Researching turbulent convection models and the density gradient reversing

Details Researching turbulent convection models and the density gradient reversing Researching turbulent convection models and the density gradient reversing

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008iaus..252..133z&link_type=abstract

The Art of Modeling Stars in the 21st Century, Proceedings of the International Astronomical Union, IAU Symposium, Volume 252, p

Astronomy and Astrophysics

Astronomy

Convection, Hydrodynamics, Stars: Interiors

Scientific paper

Turbulent convection models (TCM) provide a better way to study
convection in stars than the MLT. Improving numerical method, we adopted
larger diffusion parameters and smaller dissipation parameters in order
to further correct the p-mode oscillation frequencies of TCM models. The
density gradient reversing is discussed.

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