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...
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| Format: | Article |
| Language: | English |
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IOP Publishing,
2016-05-23T23:17:26Z.
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| Online Access: | Get fulltext |