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Anatomy of the Electroweak Phase Transition for Dark Sector induced Baryogenesis

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arxiv 2210.14352 v2 pith:XT54J6Q6 submitted 2022-10-25 hep-ph

classification hep-ph
keywords darkmodelelectroweakmatterphaseportalsectorsinglet
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

We investigate the electroweak phase transition patterns for a recently proposed baryogenesis model with CP violation originated in the dark sector. The model includes a complex scalar singlet-Higgs boson portal, a $U(1)_l$ gauge lepton symmetry with a $Z^\prime$ gauge boson portal and a fermionic dark matter particle. We find a novel thermal history of the scalar sector, featuring a $Z_2$ breaking singlet vacuum in the early Universe driven by a dark Yukawa coupling, that induces a one-step strongly first order electroweak phase transition. We explore the parameter space that generates the observed matter-antimatter asymmetry and dark matter relic abundance, while being consistent with constraints from electric dipole moment and collider searches, and dark matter direct detection bounds. The complex singlet can be produced via the Higgs portal and decays into Standard Model particles after traveling a certain distance. We explore the reach for long-lived singlet scalars at the {\unit[13]{TeV}} Large Hadron Collider with $\mathcal{L}=\unit[139]{fb^{-1}}$ and show its impact on the parameter space of the model. Setting aside currently unresolved theoretical uncertainties, we estimate the gravitational wave signatures detectable at future observatories.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Real-Time Simulation of Asymmetry Generation in Fermion-Bubble Collisions

    hep-ph 2024-12 conditional novelty 6.0 of 10

    Real-time tensor-network scattering of fermions off a complex-mass bubble wall in 1+1D yields a nonzero C asymmetry, captured by new magnitude and phase observables.

  2. Thermalization effects on the dynamics of growing vacuum bubbles

    hep-ph 2024-11 conditional novelty 6.0 of 10

    Bubble-wall terminal velocity depends on plasma thermalization; non-equilibrium and free-streaming regimes give slower or different walls, and stationary solutions can be bypassed by runaways.

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