0000000000543345

AUTHOR

Anze Slosar

showing 2 related works from this author

Observables sensitive to absolute neutrino masses. II

2008

In this followup to Phys. Rev. D 75, 053001 (2007) [arXiv:hep-ph/0608060] we report updated constraints on neutrino mass-mixing parameters, in light of recent neutrino oscillation data (KamLAND, SNO, and MINOS) and cosmological observations (WMAP 5-year and other data). We discuss their interplay with the final 0nu2beta decay results in 76-Ge claimed by part of the Heidelberg-Moscow Collaboration, using recent evaluations of the corresponding nuclear matrix elements, and their uncertainties. We also comment on the 0nu2beta limits in 130-Te recently set by Cuoricino, and on prospective limits or signals from the KATRIN experiment.

PhysicsMass numberNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsAstrophysics (astro-ph)Cosmic background radiationFOS: Physical sciencesAstrophysicsCMB cold spotHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)MINOSDouble beta decayHigh Energy Physics::ExperimentSensitivity (control systems)Nuclear Experiment (nucl-ex)NeutrinoNeutrino oscillationNuclear ExperimentPhysical Review D
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Sterile Neutrinos in Light of Recent Cosmological and Oscillation Data: a Multi-Flavor Scheme Approach

2008

Light sterile neutrinos might mix with the active ones and be copiously produced in the early Universe. In the present paper, a detailed multi-flavor analysis of sterile neutrino production is performed. Making some justified approximations allows us to consider not only neutrino interactions with the primeval medium and neutrino coherence breaking effects, but also oscillation effects arising from the presence of three light (mostly-active) neutrino states mixed with two heavier (mostly-sterile) states. First, we emphasize the underlying physics via an analytical description of sterile neutrino abundances that is valid for cases with small mixing between active and sterile neutrinos. Then,…

AstrofísicaSterile neutrinoParticle physicscosmological neutrinosAstrophysics::High Energy Astrophysical PhenomenaCosmic microwave backgroundFOS: Physical sciencesAstrophysics01 natural sciences7. Clean energyMiniBooNEHigh Energy Physics - Phenomenology (hep-ph)astro-ph0103 physical sciencesScale structurephysics of the early universe010306 general physicsneutrino propertiesPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstrophysics (astro-ph)Astronomy and Astrophysicshep-phHigh Energy Physics - PhenomenologyHigh Energy Physics::ExperimentNeutrinoPhenomenology (particle physics)Coherence (physics)
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