Solar Mikheyev-Smirnov-Wolfenstein Effect with Three Generations of Neutrinos

Under the assumption that the density variation of the electrons can beapproximated by an exponential function, the solar Mikheyev-Smirnov-Wolfensteineffect is treated for three generations of neutrinos. The generalizedhypergeometric functions that result from the exact solution of this problemare s...

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Detalles Bibliográficos
Autores principales: Osland, Per, Wu, Tai Tsun
Lenguaje:eng
Publicado: 1999
Materias:
Particle Physics - Phenomenology
Acceso en línea:https://dx.doi.org/10.1103/PhysRevD.62.013008
http://cds.cern.ch/record/428345
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author Osland, Per
Wu, Tai Tsun
author_facet Osland, Per
Wu, Tai Tsun
author_sort Osland, Per
collection CERN
description Under the assumption that the density variation of the electrons can beapproximated by an exponential function, the solar Mikheyev-Smirnov-Wolfensteineffect is treated for three generations of neutrinos. The generalizedhypergeometric functions that result from the exact solution of this problemare studied in detail, and a method for their numerical evaluation ispresented. This analysis plays a central role in the determination of neutrinomasses, not only the differences of their squares, under the assumption ofuniversal quark-lepton mixing.
id cern-428345
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 1999
record_format invenio
spelling cern-4283452023-03-14T18:59:51Zdoi:10.1103/PhysRevD.62.013008http://cds.cern.ch/record/428345engOsland, PerWu, Tai TsunSolar Mikheyev-Smirnov-Wolfenstein Effect with Three Generations of NeutrinosParticle Physics - PhenomenologyUnder the assumption that the density variation of the electrons can beapproximated by an exponential function, the solar Mikheyev-Smirnov-Wolfensteineffect is treated for three generations of neutrinos. The generalizedhypergeometric functions that result from the exact solution of this problemare studied in detail, and a method for their numerical evaluation ispresented. This analysis plays a central role in the determination of neutrinomasses, not only the differences of their squares, under the assumption ofuniversal quark-lepton mixing.Under the assumption that the density variation of the electrons can be approximated by an exponential function, the solar Mikheyev-Smirnov-Wolfenstein effect is treated for three generations of neutrinos. The generalized hypergeometric functions that result from the exact solution of this problem are studied in detail, and a method for their numerical evaluation is presented. This analysis plays a central role in the determination of neutrino masses, not only the differences of their squares, under the assumption of universal quark-lepton mixing.hep-ph/9912540CERN-TH-99-286CERN-TH-99-286oai:cds.cern.ch:4283451999-12-29
spellingShingle Particle Physics - Phenomenology
Osland, Per
Wu, Tai Tsun
Solar Mikheyev-Smirnov-Wolfenstein Effect with Three Generations of Neutrinos
title Solar Mikheyev-Smirnov-Wolfenstein Effect with Three Generations of Neutrinos
title_full Solar Mikheyev-Smirnov-Wolfenstein Effect with Three Generations of Neutrinos
title_fullStr Solar Mikheyev-Smirnov-Wolfenstein Effect with Three Generations of Neutrinos
title_full_unstemmed Solar Mikheyev-Smirnov-Wolfenstein Effect with Three Generations of Neutrinos
title_short Solar Mikheyev-Smirnov-Wolfenstein Effect with Three Generations of Neutrinos
title_sort solar mikheyev-smirnov-wolfenstein effect with three generations of neutrinos
topic Particle Physics - Phenomenology
url https://dx.doi.org/10.1103/PhysRevD.62.013008
http://cds.cern.ch/record/428345
work_keys_str_mv AT oslandper solarmikheyevsmirnovwolfensteineffectwiththreegenerationsofneutrinos
AT wutaitsun solarmikheyevsmirnovwolfensteineffectwiththreegenerationsofneutrinos

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