期刊
JOURNAL OF HIGH ENERGY PHYSICS
卷 -, 期 3, 页码 -出版社
SPRINGER
DOI: 10.1007/JHEP03(2016)132
关键词
Neutrino Physics; Solar and Atmospheric Neutrinos
资金
- Spanish MINECO [ESP2014-56003-R, FPA2011-29678, FPA2012-31880, FPA2012-34694, FPA2013-46570]
- Severo Ochoa program of IFT [SEV-2012-0249]
- Maria de Maeztu program of ICCUB [MDM-2014-0369]
- consolider-ingenio [CSD-2008-0037]
- CUR Generalitat de Catalunya [2014-SGR-104, 2014-SGR-1458]
- Generalitat Valenciana Prometeo grant [II/2014/050]
- USA-NSF [PHY-13-16617]
- EU [PITN-GA-2011-289442]
- Division Of Physics
- Direct For Mathematical & Physical Scien [1316617] Funding Source: National Science Foundation
- ICREA Funding Source: Custom
We present an update of the determination of the solar neutrino fluxes from a global analysis of the solar and terrestrial neutrino data in the framework of three-neutrino mixing. Using a Bayesian analysis we reconstruct the posterior probability distribution function for the eight normalization parameters of the solar neutrino fluxes plus the relevant masses and mixing, with and without imposing the luminosity constraint. We then use these results to compare the description provided by different Standard Solar Models. Our results show that, at present, both models with low and high metallicity can describe the data with equivalent statistical agreement. We also argue that even with the present experimental precision the solar neutrino data have the potential to improve the accuracy of the solar model predictions.
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