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Non-local Electroweak Baryogenesis Part I : Thin Wall Regime

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arxiv hep-ph/9410281 v4 pith:HRG6VRLO submitted 1994-10-13 hep-ph astro-ph

classification hep-phastro-ph
keywords wallasymmetrybaryogenesisbaryoncondensateelectroweakfirstinteractions
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abstract

We investigate `non-local' schemes for baryogenesis at a first order electroweak phase transition, in which the effects of a $CP$ violating condensate on the bubble wall propagate into the unbroken phase where the sphaleron rate is unsupressed. Such a condensate exists in multi-Higgs extensions of the standard model, and may exist due to an instability in the minimal standard model. In this paper we first discuss the general problem of determining the $CP$ violating perturbations, distinguishing two regimes (quantum and classical). We then give an analytic treatment of quantum mechanical reflection in the thin wall regime, in which interactions with the plasma can be neglected as a particle propagates across the wall. We focus on leptons because of their much weaker coupling to the plasma. We argue that they are likely to be accurately described by this calculation, but quarks are not. The relative magnitude of the baryon asymmetry produced for different fermions depends on their relative Yukawa couplings ({\it not} their zero temperature masses), their transport properties and their interactions. We calculate the baryon asymmetry for various parameter ranges and conclude that asymmetries comparable with observations can be generated.

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Cited by 3 Pith papers

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  1. Defect-Mediated Conversion: Dark Matter from Cosmological Domain-Wall Scattering

    hep-ph 2026-08 conditional novelty 8.0 of 10

    Domain-wall cores containing a scalar condensate convert bath fermions into dark fermions, producing the observed dark matter relic abundance and dominating the yield over freeze-in by 30 to 100 times.

  2. Thermal Evolution and Hydrodynamic Filtering of Pseudoscalar Dark Matter

    hep-ph 2026-08 conditional novelty 6.0 of 10

    Hydrodynamic shock heating in a deflagration phase transition enhances the filtered dark matter abundance by factors of 4.3, 5.8, and 32 for benchmark masses of 1.78, 2.30, and 5.03 TeV.

  3. The Discriminant Power of Bubble Wall Velocities: Gravitational Waves and Electroweak Baryogenesis

    hep-ph 2025-04 conditional novelty 6.0 of 10

    Using entropy conservation in local thermal equilibrium, the authors compute bubble wall velocities in singlet-extended models and find a near-universal relation between phase transition strength measures, with conseq...

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