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The Standard Solar Model

Published online by Cambridge University Press:  12 April 2016

J.N. Bahcall  and
M. Cribier
J.N. Bahcall
Affiliation:
Institute for Advanced Study,NJ 08540, Princeton, USA
M. Cribier
Affiliation:
CEN SACLAY DPhPE/SEPh, F-91191 GIF-sur Yvette CEDEX, France

Abstract

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The main features of standard solar models, the logic of the calculations, and some of the important results concerning solar neutrinos experiments are given. The input parameters that cause the greatest uncertainties in the calculated neutrino fluxes are the nuclear rection rates, the chemical abundances, the radiative opacity, and the equation of state. This article is based, with permission of the publisher, on Chapters 1 and 4 of Neutrino Astrophysics by J. N. Bahcall, Cambridge University Press (1989).

Type
Part 1: Solar Modelling
Information
International Astronomical Union Colloquium , Volume 121: Inside the Sun , 1990 , pp. 21 - 41
Copyright
Copyright © Kluwer 1990

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