A pure geometric primitive model for a main sequence star

Wanas, M.I. ; Samah Abd El-Aziz Saber Ammar 


he field equations, of a pure geometric field theory, are solved in the case of spherical symmetry. The solution obtained is shown to be an interior one with pure geometric material-energy tensor. This solution is obtained, assuming a perfect fluid filling a spherical configuration. An equation of state is obtained from, and not imposed on, the model. If the model is considered to represent a main sequence star, it gives rise to a corona and a radiation zone. Possibility of existence of a convection zone is discussed. Comparison with the parameters of the Sun is given.

Other data

Keywords Equation of state, Gravitation,Interiors Stars
Issue Date 2012
Conference 12th Marcel Grossmann Meeting on Recent Dev. in Theoretical and Experimental General Relativity, Astrophysics and Relativistic Field Theories - Proc. of the MG 2009 Meeting on General Relativity 
URI http://research.asu.edu.eg/handle/123456789/2453
ISBN 9814374512;978-981437451-4

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