A model of the sun with a neutrally stable core

Details A model of the sun with a neutrally stable core A model of the sun with a neutrally stable core

Feb 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984azh....61..170v&link_type=abstract

(Astronomicheskii Zhurnal, vol. 61, Jan.-Feb. 1984, p. 170-176) Soviet Astronomy (ISSN 0038-5301), vol. 28, Jan.-Feb. 1984, p. 1

Physics

5

Solar Neutrinos, Stellar Cores, Stellar Models, Convection, Nuclear Reactions, Opacity, Solar Atmosphere, Solar Oscillations, Solar Physics, Stellar Composition, Stellar Envelopes, Stellar Structure

Scientific paper

Using simplified formulae for the energy production and opacity a solar model is considered which consists of a convective envelope, a middle, chemically homogeneous radiative zone and a neutrally stable against convection, inhomogeneous core. Between the latter two zones, there is a jump-like change in density and composition. In comparison with the standard solar model, this model has a considerably lesser mass concentration to the centre and a smaller rate of neutrino production.

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