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@PROCEEDINGS{Lindner:407652,
key = {407652},
editor = {Lindner, Axel and Kozlowski, Todd},
title = {{A}xions, {WIMP}s and {WISP}s: proceedings, 14th {P}atras
workshop, {PATRAS} 2018, {H}amburg, {G}ermany, {J}une 18-22,
2018},
address = {Hamburg},
publisher = {Verlag Deutsches Elektronen-Synchrotron},
reportid = {PUBDB-2018-02580, DESY-PROC-2018-03},
isbn = {9783945931226},
series = {DESY-PROC},
pages = {viii, 103 pages : illustrations},
year = {2018},
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.},
month = {Jun},
date = {2018-06-18},
organization = {14th "Patras" Workshop on Axions,
WIMPs and WISPs, Hamburg (Germany), 18
Jun 2018 - 22 Jun 2018},
keywords = {Weakly interacting slim particle (DE-H253) / Weakly
interacting slender particle (DE-H253) / Weakly interacting
sub-eV particle (DE-H253) / PATRAS 2018 (DE-H253) / WIMPs
(DE-H253) / Axions (DE-H253) / WISPs (DE-H253) / Weakly
interacting massive particles (DE-H253) / Hamburg (DE-H253)},
cin = {ALPS},
cid = {I:(DE-H253)ALPS-20130318},
pnm = {6211 - Extreme States of Matter: From Cold Ions to Hot
Plasmas (POF3-621)},
pid = {G:(DE-HGF)POF3-6211},
experiment = {EXP:(DE-H253)ALPS-20150101},
typ = {PUB:(DE-HGF)3 / PUB:(DE-HGF)26},
doi = {10.3204/PUBDB-2018-02580},
url = {https://bib-pubdb1.desy.de/record/407652},
}