Precise relativistic orbits in Kerr and Kerr-(anti) de Sitter spacetimes

18 May 2004G. V. Kraniotis

The timelike geodesic equations resulting from the Kerr gravitational metric element are derived and solved exactly including the contribution from the cosmological constant. The geodesic equations are derived, by solving the Hamilton-Jacobi partial differential equation by separation of variables... (read more)

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