Limits of the Tomimatsu-Sato gravitational field

Mathematics

Scientific paper

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Einstein Equations, Extremum Values, Gravitation Theory, Gravitational Fields, Rotating Bodies, Limits (Mathematics), Mathematical Models, Moments Of Inertia, Newton Theory, Oblate Spheroids, Potential Theory, Singularity (Mathematics), Theoretical Physics

Scientific paper

The Tomimatsu-Sato (TS) solutions of the Einstein field equations are studied in several limiting cases. In the weak-field limit we construct two Newtonian models for the source, one consisting of a rotating disk of radius a/n, the other made up of n complex point multipoles. The 'extreme' limit q = 1 is also examined in detail, and we find there are many distinct ways of taking this limit. We are thereby led to a new two-parameter family of exact solutions which, unlike the TS metrics, are not asymptotically flat.

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