TURBULENT CONVECTION MODEL IN THE OVERSHOOTING REGION. II. THEORETICAL ANALYSIS

Turbulent convection models (TCMs) are thought to be good tools to deal with the convective overshooting in the stellar interior. However, they are too complex to be applied to calculations of stellar structure and evolution. In order to understand the physical processes of the convective overshooti...

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Veröffentlicht in:	The Astrophysical journal 2012-05, Vol.750 (1), p.1-9
Hauptverfasser:	ZHANG, Q. S, LI, Y
Format:	Artikel
Sprache:	eng
Schlagworte:	ANALYTICAL SOLUTION ANISOTROPY APPROXIMATIONS Astronomy ASTROPHYSICS ASTROPHYSICS, COSMOLOGY AND ASTRONOMY ASYMPTOTIC SOLUTIONS Boundaries Computational fluid dynamics CONVECTION Correlation CORRELATIONS Decay DIFFUSION Dissipation Earth, ocean, space Exact sciences and technology HEAT FLUX KINETIC ENERGY Mathematical models STAR EVOLUTION STARS TURBULENCE
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