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001     453704
005     20211222091554.0
024 7 _ |a 10.3204/PUBDB-2018-02580
|2 doi
024 7 _ |a Carenza:2018jjc
|2 INSPIRETeX
024 7 _ |a inspire:1686784
|2 inspire
024 7 _ |a arXiv:1808.04101
|2 arXiv
024 7 _ |a 10.3204/PUBDB-2021-00114
|2 datacite_doi
024 7 _ |a altmetric:46482272
|2 altmetric
037 _ _ |a PUBDB-2021-00114
041 _ _ |a English
088 _ _ |a arXiv:1808.04101
|2 arXiv
088 _ _ |a DESY-PROC-2018-03
|2 DESY
100 1 _ |a Carenza, Pierluca
|0 P.Carenza.1
|b 0
245 _ _ |a Axion emission and detection from a Galactic supernova
260 _ _ |c 2019
336 7 _ |a Preprint
|b preprint
|m preprint
|0 PUB:(DE-HGF)25
|s 1610102311_6416
|2 PUB:(DE-HGF)
336 7 _ |a WORKING_PAPER
|2 ORCID
336 7 _ |a Electronic Article
|0 28
|2 EndNote
336 7 _ |a preprint
|2 DRIVER
336 7 _ |a ARTICLE
|2 BibTeX
336 7 _ |a Output Types/Working Paper
|2 DataCite
500 _ _ |a 4 pages. Contributed to the 14th Patras Workshop on Axions, WIMPs and WISPs, DESY in Hamburg, June 18 to 22, 2018
520 _ _ |a 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.
536 _ _ |a 6211 - Extreme States of Matter: From Cold Ions to Hot Plasmas (POF3-621)
|0 G:(DE-HGF)POF3-6211
|c POF3-621
|f POF III
|x 0
588 _ _ |a Dataset connected to DataCite, INSPIRE
650 _ 7 |a axion: absorption
|2 INSPIRE
650 _ 7 |a Cherenkov counter: water
|2 INSPIRE
650 _ 7 |a supernova
|2 INSPIRE
650 _ 7 |a galaxy
|2 INSPIRE
650 _ 7 |a oxygen
|2 INSPIRE
650 _ 7 |a KAMIOKANDE
|2 INSPIRE
693 _ _ |0 EXP:(DE-H253)ALPS-20150101
|5 EXP:(DE-H253)ALPS-20150101
|e Any Light Particle Search
|x 0
700 1 _ |a Co', Giampaolo
|0 G.Co.1
|b 1
700 1 _ |a Fischer, Tobias
|b 2
700 1 _ |a Giannotti, Maurizio
|b 3
700 1 _ |a Mirizzi, Alessandro
|0 P:(DE-H253)PIP1011532
|b 4
|e Corresponding author
700 1 _ |a Rauscher, Thomas
|0 T.Rauscher.2
|b 5
773 _ _ |a 10.3204/PUBDB-2018-02580
856 4 _ |y OpenAccess
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910 1 _ |a External Institute
|0 I:(DE-HGF)0
|k Extern
|b 4
|6 P:(DE-H253)PIP1011532
913 1 _ |a DE-HGF
|b Forschungsbereich Materie
|l Von Materie zu Materialien und Leben
|1 G:(DE-HGF)POF3-620
|0 G:(DE-HGF)POF3-621
|3 G:(DE-HGF)POF3
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|v In-house research on the structure, dynamics and function of matter
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915 _ _ |a OpenAccess
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915 _ _ |a Published
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920 1 _ |0 I:(DE-H253)ALPS-20130318
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980 _ _ |a preprint
980 _ _ |a VDB
980 _ _ |a UNRESTRICTED
980 _ _ |a I:(DE-H253)ALPS-20130318
980 1 _ |a FullTexts

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