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Axion emission and detection from a Galactic supernova
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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.
Forward citations
Cited by 2 Pith papers
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Axion-induced pair production: a new strategy for axion detection
Axion-induced pair production in a nuclear electric field is the dominant detection channel for axions above roughly 10 MeV and substantially improves projected supernova axion sensitivities.
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Status and Perspectives on Axion Searches
A concise review of axion and ALP search experiments, their recent limits, and upcoming projects.
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