Consideration of the Competing Factors in Calculations of the Characteristics of Non-Magnetic Degenerate Dwarfs
Keywords:mechanical equilibrium equation, interparticle interactions, axial rotation, basis of universal functions, stability of dwarfs
Using the equation of state of the electron-nuclear model at high densities and the mechanical equilibrium equation, we have investigated the influence of interparticle interactions and the axial rotation on the macroscopic characteristics (mass, surface shape) of massive degenerate dwarfs. We propose a method of solving the equilibrium equation in the case of rotation that uses the basis of universal functions of the radial variable. The conditions, under which the axial rotation can compensate for a weight loss of the mass due to the Coulomb interactions, have been established. The maximal value of the relativistic parameter, at which the stability is disturbed, is determined within the general theory of relativity (GTR).
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