Atmospheric Sterile Neutrinos
arXiv:1202.0725 · doi:10.1007/JHEP07(2012)112
Abstract
We study production of sterile neutrinos in the atmosphere and their detection at Super-Kamiokande. A sterile neutrino in the mass range is produced by muon or pion decay, and decays to an electron-positron pair and an active neutrino. Such a decay of the sterile neutrino leaves two electron-like Cherenkov rings in the detector. We estimate the sterile neutrino flux from the well-established active neutrino fluxes and study the number of the decay events in the detector. The upper bounds for the active-sterile mixings are obtained by comparing the -like events from the sterile neutrino decays and the observed data by Super-Kamiokande. The upper bound for the muon type mixing is found to be for , which is significantly loosened compared to the previous estimation. We demonstrate that the opening angle and the total energy of the rings may serve as diagnostic tools to discover the sterile neutrinos in further data accumulation and future upgraded facilities. The directional asymmetry of the events is a sensitive measure of the diminishment of the sterile neutrino flux due to the decays on the way to the detector.
23 pages, 14 figures; a comment on the active-sterile oscillation is added (v2)
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- A facility to Search for Hidden Particles at the CERN SPS: the SHiP physics case
- Heavy neutrino search in accelerator-based experiments
- New constraints on Heavy Neutral Leptons from Super-Kamiokande data
- Searches for Atmospheric Long-Lived Particles
- Effects of Long-lived 10 MeV Scale Sterile Neutrino on Primordial Elemental Abundances and Effective Neutrino Number
- Lepton Universality in the MSM
- Searching for light long-lived neutralinos at Super-Kamiokande
- Atmospheric axion-like particles at Super-Kamiokande
- Sterile neutrino dark matter with dipole interaction
- Testing Heavy Neutral Leptons in Cosmic Ray Beam Dump experiments
- Probing heavy neutrinos in the COMET experiment