6533b851fe1ef96bd12a907d
RESEARCH PRODUCT
Relic density of neutrinos with primordial asymmetries.
Georg G. RaffeltSergio PastorTeguayco Pintosubject
PhysicsParticle physicsmedia_common.quotation_subjectAstrophysics (astro-ph)Quark modelHigh Energy Physics::PhenomenologyFOS: Physical sciencesGeneral Physics and AstronomyFísicaAstrophysicsUniverseMassless particleHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Big Bang nucleosynthesisNucleosynthesisAntimatterHigh Energy Physics::ExperimentNeutrinoLeptonmedia_commondescription
We study flavor oscillations in the early Universe, assuming primordial neutrino-antineutrino asymmetries. Including collisions and pair processes in the kinetic equations, we not only estimate the degree of flavor equilibration, but for the first time also kinetic equilibration among neutrinos and with the ambient plasma. Typically, the restrictive big-bang nucleosynthesis bound on the nu(e)(nu) over bar (e) asymmetry indeed applies to all flavors as claimed in the previous literature, but fine-tuned initial asymmetries always allow for a large surviving neutrino excess radiation that may show up in precision cosmological data.
| year | journal | country | edition | language |
|---|---|---|---|---|
| 2008-08-22 | Physical review letters |