University of Hertfordshire

By the same authors

Axion emission and detection from a galactic supernova

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Documents

  • PATRAS_2018

    Final published version, 324 KB, PDF document

  • Pierluca Carenza
  • Giampaolo Co
  • Tobias Fischer
  • Maurizio Giannotti
  • Alessandro Mirizzi
  • Thomas Rauscher
View graph of relations
Original languageEnglish
Title of host publicationProceedings of the 14th Patras Workshop on Axions, WIMPs and WISPs
EditorsTodd Kozlowski
PublisherVerlag Deutsches Elektronen-Synchrotron
Pages57-60
Number of pages4
ISBN (Electronic)9783945931226
DOIs
Publication statusPublished - 2019
Event14th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2018 - Hamburg, Germany
Duration: 18 Jun 201822 Jun 2018

Conference

Conference14th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2018
CountryGermany
CityHamburg
Period18/06/1822/06/18

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.

Notes

© 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.

ID: 22061111