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2015

Self-induced flavor conversion of supernova neutrinos on small scales

Chakraborty, Sovan, Hansen, Rasmus Sloth, Izaguirre, Ignacio et al.

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Self-induced flavor conversion of supernova (SN) neutrinos is a generic feature of neutrino-neutrino dispersion.

The corresponding run-away modes in flavor space can spontaneously break the original symmetries of the neutrino flux and in particular can spontaneously produce small-scale features as shown in recent schematic studies.
However, the unavoidable "multi-angle matter effect" shifts these small-scale instabilities into regions of matter and neutrino density which are not encountered on the way out from a SN.
The traditional modes which are uniform on the largest scales are most prone for instabilities and thus provide the most sensitive test for the appearance of self-induced flavor conversion.

Self-induced flavor conversion of supernova neutrinos on small scales · Around

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