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Astrophysics > High Energy Astrophysical Phenomena

arXiv:2108.00176 (astro-ph)
[Submitted on 31 Jul 2021 (v1), last revised 12 Sep 2021 (this version, v3)]

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

Authors:Antonio Marinelli, Antonio Ambrosone, Walid Idrissi Ibnsalih, Gennaro Miele, Pasquale Migliozzi, Ofelia Pisanti, Ankur Sharma
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Abstract:Starburst galaxies (SBGs) and more in general starforming galaxies represent a class of galaxies with a high star formation rate (up to 100 solar masses/year). Despite their low luminosity, they can 19 be considered as guaranteed "factories" of high energy neutrinos, being "reservoirs" of accelerated 20 cosmic rays and hosting a high density target gas in the central region. In this contribution 21 we present a novel multimessenger study of these sources and the possibility of observing their 22 neutrino signals with the KM3NeT/ARCA telescope. The differential sensitivity for different SBG 23 scenarios is reported considering track-like neutrino events in the 100 GeV-100 PeV energy range.
Comments: Presented at the 9th Very Large Volume Neutrino Telescope Workshop (VLVnT 2021), Prepared for submission to JINST
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE); Cosmology and Nongalactic Astrophysics (astro-ph.CO); High Energy Physics - Experiment (hep-ex)
Cite as: arXiv:2108.00176 [astro-ph.HE]
  (or arXiv:2108.00176v3 [astro-ph.HE] for this version)
  https://doi.org/10.48550/arXiv.2108.00176
Related DOI: https://doi.org/10.1088/1748-0221/16/12/C12016

Submission history

From: Antonio Marinelli [view email]
[v1] Sat, 31 Jul 2021 08:21:20 UTC (678 KB)
[v2] Tue, 24 Aug 2021 11:28:32 UTC (678 KB)
[v3] Sun, 12 Sep 2021 15:32:44 UTC (584 KB)
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