6533b853fe1ef96bd12ac2a5

RESEARCH PRODUCT

Sterile neutrino signals from supernovae

P. KeränenP. KeränenJ. RiittinenM. MyyryläinenJukka MaalampiJukka Maalampi

subject

PhysicsNuclear and High Energy PhysicsSterile neutrinoParticle physics010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyFOS: Physical sciencesWeinberg angle01 natural sciences3. Good healthStandard ModelNuclear physicsSupernovaHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)supernovat0103 physical sciencesInvariant massHigh Energy Physics::ExperimentNeutrino010306 general physicsElectron neutrinoMass gap

description

We investigate the effects of a mixing of active and sterile neutrinos on the ratios of supernova electron neutrino flux ($F_e$) and antineutrino flux ($F_{\bar e}$) to the total flux of the other neutrino and antineutrino flavours ($F_a$). We assume that the heaviest (in the normal hierarchy) Standard Model neutrino $\nu_3$ mixes with a sterile neutrino resulting in a pair of mass eigenstates with a small mass gap. Using the density matrix formalism we solve numerically the the evolution of neutrino states in the envelope of a supernova and determine the flux ratios $F_e/F_a$ and $F_{\bar{e}}/F_a$ as a function of the active-sterile mixing angle and for the experimentally allowed range of the standard active-active mixing angle $\theta_{13}$.

10.1103/physrevd.76.125026http://arxiv.org/abs/0708.3337