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Centrifugal Force and Ellipticity behaviour of a slowly rotating ultra compact object

Anshu Gupta, Sai Iyer, A. R. Prasanna

gr-qcarXiv:gr-qc/9603055

Abstract

Using the optical reference geometry approach, we have derived in the following, a general expression for the ellipticity of a slowly rotating fluid configuration using Newtonian force balance equation in the conformally projected absolute 3-space, in the realm of general relativity. Further with the help of Hartle-Thorne (H-T) metric for a slowly rotating compact object, we have evaluated the centrifugal force acting on a fluid element and also evaluated the ellipticity and found that the centrifugal reversal occurs at around R/Rs ≈ 1.45, and the ellipticity maximum at around R/Rs ≈ 2.75. The result has been compared with that of Chandrasekhar and Miller which was obtained in the full 4-spacetime formalism.

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