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Black hole accretion disks can form through the collapse of rotating massivestars. These disks produce large numbers of neutrinos and antineutrinos ofelectron flavor that can influence energetics and nucleosynthesis. Neutrinosare produced in sufficient numbers that, after they are emitted, they canundergo flavor transformation facilitated by the neutrino self interaction. Weshow that some of the neutrino flavor transformation phenomenology foraccretion disks is similar to that of the supernova case, but also, we find thedisk geometry lends itself to different transformation behaviors. Thesetransformations strongly influence the nucleosynthetic outcome of disk winds.

Neutrino oscillations above black hole accretion disks: disks with electron-flavor emission