Comments on the diffusion model of turbulent mixing

Several recent investigations of post--main-sequence stellar evolution have used a diffusion model of turbulent mixing, and each author has used a different variation. We justify the diffusion model in the framework of a statistical theory of turbulence and show that the difference between the two d...

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Veröffentlicht in:	Astrophys. J.; (United States) 1976-06, Vol.206, p.548
Hauptverfasser:	Cloutman, L. D., Eoll, J. G.
Format:	Artikel
Sprache:	eng
Schlagworte:	640102 - Astrophysics & Cosmology- Stars & Quasi-Stellar, Radio & X-Ray Sources CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS DIFFUSION INSTABILITY MAIN SEQUENCE STARS MIXING RAYLEIGH-TAYLOR INSTABILITY STAR EVOLUTION STARS TURBULENCE
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