Pith. sign in

REVIEW 1 cited by

Baryogenesis and Leptogenesis

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 hep-ph/0411301 v1 pith:LPEIGBN4 submitted 2004-11-22 hep-ph astro-phhep-th

classification hep-phastro-phhep-th
keywords baryonscosmologydarkenergygeneralmodelsparticleuniverse
verification ladder T0 review T1 audit T2 compute T3 formal

Signed reviews

No signed human review yet.

0 comments
read the original abstract

The energy budget of the universe contains two components, dark matter and dark energy, about which we have much to learn. One should not forget, however, that the baryonic component presents its own questions for particle cosmology. In the context of cosmology, baryons would have annihilated with their antiparticles in the early universe, leaving a negligible abundance of baryons, in disagreement with that observed. In this general lecture, delivered at the SLAC 2004 Summer Science Institute, I provide an overview of the central issue and the general principles behind candidate models. I also briefly discuss some popular examples of models that are firmly rooted in particle physics.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 1 Pith paper

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

  1. Enhancement of Weak Interactions in Phase Transitions in Condensed Matter and Early Universe

    hep-ph 2025-09 conditional novelty 4.0 of 10

    Weak-interaction energy differences between left- and right-handed states are amplified by the number of atoms in the critical nucleus, which can reach 10^9 to 10^10 in real materials.

Pith tools