Bimodal coherence in dense self-interacting neutrino gases
- 15 May 1996
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review D
- Vol. 53 (10) , 5382-5393
- https://doi.org/10.1103/physrevd.53.5382
Abstract
Analytical solutions are obtained to the nonlinear equations describing neutrino oscillations when explicit neutrino-antineutrino asymmetries are present. Such a system occurs in the early Universe if neutrinos have a nonzero chemical potential. Solutions to the equations lead to a new type of coherent behavior governed by two modes. These bimodal solutions provide new insight into dense neutrino gases and into neutrino oscillations in the early Universe, thereby allowing one to surmise the flavor behavior of neutrinos with a nonzero chemical potential. © 1996 The American Physical Society.Keywords
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This publication has 18 references indexed in Scilit:
- Neutrino-neutrino scattering and matter-enhanced neutrino flavor transformation in supernovaePhysical Review D, 1995
- Nonlinear neutrino oscillations in the expanding UniversePhysical Review D, 1994
- Neutrino oscillations in the early universe with an inverted neutrino-mass hierarchyPhysics Letters B, 1993
- Neutrino oscillations in the early universePhysics Letters B, 1993
- General kinetic description of relativistic mixed neutrinosNuclear Physics B, 1993
- Neutrino oscillations in dense neutrino gasesPhysical Review D, 1993
- Neutrino oscillations and the leptonic charge of the universeThe Astrophysical Journal, 1991
- Neutrino dispersion at finite temperature and densityNuclear Physics B, 1988
- Treatment of neutrino oscillations in a thermal environmentPhysical Review D, 1987
- Implications of the mikheyev-smirnov-wolfenstein (MSW) mechanism of amplification of neutrino oscillations in matterNuclear Physics B, 1987