Neutrino condensates at center of galaxies as background for the MSW mechanism
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The possibility is explored that neutrino condensates, possible candidates for the explanation of very massive objects in galactic centers, could act as background for the Mikheyev-Smirnov-Wolfeinstein mechanism responsible of neutrino oscillations. Assuming a simple neutrino star model with constant density, the lower limit of the mass squared difference of neutrino oscillations is inferred. Consequences on neutrino asymmetry are discussed.
5 pages, to appear in Mod. Phys. Lett. A
5 pages, to appear in Mod. Phys. Lett. A