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Enhanced solar antineutrino flux in random magnetic fields

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Enhanced solar antineutrino flux in random magnetic fields

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dc.contributor.author Miranda, O.G.
dc.contributor.author Rashba, Timur I.
dc.contributor.author Rez, A. I.
dc.contributor.author Furtado Valle, José Wagner
dc.date.accessioned 2015-09-30T12:12:52Z
dc.date.available 2015-09-30T12:12:52Z
dc.date.issued 2004
dc.identifier.citation Miranda, O.G. Rashba, Timur I. Rez, A. I. Furtado Valle, José Wagner 2004 Enhanced solar antineutrino flux in random magnetic fields Physical Review D 70 11 113002 113013
dc.identifier.uri http://hdl.handle.net/10550/47502
dc.description.abstract We discuss the impact of the recent KamLAND constraint on the solar anti-neutrino flux on the analysis of solar neutrino data in the presence of Majorana neutrino transition magnetic moments and solar magnetic fields. We consider different stationary solar magnetic field models, both regular and random, highlighting the strong enhancement in the anti-neutrino production rates that characterize turbulent solar magnetic field models. Moreover, we show that for such magnetic fields inside the Sun, one can constrain the intrinsic neutrino magnetic moment down to the level of mu_nu lessthan few times 10^-12 x mu_B irrespective of details of the underlying turbulence model. This limit is more stringent than all current experimental sensitivities, and similar to the most stringent bounds obtained from stellar cooling. We also comment on the robustness of this limit and show that at most it might be weakened by one order of magnitude, under very unlikely circumstances.
dc.language.iso eng
dc.relation.ispartof Physical Review D, 2004, vol. 70, num. 11, p. 113002-113013
dc.subject Física
dc.title Enhanced solar antineutrino flux in random magnetic fields
dc.type journal article es_ES
dc.date.updated 2015-09-30T12:12:52Z
dc.identifier.doi 10.1103/PhysRevD.70.113002
dc.identifier.idgrec 018338
dc.rights.accessRights open access es_ES

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