Solar Model Parameters and Direct Measurements of Solar Neutrino Fluxes

dc.contributor.areaPhysicsen_US
dc.contributor.authorBandyopadhyay, Abhijiten_US
dc.contributor.authorChoubey, Sandhyaen_US
dc.contributor.authorGoswami, Srubabatien_US
dc.contributor.authorPetcov, Serguey T.en_US
dc.contributor.departmentElementary Particle Theoryen_US
dc.date.accessioned2006-09-07T10:32:29Zen_US
dc.date.accessioned2011-09-07T20:27:33Z
dc.date.available2006-09-07T10:32:29Zen_US
dc.date.available2011-09-07T20:27:33Z
dc.date.issued2006-09-07T10:32:29Zen_US
dc.description.abstractWe explore a novel possibility of determining the solar model parameters, which serve as input in the calculations of the solar neutrino fluxes, by exploiting the data from direct measurements of the fluxes. More specifically, we use the rather precise value of the $^8B$ neutrino flux, $\phi_B$ obtained from the global analysis of the solar neutrino and KamLAND data, to derive constraints on each of the solar model parameters on which $\phi_B$ depends. We also use more precise values of $^7Be$ and $pp$ fluxes as can be obtained from future prospective data and discuss whether such measurements can help in reducing the uncertainties of one or more input parameters of the Standard Solar Model.en_US
dc.format.extent329712 bytesen_US
dc.format.mimetypeapplication/pdfen_US
dc.identifier.citationPhys. Rev. D 75 (2007) 093007en_US
dc.identifier.urihttps://openscience.sissa.it/handle/1963/1851en_US
dc.language.isoen_USen_US
dc.relation.ispartofseriesSISSA;44/2006/EPen_US
dc.relation.ispartofseriesarXiv.org;hep-ph/0608323en_US
dc.relation.uri10.1103/PhysRevD.75.093007en_US
dc.titleSolar Model Parameters and Direct Measurements of Solar Neutrino Fluxesen_US
dc.typePreprinten_US
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