Pith. sign in

REVIEW 4 cited by

Baryogenesis and Leptogenesis from Supercooled Confinement

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 2312.09282 v2 pith:RCNW35FH submitted 2023-12-14 hep-ph

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

Signed reviews

No signed human review yet.

0 comments
read the original abstract

We propose a framework of baryogenesis and leptogenesis that relies on a supercooled confining phase transition (PT) in the early universe. The baryon or lepton asymmetry is sourced by decays of hadrons of the strong dynamics after the PT, and it is enhanced compared to the non-confining case, which was the only one explored so far. This widens the energy range of the PT, where the observed baryon asymmetry can be reproduced, down to the electroweak scale. The framework then becomes testable with gravity waves (GW) at LISA and the Einstein Telescope. We then study two explicit realisations: one of leptogenesis from composite sterile neutrinos that realises inverse see-saw; one of baryogenesis from composite scalars that is partly testable by existing colliders and flavour factories.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 4 Pith papers

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

  1. Can the universe be matter-dominated after a supercooled first-order phase transition?

    hep-ph 2026-07 conditional novelty 7.0 of 10

    After a supercooled first-order phase transition, the scalar field's equation of state is set by the bubble-wall Lorentz factor γ*, and matter domination is delayed until a/a* ≃ γ* in the free-streaming limit.

  2. Bubble wall dynamics from nonequilibrium quantum field theory

    hep-ph 2025-04 conditional novelty 7.0 of 10

    The conventional kinetic equation of motion for bubble walls is incomplete, missing a condensate self-energy term that produces additional friction from particle production, mixing, and transition radiation.

  3. Prospecting bipartite Dark Matter through Gravitational Waves

    hep-ph 2024-12 conditional novelty 6.0 of 10

    A two-component dark matter model with an inert triplet scalar and a singlet fermion can explain the relic abundance while producing a strong electroweak phase transition and gravitational wave signals detectable by L...

  4. Holographic composite Higgs model and gravitational waves produced during first order phase transition

    hep-th 2025-05 conditional novelty 5.0 of 10

    In the soft-wall holographic composite Higgs model, the symmetry breaking transition is strongly first order with alpha up to 10^3 and beta/H between 10^5 and 5x10^6, producing gravitational waves peaked near the BBO/...

Pith tools