Does the sun shine by p p or CNO fusion reactions?

Bahcall, John N.; González García, Ma. Concepción; Peña Garay, Carlos

Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/12849

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DC Field	Value	Language
dc.contributor.author	Bahcall, John N.	cat
dc.contributor.author	González García, Ma. Concepción	cat
dc.contributor.author	Peña Garay, Carlos	cat
dc.date.accessioned	2010-06-11T11:07:16Z	-
dc.date.available	2010-06-11T11:07:16Z	-
dc.date.issued	2003	-
dc.identifier.issn	0031-9007	-
dc.identifier.uri	http://hdl.handle.net/2445/12849	-
dc.description.abstract	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.	eng
dc.format.extent	p. 4	-
dc.format.mimetype	application/pdf	-
dc.language.iso	eng	eng
dc.publisher	American Physical Society	eng
dc.relation.isformatof	Reproducció digital del document proporcionada per PROLA i http://dx.doi.org/10.1103/PhysRevLett.90.131301	cat
dc.relation.ispartof	Physical Review Letters, 2003, vol. 90, núm. 13, p. 131301-1-131301-4	cat
dc.relation.uri	http://dx.doi.org/10.1103/PhysRevLett.90.131301	-
dc.rights	(c) American Physical Society, 2003	eng
dc.source	Articles publicats en revistes (Física Quàntica i Astrofísica)	-
dc.subject.classification	Astrofísica nuclear	cat
dc.subject.classification	Reaccions nuclears	cat
dc.subject.other	Nuclear astrophysics	eng
dc.subject.other	Nuclear reactions	eng
dc.title	Does the sun shine by p p or CNO fusion reactions?	eng
dc.type	info:eu-repo/semantics/article	eng
dc.type	info:eu-repo/semantics/publishedVersion	-
dc.identifier.idgrec	551565	-
dc.rights.accessRights	info:eu-repo/semantics/openAccess	-
Appears in Collections:	Articles publicats en revistes (Física Quàntica i Astrofísica)

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