Pith. sign in

REVIEW 2 cited by

Is electroweak baryogenesis dead?

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1704.08911 v2 pith:GYKR3Y6U submitted 2017-04-28 hep-ph

classification hep-ph
keywords baryogenesiselectroweakmodelsaboveasymmetrycouplingsdemonstratedfine
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

Electroweak baryogenesis is severely challenged in its traditional settings: the Minimal Supersymmetric Standard Model, and in more general two Higgs doublet models. Fine tuning of parameters is required, or large couplings leading to a Landau pole at scales just above the new physics introduced. The situation is somewhat better in models with a singlet scalar coupling to the Higgs so as to give a strongly first order phase transition due to a tree-level barrier, but even in this case no UV complete models had been demonstrated to give successful baryogenesis. Here we point out some directions that overcome this limitation, by introducing a new source of CP violation in the couplings of the singlet field. A model of electroweak baryogenesis requiring no fine tuning and consistent to scales far above 1 TeV is demonstrated, in which dark matter plays the leading role in creating a CP asymmetry that is the source of the baryon asymmetry.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 2 Pith papers

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

  1. Lepton sourced baryon asymmetry in the fourth generation model

    hep-ph 2026-01 reject novelty 5.0 of 10

    A fourth-generation model is claimed to yield the observed baryon asymmetry η_B ≈ 10^-10, but the derivation sets the matching scale equal to the t' quark mass while also adopting a value about nine times smaller.

  2. Populating dark sectors with relativistic bubble walls

    hep-ph 2024-12 conditional novelty 3.0 of 10

    Relativistic bubble walls can pair-produce dark matter much heavier than the phase transition scale, which then free-streams as warm dark matter.

Pith tools