KamLAND SENSITIVITY TO NEUTRINOS FROM PRE-SUPERNOVA STARS
In the late stages of nuclear burning for massive stars (M > 8 M[subscript ⊙]), the production of neutrino-antineutrino pairs through various processes becomes the dominant stellar cooling mechanism. As the star evolves, the energy of these neutrinos increases and in the days preceding the supern...
Main Author: | |
---|---|
Other Authors: | |
Format: | Article |
Language: | English |
Published: |
IOP Publishing,
2016-05-23T23:17:26Z.
|
Subjects: | |
Online Access: | Get fulltext |