physrevd.110.115027

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