2005
DOI: 10.1103/physrevd.72.045003
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Speed-up of neutrino transformations in a supernova environment

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.Comment: 8 pages, 4 figure

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Cited by 277 publications
(265 citation statements)
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“…With hindsight this is probably the same "speed-up effect" discussed in Ref. [11]. However, the fast speed κ = √ 2ωµ is not introduced by the multi-angle effect as is perhaps suggested in Ref.…”
Section: Discussionmentioning
confidence: 82%
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“…With hindsight this is probably the same "speed-up effect" discussed in Ref. [11]. However, the fast speed κ = √ 2ωµ is not introduced by the multi-angle effect as is perhaps suggested in Ref.…”
Section: Discussionmentioning
confidence: 82%
“…However, the fast speed κ = √ 2ωµ is not introduced by the multi-angle effect as is perhaps suggested in Ref. [11]. Rather, κ is the bipolar oscillation frequency that is inherent even in the isotropic system.…”
Section: Discussionmentioning
confidence: 99%
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“…The effective Hamiltonian describing the propagation of neutrinos in a background of electrons is given by [29] …”
Section: Three Neutrino Flavorsmentioning
confidence: 99%