Speed-up of neutrino transformations in a supernova environment
arXiv:hep-ph/0503013 · doi:10.1103/PhysRevD.72.045003
Abstract
When the neutral current neutrino-neutrino interaction is treated completely, rather than as an interaction among angle-averaged distributions, or as a set of flavor-diagonal effective potentials, the result can be flavor mixing at a speed orders of magnitude faster than that one would anticipate from the measured neutrino oscillation parameters. It is possible that the energy spectra of the three active species of neutrinos emerging from a supernova are nearly identical.
8 pages, 4 figures
Cited by in corpus (210)
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