Semiconvective diffusion and energy transport

Details Semiconvective diffusion and energy transport Semiconvective diffusion and energy transport

Sep 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...126..207l&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 126, no. 1, Sept. 1983, p. 207, 208. Sponsorship: Deutsche Forschungsgemeinsch

Astronomy and Astrophysics

Astrophysics

85

Astrophysics, Convection, Diffusion, Energy Transfer, Stellar Structure, Diffusion Coefficient, Stellar Interiors, Temperature Gradients

Scientific paper

An expression is formulated, on the basis of radiation-driven overstability and nonradial oscillation theories, which is applicable to the semiconductive mixing in stellar interiors. A diffusion equation may then be applied independently of time to deviations from the Schwarzschild criterion, as well as to those from the Ledoux criterion and the mixing of chemical elements.

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