NAGIOS: RODERIC FUNCIONANDO

Does the Sun shine by pp or CNO fusion reactions?

Repositori DSpace/Manakin

dc.contributor.author	Bahcall, John N.
dc.contributor.author	González García, Mª Concepción
dc.contributor.author	Peña Garay, Carlos
dc.date.accessioned	2014-11-03T12:45:56Z
dc.date.available	2014-11-03T12:45:56Z
dc.date.issued	2003
dc.identifier.citation	Bahcall, John N. González García, Mª Concepción Peña Garay, Carlos 2003 Does the Sun shine by pp or CNO fusion reactions? Physical Review Letters 90 13 131301
dc.identifier.uri	http://hdl.handle.net/10550/39546
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.
dc.language.iso	eng
dc.relation.ispartof	Physical Review Letters, 2003, vol. 90, num. 13, p. 131301
dc.subject	Física
dc.title	Does the Sun shine by pp or CNO fusion reactions?
dc.type	journal article	es_ES
dc.date.updated	2014-11-03T12:45:56Z
dc.identifier.doi	10.1103/PhysRevLett.90.131301
dc.identifier.idgrec	097454
dc.rights.accessRights	open access	es_ES