Preprint

PUBDB-2021-00114

http://join2-wiki.gsi.de/foswiki/pub/Main/Artwork/join2_logo100x88.png Axion emission and detection from a Galactic supernova

Carenza, P. ; Co', G. ; Fischer, T. ; Giannotti, M. ; Mirizzi, A. (Corresponding author)Extern* ; Rauscher, T.

2019

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Please use a persistent id in citations: doi:10.3204/PUBDB-2018-02580  doi:10.3204/PUBDB-2021-00114

Report No.: DESY-PROC-2018-03; arXiv:1808.04101

Abstract: 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.

Keyword(s): axion: absorption ; Cherenkov counter: water ; supernova ; galaxy ; oxygen ; KAMIOKANDE

Note: 4 pages. Contributed to the 14th Patras Workshop on Axions, WIMPs and WISPs, DESY in Hamburg, June 18 to 22, 2018

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Contributing Institute(s):

1. Any Light Particle Search (ALPS)

Research Program(s):

1. 6211 - Extreme States of Matter: From Cold Ions to Hot Plasmas (POF3-621) (POF3-621)

Experiment(s):

1. Any Light Particle Search

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Database coverage:
; Published

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Linked articles:

http://join2-wiki.gsi.de/foswiki/pub/Main/Artwork/join2_logo100x88.png Book/Proceedings Lindner, A. (Editor)DESY* ; Kozlowski, T. (Editor)Extern*
Axions, WIMPs and WISPs: proceedings, 14th Patras workshop, PATRAS 2018, Hamburg, Germany, June 18-22, 2018
201814th "Patras" Workshop on Axions, WIMPs and WISPs, PATRAS 2018, HamburgHamburg, Germany, 18 Jun 2018 - 22 Jun 20182018-06-182018-06-22 Hamburg : Verlag Deutsches Elektronen-Synchrotron, DESY-PROC viii, 103 pages : illustrations (2018) [10.3204/PUBDB-2018-02580]2018     Files BibTeX | EndNote: XML, Text | RIS

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