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Adiabatic Oscillations of Solar Models with a High-Z Convective Zone*

Published online by Cambridge University Press:  12 April 2016

S.V. Vorontsov  and
K.I. Marchenkov
S.V. Vorontsov
Affiliation:
Department of Theoretical Physics, Institute of Physics of the Earth, Academy of Sciences of the USSR, Moscow 123810, U.S.S.R.
K.I. Marchenkov
Affiliation:
Department of Theoretical Physics, Institute of Physics of the Earth, Academy of Sciences of the USSR, Moscow 123810, U.S.S.R.

Abstract

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Normal mode spectra and neutrino counting rates are calculated for a set of chemically-inhomogeneous solar models. Each model has a core with a high concentration of heavy elements; high opacity makes the core convective. The structure of the envelope is that of the standard model. It is shown that (1) the spectrum of g modes becomes less densely separated than that of the standard model, which simplifies the problem of interpreting 160-min oscillations; (2) low neutrino counting rates may be achieved for a low initial helium concentration in the core; (3) the models do not contradict the frequency spacing of global 5-min oscillations.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 66: Problems of Solar and Stellar Oscillations , 1983 , pp. 215 - 222
Copyright
Copyright © Reidel 1983

Footnotes

*

Proceedings of the 66th IAU Colloquium: Problems in Solar and Stellar Oscillations, held at the Crimean Astrophysical Observatory, U.S.S.R., 1–5 September, 1981.

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