Constraining sterile neutrinos by core-collapse supernovae with multiple detectors
arXiv:2005.09168 · doi:10.1088/1475-7516/2020/10/038
Abstract
The eV-scale sterile neutrino has been proposed to explain some anomalous results in experiments, \textit{such as} the deficit of reactor neutrino fluxes and the excess of in LSND. This hypothesis can be tested by future core-collapse supernova neutrino detection independently since the active-sterile mixing scheme affects the flavor conversion of neutrinos inside the supernova. In this work, we compute the predicted supernova neutrino events in future detectors -- DUNE, Hyper-K, and JUNO -- for neutrinos emitted during the neutronization burst phase when the luminosity of dominates the other flavors. We find that for a supernova occurring within 10 kpc, the difference in the event numbers with and without sterile neutrinos allows to exclude the sterile neutrino hypothesis at more than confidence level robustly. The derived constraints on sterile neutrinos mixing parameters are comparably better than the results from cosmology and on-going or proposed reactor experiments by more than two orders of magnitude in the - plane.
24 pages, 12 figures, 4 tables
References in corpus (12)
- The Reactor Antineutrino Anomaly
- Light Sterile Neutrinos: A White Paper
- Statistical Significance of the Gallium Anomaly
- Stellar cooling bounds on new light particles: plasma mixing effects
- Supernova bound on keV-mass sterile neutrinos reexamined
- Bounds on light sterile neutrino mass and mixing from cosmology and laboratory searches
- Improved Constraints on Sterile Neutrino Mixing from Disappearance Searches in the MINOS, MINOS+, Daya Bay, and Bugey-3 Experiments
- Getting the Most from Detection of Galactic Supernova Neutrinos in Future Large Liquid-Scintillator Detectors
- Robust measurement of supernova spectra with future neutrino detectors
- MeV-scale reheating temperature and cosmological production of light sterile neutrinos
- IceCube Sterile Neutrino Searches
- The gallium anomaly reassessed using a Bayesian approach
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- The Present and Future Status of Heavy Neutral Leptons
- Supernova Neutrino Burst Detection with the Deep Underground Neutrino Experiment
- Snowmass White Paper: Beyond the Standard Model effects on Neutrino Flavor
- Neutrinos and nucleosynthesis of elements
- Towards Probing the Diffuse Supernova Neutrino Background in All Flavors
- Exploiting a future galactic supernova to probe neutrino magnetic moments
- Supernova neutrino fluxes in HALO-1kT, Super-Kamiokande, and JUNO
- New Resonances of Supernova Neutrinos in Twisting Magnetic Fields
- JUNO Physics and Detector
- Supernova Neutrinos: flavour conversion mechanisms and new physics scenarios
- Non-Standard Interactions of Supernova Neutrinos and Mass Ordering Ambiguity at DUNE
- Resonant Production of Light Sterile Neutrinos in Compact Binary Merger Remnants
- Neutrino interactions in liquid scintillators including active-sterile neutrino mixing
- Dark matter, supernova neutrinos and other backgrounds in direct dark matter searches. The ANDES laboratory prospects