SN1987A still shining: A Quest for Pseudo-Dirac Neutrinos
arXiv:2105.12736 · doi:10.1103/PhysRevD.105.095019
Abstract
Ever since the discovery of neutrinos, we have wondered if neutrinos are their own antiparticles. One remarkable possibility is that neutrinos have a pseudo-Dirac nature, predicting a tiny mass difference between active and sterile states. We analyze the neutrino data from SN1987A in the light of active-sterile oscillations and find a mild preference () for . Notably, the same data is able to exclude with , the tiniest mass differences constrained so far. We further consider the next-generation of experiments and demonstrate their sensitivity exploring the nature of the neutrino mass.
arXiv comment5+3 pages, 7 Figures; added clarifications and additional checks in appendix
References in corpus (37)
- The fate of hints: updated global analysis of three-flavor neutrino oscillations
- Identifying the neutrino mass spectrum from a supernova neutrino burst
- Precise quasielastic neutrino/nucleon cross section
- Hyper-Kamiokande Design Report
- High-resolution supernova neutrino spectra represented by a simple fit
- Direct Bounds on Electroweak Scale Pseudo-Dirac Neutrinos from TeV LHC Data
- Pseudo-Dirac Neutrinos, a Challenge for Neutrino Telescopes
- Neutrino Oscillations and the Supernova 1987A Signal
- Detecting non-relativistic cosmic neutrinos by capture on tritium: phenomenology and physics potential
- Supernova neutrino physics with xenon dark matter detectors: A timely perspective
- Pseudo-Dirac Neutrinos in the New Standard Model
- Addressing the Majorana vs. Dirac Question with Neutrino Decays
- Deep Underground Neutrino Experiment (DUNE), Far Detector Technical Design Report, Volume II: DUNE Physics
- Measurement of the muon decay spectrum with the ICARUS liquid Argon TPC
- Fundamental physics with the diffuse supernova background neutrinos
- Pseudo-Dirac Scenario for Neutrino Oscillations
- Effects of sterile neutrinos on the ultrahigh-energy cosmic neutrino flux
- Pseudo-Dirac Neutrino Scenario: Cosmic Neutrinos at Neutrino Telescopes
- Mirror model for sterile neutrinos
- Comparative analysis of SN1987A antineutrino fluence
- The diffuse supernova neutrino flux, supernova rate and SN1987A
- Distinguishing Dirac and Majorana neutrinos by their gravi-majoron decays
- Decoherence and oscillations of supernova neutrinos
- Majorana vs Pseudo-Dirac Neutrinos at the ILC
- On the Impact of Neutrino Decays on the Supernova Neutronization-Burst Flux
- Implications of the Pseudo-Dirac Scenario for Ultra High Energy Neutrinos from GRBs
- New analysis of the SN 1987A neutrinos with a flexible spectral shape
- Pseudo-Dirac neutrinos via mirror-world and depletion of UHE neutrinos
- Quasi Dirac neutrino oscillations
- Three-Body Decays of Heavy Dirac and Majorana Fermions
- Quasi-Dirac neutrino oscillations at DUNE and JUNO
- The likelihood for supernova neutrino analyses
- IceCube Flavor Ratios with Identified Astrophysical Sources: Towards Improving New Physics Testability
- Neutrino mass from bremsstrahlung endpoint in coherent scattering on nuclei
- Shining Light on the Mass Scale and Nature of Neutrinos with
- Effects of degenerate sterile neutrinos on the supernova neutrino flux
- Coherence of oscillations in matter and supernova neutrinos
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- Naturally Light Dirac and Pseudo-Dirac Neutrinos from Left-Right Symmetry
- Astrophysical neutrino oscillations after pulsar timing array analyses
- Revisiting pseudo-Dirac neutrino scenario after recent solar neutrino data
- Probing Pseudo-Dirac Neutrinos with Astrophysical Sources at IceCube
- Solar Neutrinos at DARWIN
- Relic neutrino decay solution to the excess radio background
- Supernova Neutrinos: flavour conversion mechanisms and new physics scenarios
- Pseudo-Dirac Neutrinos and Relic Neutrino Matter Effect on the High-energy Neutrino Flavor Composition
- How Broad is a Neutrino?
- Constraining the pseudo-Dirac nature of neutrinos using astrophysical neutrino flavor data
- Cosmogenic neutrinos as probes of new physics
- Neutrino Theory Overview
- Cosmic neutrino background detection in the minimally extended Standard Model
- Boomerang mechanism explaining the excess radio background