Exact solutions for charged spheres and their stability. II. Anisotropic Fluids
Abstract
We study exact solutions of the Einstein-Maxwell equations for the interior gravitational field of static spherically symmetric charged compact spheres. The spheres consist of an anisotropic fluid with a charge distribution that gives rise to a static radial electric field. The density of the fluid has the form (r) = o + α r2 (here o and α are constants) and the total charge q(r) within a sphere of radius r has the form q = β r3 (with β a constant). We evaluate the critical values of M/R for these spheres as a function of Q/R and compare these values with those given by the Andr\'easson formula.
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