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arxiv: 1709.09691 · v2 · submitted 2017-09-27 · ✦ hep-ph

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Probing the baryogenesis and dark matter relaxed in phase transition by gravitational waves and colliders

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classification ✦ hep-ph
keywords darkmatterbaryogenesisgravitationalphaserelaxedsignalstransition
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The cosmological phase transition with Q-balls production mechanism can explain the baryogenesis and dark matter simultaneously, where constraints on dark matter masses and reverse dilution are significantly relaxed. We study how to probe this scenario by collider signals at QCD next-to-leading order and gravitational wave signals.

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Cited by 1 Pith paper

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  1. Dark Matter Production from Bubble Collisions during a First-Order Phase Transition at the End of Inflation

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    Bubble collisions during a first-order phase transition at the end of inflation can generate the observed dark matter abundance in a restricted region of parameter space via direct production and spectator decays.