Ponente
Antonio Marinelli
(INFN Naples)
Descripción
Starburst galaxies (SBGs) and more in general starforming galaxies represent a class of galaxies with a high star formation rate (up to 100 Mo/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 and discovery potential for different SBG scenarios are reported considering track-like events in the 100 GeV-100 PeV energy range.
| Affiliation | INFN Naples |
|---|
Autor primario
Antonio Marinelli
(INFN Naples)
Coautores
Sr.
Antonio Ambrosone
(Università di Napoli "Federico II")
Sr.
Walid Idrissi ibnsalih
(Università della Campania)
Dr.
Ankur Sharma
(University of Uppsala)
