The central solar temperature T and its uncertainties are calculated in helioseismologically-constrained solar models. From the best fit to the convective radius, density at the convective radius and seismically determined helium abundance the central temperature is found to be T = 1.58 x 10(7) K, in excellent agreement with Standard Solar Models. Conservatively, we estimate that the accuracy of this determination is Delta T/T = 1.4%, better than that in SSM. Neutrino fluxes are calculated, The lower limit to the boron neutrino flux, obtained with maximum reduction factors from all sources of uncertainties, is 2 sigma higher than the flux measured recently by SuperKamiokande. (C) 1997 Published by Elsevier Science B.V.
|Autori:||Ricci B; Berezinsky V; Degl'Innocenti S; Dziembowski WA; Fiorentini G|
|Titolo:||Helioseismic constraints to the central solar temperature and neutrino fluxes|
|Anno del prodotto:||1997|
|Digital Object Identifier (DOI):||10.1016/S0370-2693(97)00759-4|
|Appare nelle tipologie:||1.1 Articolo in rivista|