| dc.contributor.author | Carenza, Pierluca | |
| dc.contributor.author | Co, Giampaolo | |
| dc.contributor.author | Fischer, Tobias | |
| dc.contributor.author | Giannotti, Maurizio | |
| dc.contributor.author | Mirizzi, Alessandro | |
| dc.contributor.author | Rauscher, Thomas | |
| dc.contributor.editor | Kozlowski, Todd | |
| dc.date.accessioned | 2020-06-21T00:18:18Z | |
| dc.date.available | 2020-06-21T00:18:18Z | |
| dc.date.issued | 2019 | |
| dc.identifier.citation | Carenza , P , Co , G , Fischer , T , Giannotti , M , Mirizzi , A & Rauscher , T 2019 , Axion emission and detection from a galactic supernova . in T Kozlowski (ed.) , Proceedings of the 14th Patras Workshop on Axions, WIMPs and WISPs . Verlag Deutsches Elektronen-Synchrotron , pp. 57-60 , 14th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2018 , Hamburg , Germany , 18/06/18 . https://doi.org/10.3204/DESY-PROC-2018-03/Mirizzi_Alessandro | |
| dc.identifier.citation | conference | |
| dc.identifier.isbn | 9783945931226 | |
| dc.identifier.other | PURE: 22061111 | |
| dc.identifier.other | PURE UUID: 153fb2f5-8ed6-4466-b0fd-f324b34de61c | |
| dc.identifier.other | Scopus: 85085954230 | |
| dc.identifier.uri | http://hdl.handle.net/2299/22901 | |
| dc.description | © 2019 The Author(s). The copyright is governed by the Creative Commons agreement under CC BY 4.0 (https://creativecommons.org/licenses/by/4.0/), which allows to copy, distribute, display and perform the work and make derivative works and remixes based on it only if they give the author or licensor the credits (attribution) in the manner specified by these. | |
| dc.description.abstract | A Galactic supernova (SN) axion signal would be detected in a future neutrino Mtonclass 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. | en |
| dc.format.extent | 4 | |
| dc.language.iso | eng | |
| dc.publisher | Verlag Deutsches Elektronen-Synchrotron | |
| dc.relation.ispartof | Proceedings of the 14th Patras Workshop on Axions, WIMPs and WISPs | |
| dc.rights | Open | |
| dc.subject | Nuclear and High Energy Physics | |
| dc.subject | Atomic and Molecular Physics, and Optics | |
| dc.title | Axion emission and detection from a galactic supernova | en |
| dc.contributor.institution | Centre for Astrophysics Research | |
| dc.identifier.url | http://www.scopus.com/inward/record.url?scp=85085954230&partnerID=8YFLogxK | |
| dc.description.versiontype | Final Published version | |
| dcterms.dateAccepted | 2019 | |
| rioxxterms.version | VoR | |
| rioxxterms.versionofrecord | https://doi.org/10.3204/DESY-PROC-2018-03/Mirizzi_Alessandro | |
| rioxxterms.licenseref.uri | http://creativecommons.org/licenses/by/4.0/ | |
| rioxxterms.type | Other | |
| herts.preservation.rarelyaccessed | true | |
| herts.rights.accesstype | Open | |
