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: | Winslow, Lindley (Contributor) |
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Other Authors: | Massachusetts Institute of Technology. Department of Physics (Contributor) |
Format: | Article |
Language: | English |
Published: |
IOP Publishing,
2016-05-23T23:17:26Z.
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Subjects: | |
Online Access: | Get fulltext |
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