Graph explorer

Warm baryogenesis

We show that a baryon asymmetry can be generated by dissipative effects during warm inflation via a supersymmetric two-stage mechanism, where the inflaton is coupled to heavy mediator fields that then decay into light species through B- and CP-violating interactions. In contrast with thermal GUT baryogenesis models, the temperature during inflation is always below the heavy mass threshold, simultaneously suppressing thermal and quantum corrections to the inflaton potential and the production of dangerous GUT relics. This naturally gives a small baryon asymmetry close to the observed value, although parametrically larger values may be diluted after inflation along with any gravitino overabundance. Furthermore, this process yields baryon isocurvature perturbations within the range of future experiments, making this an attractive and testable model of GUT baryogenesis.

8 nodes9 linksoverview previewWarm baryogenesis
8 nodes9 links
Warm baryogenesis8 visible / 8 total nodes / 15 links
Co-authorshipCo-authorshipCo-authorshipCo-authorshipCo-authorshipCo-authorshipAuthorshipAuthorshipAuthorshipAuthorshipTopic signalTopic signalTopic signalRelated contextRelated contextWWarm baryogenesispreprint / 2012AMar Bastero-GilResearcherAArjun BereraResearcherARudnei O. RamosResearcherAJoao G. RosaResearcherThep-ph13193 worksTastro-ph.CO6979 worksThep-th13268 works
PaperSignal 107 links

Warm baryogenesis

preprint / 2012

Open