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KM3NeT/ARCA expectations in view of a novel multimessenger study of starburst galaxies

  • A. Marinelli
  • , A. Ambrosone
  • , W.I. Ibnsalih
  • , G. Miele
  • , P. Migliozzi
  • , O. Pisanti
  • , A. Sharma
  • , M. Ageron
  • , S. Aiello
  • , A. Albert
  • , M. Alshamsi
  • , Garre Alves
  • , Z. Aly
  • , A. Ambrosone
  • , F. Ameli
  • , M. Andre
  • , G. Androulakis
  • , M. Anghinolfi
  • , M. Anguita
  • , G. Anton
  • M. Ardid, S. Ardid, W. Assal, J. Aublin, C. Bagatelas, B. Baret, Du Basegmez, M. Bendahman, F. Benfenati, E. Berbee, Den Van, V. Bertin, S. Beurthey, Beveren Van, S. Biagi, M. Billault, M. Bissinger, M. Boettcher, Cabo Bou, J. Boumaaza, M. Bouta, C. Boutonnet, G. Bouvet, M. Bouwhuis, C. Bozza, H. Branzaş, R. Bruijn, J. Brunner, R. Bruno, E. Buis, R. Buompane, M. Filipovic, al et al

Research output: Contribution to journalArticlepeer-review

3 Citations (Scopus)

Abstract

Starburst galaxies (SBGs) and more in general star-forming galaxies represent a class of galaxies with a high star formation rate (up to 100Mo˙/year). Despite their low luminosity, they can be considered as guaranteed "factories"of high energy neutrinos, being "reservoirs"of accelerated cosmic rays and hosting a high density target gas in the central region. In this contribution we present a novel multimessenger study of these sources and the possibility of observing their neutrino signals with the KM3NeT/ARCA telescope. The differential sensitivity for different SBG scenarios is reported considering track-like neutrino events in the 100 GeV-100 PeV energy range.

Original languageEnglish
Article numberC12016
Number of pages9
JournalJournal of Instrumentation
Volume16
Issue number12
DOIs
Publication statusPublished - 1 Dec 2021

Bibliographical note

Publisher Copyright:
© 2021 IOP Publishing Ltd and Sissa Medialab.

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