6533b825fe1ef96bd12828e0

RESEARCH PRODUCT

Decaying sterile neutrinos and the short baseline oscillation anomalies

Ivan EstebanPedro A. N. MachadoMona DentlerJoachim KoppJoachim Kopp

subject

Sterile neutrinoParticle physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesElectron7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentMiniBooNEHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesMuon neutrino010306 general physicsNeutrino oscillationParticle Physics - PhenomenologyBosonPhysicshep-ex010308 nuclear & particles physicsOscillationHigh Energy Physics::Phenomenologyhep-ph3. Good healthHigh Energy Physics - PhenomenologyHigh Energy Physics::ExperimentNeutrinoParticle Physics - Experiment

description

The MiniBooNE experiment has observed a significant excess of electron neutrinos in a muon neutrino beam at source-detector distances too short to be compatible with standard neutrino oscillations. The most straightforward explanation for this signal in terms of oscillations between Standard Model neutrinos and a new, sterile, neutrino, is disfavored by null results from experiments looking for muon neutrino disappearance. Here, we discuss the possibility that MiniBooNE data are instead explained by a sterile neutrino that decays quickly back into active neutrinos plus a light boson. The flavor composition of the secondary neutrinos is determined by the sterile neutrino mixing angles, and we show that the data is best explained if the sterile neutrino mixes mostly with electron neutrinos. The preferred range for the mass of the sterile neutrino is between 100 eV and 1 keV. We argue that the model can easily satisfy cosmological constraints because it has the "secret interactions" mechanism built-in. Accommodating in addition to the MiniBooNE anomaly also the LSND, reactor, and gallium anomalies is possible, but in this case the model needs to be extended to avoid cosmological limits.

https://doi.org/10.1103/physrevd.101.115013