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: | en_US |
| Published: |
IOP Publishing
2016
|
| Online Access: | http://hdl.handle.net/1721.1/102640 https://orcid.org/0000-0002-9970-108X |