A Galactic supernova (SN) axion signal would be detected in a future neutrino Mton-class water Cherenkov detector, such as the proposed Hyper-Kamiokande in Japan. The main detection channel for axions is absorption on the oxygen nuclei in the water. The subsequent oxygen de-excitation leads to a potentially detectable gamma signal. In this contribution we present a calculation of the SN axion signal and discuss its detectability in Hyper-Kamiokande.
Cite
@article{arxiv.1808.04101,
title = {Axion emission and detection from a Galactic supernova},
author = {Pierluca Carenza and Giampaolo Co' and Tobias Fischer and Maurizio Giannotti and Alessandro Mirizzi and Thomas Rauscher},
journal= {arXiv preprint arXiv:1808.04101},
year = {2019}
}
Comments
4 pages. Contributed to the 14th Patras Workshop on Axions, WIMPs and WISPs, DESY in Hamburg, June 18 to 22, 2018