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arXiv:0807.0659·v2·Astrophysics

Role of dense matter in collective supernova neutrino transformations

A. Esteban-Pretel🇪🇸 · A. Mirizzi🇩🇪 · S. Pastor🇪🇸 · R. Tomas🇩🇪 · G.G. Raffelt🇩🇪 · P.D. Serpico🇺🇸 · G. Sigl🇩🇪

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Abstract

For neutrinos streaming from a supernova (SN) core, dense matter suppresses self-induced flavor transformations if the electron density n_e significantly exceeds the neutrino density n_nu in the conversion region. If n_e is comparable to n_nu one finds multi-angle decoherence, whereas the standard self-induced transformation behavior requires that in the transformation region n_nu is safely above n_e. This condition need not be satisfied in the early phase after supernova core bounce. Our new multi-angle effect is a subtle consequence of neutrinos traveling on different trajectories when streaming from a source that is not point-like.

Comments: 7 pages, 2 figures. Published version

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