0000000000591411

AUTHOR

A.d. Dolgov

showing 3 related works from this author

Screening of long-range leptonic forces by cosmic background neutrinos.

1995

The absence of dispersion effects of the SN~1987A neutrino pulse has been used to constrain novel long-range forces between neutrinos and galactic baryonic or non-baryonic matter. If these forces are mediated by vector bosons, screening effects by the cosmic neutrino background invalidate the SN~1987A limits and other related arguments.

PhysicsParticle physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaSolar neutrinoHigh Energy Physics::PhenomenologyDark matterCosmic background radiationFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsSolar neutrino problemCosmic neutrino backgroundHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Measurements of neutrino speedHigh Energy Physics::ExperimentNeutrino astronomyNeutrinoPhysical review. D, Particles and fields
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Primordial Nucleosynthesis, Majorons and Heavy Tau Neutrinos

1996

We determine the restrictions imposed by primordial nucleosynthesis upon a heavy tau neutrino, in the presence of nu-tau annihilations into Majorons, as expected in a wide class of particle physics models of neutrino mass. We determine the equivalent number of light neutrino species $N_{eq}$ as a function of nu-tau mass and the nu-tau-Majoron coupling $g$. We show that for theoretically plausible $g$ values $\gsim 10^{-4}$ present nucleosynthesis observations can not rule out nu-tau masses in the MeV range. Moreover, these models give $N_{eq} \leq 3$ in the nu-tau mass region 1-10 MeV, for very reasonable values of $g \geq 3 \times 10^{-4}$. The evasion of the cosmological limits brings new…

PhysicsNuclear and High Energy PhysicsParticle physicsRange (particle radiation)Astrophysics (astro-ph)High Energy Physics::PhenomenologyFOS: Physical sciencesFísicaFunction (mathematics)Coupling (probability)AstrophysicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Big Bang nucleosynthesisNucleosynthesisTau neutrinoLimit (mathematics)Neutrino
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An improved cosmological bound on the tau-neutrino mass

1996

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.

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)
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