Nonlinear Dynamical Stability of Newtonian Rotating White Dwarfs and Supermassive Stars
نویسندگان
چکیده
We prove general nonlinear stability and existence theorems for rotating star solutions which are axi-symmetric steady-state solutions of the compressible isentropic EulerPoisson equations in 3 spatial dimensions. We apply our results to rotating and nonrotating white dwarf, and rotating high density supermassive (extreme relativistic) stars, stars which are in convective equilibrium and have uniform chemical composition. This paper is a continuation of our earlier work ([28]).
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