Core-Collapse Supernova neutrino detection prospects with the KM3NeT neutrino telescopes.

Core Collapse Supernovae (CCSN) are explosive phenomena that may occur at the end of the life of massive stars, releasing over 99% of the energy through neutrino emission with energies on the 10 MeV scale. While the explosion mechanism is not fully understood, neutrinos are believed to play an impor...

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Bibliographic Details
Main Authors: Colomer Molla Marta, Lincetto Massimiliano
Format: Article
Language:English
Published: EDP Sciences 2019-01-01
Series:EPJ Web of Conferences
Online Access:https://www.epj-conferences.org/articles/epjconf/pdf/2019/14/epjconf_ricap2019_01009.pdf