Approximate Kerr-like interior and exterior solutions for a very slowly rotating star of perfect fluid

Details Approximate Kerr-like interior and exterior solutions for a very slowly rotating star of perfect fluid Approximate Kerr-like interior and exterior solutions for a very slowly rotating star of perfect fluid

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ijps....6...93n&link_type=abstract

International Journal of the Physical Sciences Vol. 6(1), pp. 93-97, 2011

Physics

Slowly Rotating Oblate Star, Approximate Kerr- Like Metric, Exterior Interior Solution

Scientific paper

Approximate Kerr- like interior and exterior solutions for a very slowly rotating star of perfect fluid is presented here which is valid for a very slowly rotating and hence very slightly oblate star of perfect fluid rotating with a very small constant angular velocity. Corresponding approximate exterior metric represents approximate Kerr exterior metric for a perfect fluid. The aim here is to obtain Kerr-like approximate exterior and interior solutions for a very slowly rotating star of perfect fluid simply following standard procedure used to obtain Schwarzschild solutions.

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