On the definition of mass-energy of a static spherically-sysmmetric mass in the post-Newtonian approximation of general relativity

Astronomy and Astrophysics – Astrophysics

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Energy Conservation, Equations Of Motion, Gauge Theory, Mass, Relativistic Theory, Schwarzschild Metric, Coordinate Transformations, Gravitational Fields, Spheres, Steady State, Symmetry

Scientific paper

Recently we (Roy and Rana, 1990a) critically examined the self-consistency of the EIH equations of motion. A static spherically symmetric body, as was pointed out there, may not appear as a point mass with all its mass concentrated at its center to a particle placed outside the body. An attempt to analyze this aspect further is made here in the context of the Chandrasekhar gauge. A comparison is also made with the general solutions obtained by Schwarzschild in the standard co-ordinates. Certain difficulties still exist.

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