Static solutions and equilibrium distributions of a gravitating fluid in general relativity. I - Plane symmetry

Statistics – Computation

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Computational Astrophysics, Density Distribution, Gravitational Fields, Incompressible Fluids, Relativistic Theory, Static Characteristics, Cosmology, Einstein Equations, Equations Of State, Equilibrium Equations

Scientific paper

Static V4 fields and equilibrium distributions of a plane-symmetric gravitating liquid are studied in the framework of the general relativity theory, on the basis of the obtained analytic solutions, for polytropic relativistic equations of state. P = nɛ (0 < n ≤ 1), as well as for a plane homogeneous layer of a non-compressible medium with ɛ0 = const. It is shown that plane-symmetric static solutions of the Einstein equations always contain a physical vacuum singularity, a singular repulsing plane with negative gravitational mass, and are thus principally different from an infinite plane equilibrium layer of liquid in the Newtonian theory.

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