6533b850fe1ef96bd12a85eb

RESEARCH PRODUCT

An improved cosmological bound on the tau-neutrino mass

José W. F. ValleSergio PastorA.d. Dolgov

subject

PhysicsNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)High Energy Physics::PhenomenologyFOS: Physical sciencesFísicaAstrophysicsUpper and lower boundsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)NucleosynthesisTau neutrinoHigh Energy Physics::ExperimentNeutrinoBar (unit)

description

We consider the influence of non-equilibrium electronic neutrinos (and anti-neutrinos) on the neutron-to-proton ratio. These neutrinos would come from massive $\nu_\tau$ annihilations $\bar \nu_\tau \nu_\tau \rightarrow \bar \nu_e \nu_e$. For sufficiently large $\nu_\tau$ masses this new effect would strongly enhance the (n/p)-ratio, leading to a very stringent bound on the $\nu_\tau$ mass, even adopting a rather weak upper bound on the effective number on neutrino species during nucleosynthesis.

10.1016/0370-2693(96)00718-6http://dx.doi.org/10.1016/0370-2693(96)00718-6