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A simple derivation and interpretation of the third integral in stellar dynamics

โœ Scribed by D. Lynden-Bell


Publisher
John Wiley and Sons
Year
2003
Tongue
English
Weight
64 KB
Volume
338
Category
Article
ISSN
0035-8711

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โœ H. J. Haubold; A. M. Mathai ๐Ÿ“‚ Article ๐Ÿ“… 1986 ๐Ÿ› John Wiley and Sons ๐ŸŒ English โš– 252 KB ๐Ÿ‘ 1 views

This paper deals with complete analytic solution to the problem of evaluating the total net rate of nuclear energy generation and the basic integral of the luminosity of a purely gaseous star in hydrostatic equilibrium. It is assumed that the total energy production is proportional to certain powers

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Necessary and sufficient conditions for the strong ellipticity of isotropic hyperelastic materials were first given by Knowles and Sternberg [3,4] by means of a lengthy calculation. Since then Aubert and Tahraoui [1] have shown the necessity of these conditions and simplified one of them using a dif