Nonlinear neutrino oscillations in the expanding Universe

dc.contributor.authorKostelecký, V.A.
dc.contributor.authorSamuel, S.
dc.date.accessioned2014-09-05T16:53:44Z
dc.date.available2014-09-05T16:53:44Z
dc.date.issued1994
dc.description.abstractWe derive the equations that govern neutrino and antineutrino behavior in the early Universe. Results are presented from numerical simulations incorporating nonlinear effects of the neutrino-antineutrino background as well as the leading CP-symmetric and CP-asymmetric terms arising from the interactions with electrons and positrons. A broad spectrum of neutrino and antineutrino behavior is observed, ranging from vacuumlike to smooth. Oscillations exhibiting self-maintained coherence also appear. We identify a variety of neutrino properties arising as a consequence of the nonlinear neutrino self-interactions. The nonlinear effects tend to suppress any CP asymmetry relative to the linear case. An analytical approximation scheme reproducing bulk neutrino behavior is described. We discuss some physical implications of our results.
dc.identifier.citationKostelecký, V. A., & Samuel, S. (1994). Nonlinear neutrino oscillations in the expanding Universe. Physical Review D, 49(4), 1740-1757. http://dx.doi.org/10.1103/PhysRevD.49.1740
dc.identifier.urihttps://hdl.handle.net/2022/18663
dc.language.isoen_US
dc.publisherAmerican Physical Society
dc.relation.isversionofhttps://doi.org/10.1103/PhysRevD.49.1740
dc.rights© 1994 American Physical Society.
dc.titleNonlinear neutrino oscillations in the expanding Universe
dc.typeArticle

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