SN1987A still shining: A Quest for Pseudo-Dirac Neutrinos

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 ($\Delta {\chi }^2\approx 3$) for $\delta m^2=6.31\times 10^{-20}{\mathrm{eV}}^2$. Notably, the same data is able to exclude $\delta m^2\sim [2.55,3.01]\times 10^{-20}{\mathrm{eV}}^2$ with $\Delta {\chi }^2>9$, 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.

5+3 pages, 7 Figures; added clarifications and additional checks in appendix

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• 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