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Strong electroweak phase transition in t-channel simplified dark matter models

Simone Biondini, Philipp Schicho, Tuomas V. I. Tenkanen

2022Journal of Cosmology and Astroparticle Physics22 citationsDOI

Abstract

Abstract Beyond the Standard Model physics is required to explain both dark matter and the baryon asymmetry of the universe, the latter possibly generated during a strong first-order electroweak phase transition. While many proposed models tackle these problems independently, it is interesting to inquire whether the same model can explain both. In this context, we link state-of-the-art perturbative assessments of the phase transition thermodynamics with the extraction of the dark matter energy density. These techniques are applied to a next-to-minimal dark matter model containing an inert Majorana fermion that is coupled to Standard Model leptons via a scalar mediator, where the mediator interacts directly with the Higgs boson. For dark matter masses 180 GeV < M χ ≲ 300 GeV, we discern regions of the model parameter space that reproduce the observed dark matter energy density and allow for a first-order phase transition, while evading the most stringent collider constraints.

Topics & Concepts

PhysicsParticle physicsElectroweak interactionDark matterBaryon asymmetryDark energyHiggs bosonPhase transitionScalar field dark matterPhysics beyond the Standard ModelMAJORANABaryogenesisWarm dark matterLight dark matterStandard Model (mathematical formulation)FermionLeptonCosmologyNuclear physicsAstrophysicsQuantum mechanicsElectronGauge (firearms)HistoryArchaeologyParticle physics theoretical and experimental studiesDark Matter and Cosmic PhenomenaCosmology and Gravitation Theories
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