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On Solar Neutrinos and Chemically Inhomogeneous Solar Models

Published online by Cambridge University Press:  25 April 2016

S. J. Robinson
S. J. Robinson*
Affiliation:
Monash University
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Abstract

Work is in progress on the extension of a detailed stellar structure code to explore a suggested solution to the Solar Neutrino Problem where the Sun has a small (∼0.01M⊙) high-Z core on entry to the ZAMS. A basic premise of such models is that the core will burn itself out by solar age and the model acquire a neutrino luminosity in line with that observed. The work to date has involved the construction of a standard solar model and, currently, the development of inhomogeneous models with associated adjustments to the structure equations.

Type
Theoretical
Information
Publications of the Astronomical Society of Australia , Volume 7 , Issue 2 , 1987 , pp. 139 - 140
Copyright
Copyright © Astronomical Society of Australia 1987

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