Dark Matter Interpretation of the Super-Kamiokande Antineutrino Excess and Predictions for JUNO

Fuente: arXiv
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Main Authors: Granelli, Alessandro, Pascoli, Silvia, Rosauro-Alcaraz, Salvador
Format: Preprint
Published: 2026
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author Granelli, Alessandro
Pascoli, Silvia
Rosauro-Alcaraz, Salvador
author_facet Granelli, Alessandro
Pascoli, Silvia
Rosauro-Alcaraz, Salvador
contents Super-Kamiokande has reported a small excess of electron antineutrino events in the 20 MeV energy range, in the search for the diffuse supernova neutrino background. We interpret this signal as a possible indication of dark matter that annihilates dominantly into neutrinos, pointing to a thermal dark matter candidate with $s$-wave annihilation and with mass in the tens of MeV range. This mass scale naturally fits into rich dark sector extensions of the Standard Model. Neutrino experiments, including JUNO, will be able to test this hypothesis in the coming years.
format Preprint
id arxiv_https___arxiv_org_abs_2605_20162
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Dark Matter Interpretation of the Super-Kamiokande Antineutrino Excess and Predictions for JUNO
Granelli, Alessandro
Pascoli, Silvia
Rosauro-Alcaraz, Salvador
High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
Super-Kamiokande has reported a small excess of electron antineutrino events in the 20 MeV energy range, in the search for the diffuse supernova neutrino background. We interpret this signal as a possible indication of dark matter that annihilates dominantly into neutrinos, pointing to a thermal dark matter candidate with $s$-wave annihilation and with mass in the tens of MeV range. This mass scale naturally fits into rich dark sector extensions of the Standard Model. Neutrino experiments, including JUNO, will be able to test this hypothesis in the coming years.
title Dark Matter Interpretation of the Super-Kamiokande Antineutrino Excess and Predictions for JUNO
topic High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2605.20162