Non standard analysis of the solar neutrino anomaly

Continuing previous work, a model independent analysis of the solar neutrino anomaly is performed in terms of neutrino oscillations, allowing a comparison with the predictions of the Standard Solar Model. SMA and LMA solutions emerge also in this case, although somewhat different from the standard o...

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Detalles Bibliográficos
Autores principales: Barbieri, Riccardo, Strumia, Alessandro
Lenguaje:eng
Publicado: 2000
Materias:
Particle Physics - Phenomenology
Acceso en línea:https://dx.doi.org/10.1088/1126-6708/2000/12/016
http://cds.cern.ch/record/481670
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author Barbieri, Riccardo
Strumia, Alessandro
author_facet Barbieri, Riccardo
Strumia, Alessandro
author_sort Barbieri, Riccardo
collection CERN
description Continuing previous work, a model independent analysis of the solar neutrino anomaly is performed in terms of neutrino oscillations, allowing a comparison with the predictions of the Standard Solar Model. SMA and LMA solutions emerge also in this case, although somewhat different from the standard ones. The significance of the NC/CC double ratio measurable in SNO is illustrated in this context.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2000
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spelling cern-4816702023-03-14T17:59:20Zdoi:10.1088/1126-6708/2000/12/016http://cds.cern.ch/record/481670engBarbieri, RiccardoStrumia, AlessandroNon standard analysis of the solar neutrino anomalyParticle Physics - PhenomenologyContinuing previous work, a model independent analysis of the solar neutrino anomaly is performed in terms of neutrino oscillations, allowing a comparison with the predictions of the Standard Solar Model. SMA and LMA solutions emerge also in this case, although somewhat different from the standard ones. The significance of the NC/CC double ratio measurable in SNO is illustrated in this context.Continuing previous work, a model independent analysis of the solar neutrino anomaly is performed in terms of neutrino oscillations, allowing a comparison with the predictions of the Standard Solar Model. SMA and LMA solutions emerge also in this case, although somewhat different from the standard ones. The significance of the NC/CC double ratio measurable in SNO is illustrated in this context.hep-ph/0011307CERN-TH-2000-345IFUP-TH-2000-43SNS-PH-00-17CERN-TH-2000-345IFUP-TH-2000-43SNS-PH-2000-17oai:cds.cern.ch:4816702000-11-24
spellingShingle Particle Physics - Phenomenology
Barbieri, Riccardo
Strumia, Alessandro
Non standard analysis of the solar neutrino anomaly
title Non standard analysis of the solar neutrino anomaly
title_full Non standard analysis of the solar neutrino anomaly
title_fullStr Non standard analysis of the solar neutrino anomaly
title_full_unstemmed Non standard analysis of the solar neutrino anomaly
title_short Non standard analysis of the solar neutrino anomaly
title_sort non standard analysis of the solar neutrino anomaly
topic Particle Physics - Phenomenology
url https://dx.doi.org/10.1088/1126-6708/2000/12/016
http://cds.cern.ch/record/481670
work_keys_str_mv AT barbieririccardo nonstandardanalysisofthesolarneutrinoanomaly
AT strumiaalessandro nonstandardanalysisofthesolarneutrinoanomaly

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