Neutrino self-interactions inside neutrino-cooled accretion disks are argued to push flavors toward equipartition, reducing the neutrino-antineutrino annihilation energy deposition around black holes by a factor up to about five.
Neutrino oscillations in the early universe with an inverted neutrino mass hierarchy
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Neutrino oscillations in a neutrino-dominated accretion disk around a Kerr BH
Neutrino self-interactions inside neutrino-cooled accretion disks are argued to push flavors toward equipartition, reducing the neutrino-antineutrino annihilation energy deposition around black holes by a factor up to about five.