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Microscopic Physics in the Solar Standard Model

Published online by Cambridge University Press:  12 April 2016

Ilidio Lopes and
Sylvaine Turck-Chieze
Ilidio Lopes
Affiliation:
Service d’Astrophysique, DAPNIA, CE Saclay, 91191 Gif-sur-Yvette Cedex 01, France
Sylvaine Turck-Chieze
Affiliation:
Service d’Astrophysique, DAPNIA, CE Saclay, 91191 Gif-sur-Yvette Cedex 01, France

Abstract

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The microphysics of the solar standard model is revised. We discuss the contribution of composition, nuclear reaction rates, screening effect and opacity (OPAL project) to the theoretical predictions on neutrino flux and acoustic modes.

Information

Type
I. Setting the stage: Sun, Stars Galaxies and the Universe
Information
International Astronomical Union Colloquium , Volume 137: Inside the Stars , 1993, pp. 51 - 53
Copyright
Copyright © Astronomical Society of the Pacific 1993

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