Axion emission and detection from a galactic supernova

Pierluca Carenza; Giampaolo Co; Tobias Fischer; Maurizio Giannotti; Alessandro Mirizzi; Thomas Rauscher

doi:10.3204/DESY-PROC-2018-03/Mirizzi_Alessandro

Axion emission and detection from a galactic supernova

Pierluca Carenza, Giampaolo Co, Tobias Fischer, Maurizio Giannotti, Alessandro Mirizzi, Thomas Rauscher

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

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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.

Original language	English
Title of host publication	Proceedings of the 14th Patras Workshop on Axions, WIMPs and WISPs
Editors	Todd Kozlowski
Publisher	Verlag Deutsches Elektronen-Synchrotron
Pages	57-60
Number of pages	4
ISBN (Electronic)	9783945931226
DOIs	https://doi.org/10.3204/DESY-PROC-2018-03/Mirizzi_Alessandro
Publication status	Published - 2019
Event	14th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2018 - Hamburg, Germany Duration: 18 Jun 2018 → 22 Jun 2018

Conference

Conference	14th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2018
Country/Territory	Germany
City	Hamburg
Period	18/06/18 → 22/06/18

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10.3204/DESY-PROC-2018-03/Mirizzi_AlessandroLicence: CC BY

PATRAS_2018
© 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.
Final published version, 324 KBLicence: CC BY

Cite this

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title = "Axion emission and detection from a galactic supernova",

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.",

author = "Pierluca Carenza and Giampaolo Co and Tobias Fischer and Maurizio Giannotti and Alessandro Mirizzi and Thomas Rauscher",

note = "{\textcopyright} 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.; 14th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2018 ; Conference date: 18-06-2018 Through 22-06-2018",

year = "2019",

doi = "10.3204/DESY-PROC-2018-03/Mirizzi\_Alessandro",

language = "English",

pages = "57--60",

editor = "Todd Kozlowski",

booktitle = "Proceedings of the 14th Patras Workshop on Axions, WIMPs and WISPs",

publisher = "Verlag Deutsches Elektronen-Synchrotron",

}

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

TY - GEN

T1 - Axion emission and detection from a galactic supernova

AU - Carenza, Pierluca

AU - Co, Giampaolo

AU - Fischer, Tobias

AU - Giannotti, Maurizio

AU - Mirizzi, Alessandro

AU - Rauscher, Thomas

N1 - © 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.

PY - 2019

Y1 - 2019

N2 - 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.

AB - 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.

UR - https://www.scopus.com/pages/publications/85085954230

U2 - 10.3204/DESY-PROC-2018-03/Mirizzi_Alessandro

DO - 10.3204/DESY-PROC-2018-03/Mirizzi_Alessandro

M3 - Conference contribution

AN - SCOPUS:85085954230

SP - 57

EP - 60

BT - Proceedings of the 14th Patras Workshop on Axions, WIMPs and WISPs

A2 - Kozlowski, Todd

PB - Verlag Deutsches Elektronen-Synchrotron

T2 - 14th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2018

Y2 - 18 June 2018 through 22 June 2018

ER -

Axion emission and detection from a galactic supernova

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