Book/Proceedings

PUBDB-2018-02580

http://join2-wiki.gsi.de/foswiki/pub/Main/Artwork/join2_logo100x88.png Axions, WIMPs and WISPs: proceedings, 14th Patras workshop, PATRAS 2018, Hamburg, Germany, June 18-22, 2018

Lindner, A. (Editor)DESY* ; Kozlowski, T. (Editor)Extern*

2018
Verlag Deutsches Elektronen-Synchrotron Hamburg
ISBN: 9783945931226

This record in other databases:  

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

Report No.: DESY-PROC-2018-03

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): Weakly interacting slim particle ; Weakly interacting slender particle ; Weakly interacting sub-eV particle ; PATRAS 2018 ; WIMPs ; Axions ; WISPs ; Weakly interacting massive particles ; Hamburg

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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

Appears in the scientific report 2019

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Linked articles:

http://join2-wiki.gsi.de/foswiki/pub/Main/Artwork/join2_logo100x88.png Preprint Carenza, P. ; Co', G. ; Fischer, T. ; Giannotti, M. ; Mirizzi, A. (Corresponding author)Extern* ; Rauscher, T.
Axion emission and detection from a Galactic supernova
[10.3204/PUBDB-2018-02580]     Files  Fulltext by arXiv.org BibTeX | EndNote: XML, Text | RIS

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