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dc.contributor.authorBahcall, John
dc.contributor.authorGonzález García, Ma. Concepcióncat
dc.contributor.authorPeña Garay, Carloscat
dc.description.abstractWe 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.eng
dc.format.extentp. 4-
dc.publisherAmerican Physical Societyeng
dc.relation.isformatofReproducció digital del document proporcionada per PROLA i
dc.relation.ispartofPhysical Review Letters, 2003, vol. 90, núm. 13, p. 131301-1-131301-4cat
dc.rights(c) American Physical Society, 2003eng
dc.sourceArticles publicats en revistes (Física Quàntica i Astrofísica)-
dc.subject.classificationAstrofísica nuclearcat
dc.subject.classificationReaccions nuclearscat
dc.subject.otherNuclear astrophysicseng
dc.subject.otherNuclear reactionseng
dc.titleDoes the sun shine by p p or CNO fusion reactions?eng
Appears in Collections:Articles publicats en revistes (Física Quàntica i Astrofísica)

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