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Cornering Solar radiative-zone fluctuations with KamLAND and SNO salt

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Cornering Solar radiative-zone fluctuations with KamLAND and SNO salt

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dc.contributor.author	Burgess, C. P.
dc.contributor.author	Dzhalilov, N. S.
dc.contributor.author	Maltoni, Michele
dc.contributor.author	Rashba, Timur I.
dc.contributor.author	Semikoz, Victor B.
dc.contributor.author	Tórtola Baixauli, María Amparo
dc.contributor.author	Furtado Valle, José Wagner
dc.date.accessioned	2015-10-19T10:20:33Z
dc.date.available	2015-10-19T10:20:33Z
dc.date.issued	2004
dc.identifier.citation	Burgess, C. P. Dzhalilov, N. S. Maltoni, Michele Rashba, Timur I. Semikoz, Victor B. Tórtola Baixauli, María Amparo Furtado Valle, José Wagner 2004 Cornering Solar radiative-zone fluctuations with KamLAND and SNO salt Journal of Cosmological and Astroparticle Physics 2004 01 007-1 007-10
dc.identifier.uri	http://hdl.handle.net/10550/47766
dc.description.abstract	We update the best constraints on fluctuations in the solar medium deep within the solar Radiative Zone to include the new SNO-salt solar neutrino measurements. We find that these new measurements are now sufficiently precise that neutrino oscillation parameters can be inferred independently of any assumptions about fluctuation properties. Constraints on fluctuations are also improved, with amplitudes of 5% now excluded at the 99% confidence level for correlation lengths in the range of several hundred km. Because they are sensitive to correlation lengths which are so short, these solar neutrino results are complementary to constraints coming from helioseismology.
dc.language.iso	eng
dc.relation.ispartof	Journal of Cosmological and Astroparticle Physics, 2004, vol. 2004, num. 01, p. 007-1-007-10
dc.subject	Física
dc.title	Cornering Solar radiative-zone fluctuations with KamLAND and SNO salt
dc.type	journal article	es_ES
dc.date.updated	2015-10-19T10:20:34Z
dc.identifier.doi	10.1088/1475-7516/2004/01/007
dc.identifier.idgrec	018333
dc.rights.accessRights	open access	es_ES