Does the Sun Shine by pp or CNO Fusion Reactions?

We show that solar neutrino experiments set an upper limit of 7.8% (7.3% including the recent KamLAND measurements) to the fraction of energy that the Sun produces via the CNO fusion cycle, which is an order of magnitude improvement upon the previous limit. New experiments are required to detect CNO...

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Detalles Bibliográficos
Autores principales: Bahcall, John N., Gonzalez-Garcia, M.C., Pena-Garay, Carlos
Lenguaje:eng
Publicado: 2002
Materias:
Astrophysics and Astronomy
Acceso en línea:https://dx.doi.org/10.1103/PhysRevLett.90.131301
http://cds.cern.ch/record/597269
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author Bahcall, John N.
Gonzalez-Garcia, M.C.
Pena-Garay, Carlos
author_facet Bahcall, John N.
Gonzalez-Garcia, M.C.
Pena-Garay, Carlos
author_sort Bahcall, John N.
collection CERN
description We show that solar neutrino experiments set an upper limit of 7.8% (7.3% including the recent KamLAND measurements) to the fraction of energy that the Sun produces via the CNO fusion cycle, which is an order of magnitude improvement upon the previous limit. New experiments are required to detect CNO neutrinos corresponding to the 1.5% of the solar luminosity that the standard solar model predicts is generated by the CNO cycle.
id cern-597269
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2002
record_format invenio
spelling cern-5972692020-06-12T20:58:44Zdoi:10.1103/PhysRevLett.90.131301http://cds.cern.ch/record/597269engBahcall, John N.Gonzalez-Garcia, M.C.Pena-Garay, CarlosDoes the Sun Shine by pp or CNO Fusion Reactions?Astrophysics and AstronomyWe show that solar neutrino experiments set an upper limit of 7.8% (7.3% including the recent KamLAND measurements) to the fraction of energy that the Sun produces via the CNO fusion cycle, which is an order of magnitude improvement upon the previous limit. New experiments are required to detect CNO neutrinos corresponding to the 1.5% of the solar luminosity that the standard solar model predicts is generated by the CNO cycle.We show that solar neutrino experiments set an upper limit of 7.8% (7.3% including the recent KamLAND measurements) to the fraction of energy that the Sun produces via the CNO fusion cycle, which is an order of magnitude improvement upon the previous limit. New experiments are required to detect CNO neutrinos corresponding to the 1.5% of the solar luminosity that the standard solar model predicts is generated by the CNO cycle.astro-ph/0212331YITP-SB-77-02CERN-TH-2002-361CERN-TH-2002-361YITP-SB-2002-77oai:cds.cern.ch:5972692002-12-15
spellingShingle Astrophysics and Astronomy
Bahcall, John N.
Gonzalez-Garcia, M.C.
Pena-Garay, Carlos
Does the Sun Shine by pp or CNO Fusion Reactions?
title Does the Sun Shine by pp or CNO Fusion Reactions?
title_full Does the Sun Shine by pp or CNO Fusion Reactions?
title_fullStr Does the Sun Shine by pp or CNO Fusion Reactions?
title_full_unstemmed Does the Sun Shine by pp or CNO Fusion Reactions?
title_short Does the Sun Shine by pp or CNO Fusion Reactions?
title_sort does the sun shine by pp or cno fusion reactions?
topic Astrophysics and Astronomy
url https://dx.doi.org/10.1103/PhysRevLett.90.131301
http://cds.cern.ch/record/597269
work_keys_str_mv AT bahcalljohnn doesthesunshinebypporcnofusionreactions
AT gonzalezgarciamc doesthesunshinebypporcnofusionreactions
AT penagaraycarlos doesthesunshinebypporcnofusionreactions

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