Rotating bodies in general relativity

Details Rotating bodies in general relativity Rotating bodies in general relativity

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983gregr..15..945g&link_type=abstract

General Relativity and Gravitation (ISSN 0001-7701), vol. 15, Oct. 1983, p. 945-957.

Physics

2

Gravitational Fields, Relativity, Rotating Bodies, Approximation, Axisymmetric Bodies, Einstein Equations, Mass Distribution, Metric Space, Tensor Analysis

Scientific paper

Synge's approximation method is used in order to obtain the gravitational field of a massive body with an axis of symmetry around which it is rotating steadily. The method is carried out to include the second approximation. This means that terms of order m2 are retained as significant, and there is an error of order m3 in the field equations, m being the mass of the body.

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