Neutrino helioseismology

The observed deficit of $\rm ^8B$ solar neutrinos may call for an improved standard model of the sun or an expanded standard model of particle physics ({\it e.g.,} with neutrino masses and mixing). In the former case, contemporary fluid motions and thermal fluctuations in the sun's core may mod...

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Detalles Bibliográficos
Autores principales: De Rujula, A., Glashow, S.L.
Lenguaje:eng
Publicado: 1992
Materias:
Other Fields of Physics
Acceso en línea:http://cds.cern.ch/record/240077
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author De Rujula, A.
Glashow, S.L.
author_facet De Rujula, A.
Glashow, S.L.
author_sort De Rujula, A.
collection CERN
description The observed deficit of $\rm ^8B$ solar neutrinos may call for an improved standard model of the sun or an expanded standard model of particle physics ({\it e.g.,} with neutrino masses and mixing). In the former case, contemporary fluid motions and thermal fluctuations in the sun's core may modify nuclear reaction rates and restore agreement. To test this notion, we propose a search for short--term variations of the solar neutrino flux.
id cern-240077
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 1992
record_format invenio
spelling cern-2400772023-03-14T19:28:07Zhttp://cds.cern.ch/record/240077engDe Rujula, A.Glashow, S.L.Neutrino helioseismologyOther Fields of PhysicsThe observed deficit of $\rm ^8B$ solar neutrinos may call for an improved standard model of the sun or an expanded standard model of particle physics ({\it e.g.,} with neutrino masses and mixing). In the former case, contemporary fluid motions and thermal fluctuations in the sun's core may modify nuclear reaction rates and restore agreement. To test this notion, we propose a search for short--term variations of the solar neutrino flux.The observed deficit of $\rm ~8B$ solar neutrinos may call for an improved standard model of the sun or an expanded standard model of particle physics ({\it e.g.,} with neutrino masses and mixing). In the former case, contemporary fluid motions and thermal fluctuations in the sun's core may modify nuclear reaction rates and restore agreement. To test this notion, we propose a search for short--term variations of the solar neutrino flux.hep-ph/9208223HUTP-92-A038CERN-TH-6608-92CERN-TH-6608-92HUTP-92-A-038oai:cds.cern.ch:2400771992
spellingShingle Other Fields of Physics
De Rujula, A.
Glashow, S.L.
Neutrino helioseismology
title Neutrino helioseismology
title_full Neutrino helioseismology
title_fullStr Neutrino helioseismology
title_full_unstemmed Neutrino helioseismology
title_short Neutrino helioseismology
title_sort neutrino helioseismology
topic Other Fields of Physics
url http://cds.cern.ch/record/240077
work_keys_str_mv AT derujulaa neutrinohelioseismology
AT glashowsl neutrinohelioseismology

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