Resonant amplification of ν oscillations in matter and solar-neutrino spectroscopy View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

1986-01

AUTHORS

S. P. Mikheyev, A. Yu. Smirnov

ABSTRACT

For small mixing angles θ the amplification of ν oscillations in matter has the resonance form (resonance in neutrino energy or matter density). In the Sun resonance effect results in nontrivial changing (suppression) of ν-flux for a wide range of neutrino parameters Δm2=(3·10−4÷10−8) (eV)2, sin22θ>10−4.

PAGES

17-26

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/bf02508049

DOI

http://dx.doi.org/10.1007/bf02508049

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1013292126


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