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...
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 |
Similar Items
-
Core-Collapse Supernova neutrino detection with KM3NeT
by: Molla Marta Colomer, et al.
Published: (2019-01-01) -
Neutrinos from core-collapse supernovae at KM3NeT
by: Bendahman Meriem
Published: (2023-01-01) -
The KM3NeT potential for the next core-collapse supernova observation with neutrinos
by: S. Aiello, et al.
Published: (2021-05-01) -
Implementation and first results of the KM3NeT real-time core-collapse supernova neutrino search
by: S. Aiello, et al.
Published: (2022-04-01) -
Combining neutrino experimental light-curves for pointing to the next galactic core-collapse supernova
by: A. Coleiro, et al.
Published: (2020-09-01)