Regular axisymmetric description of the Kerr spacetime

Details Regular axisymmetric description of the Kerr spacetime Regular axisymmetric description of the Kerr spacetime

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005gregr..37..793m&link_type=abstract

General Relativity and Gravitation, Volume 37, Issue 4, pp.793-801

Computer Science

1

Black Holes, Horizon, Kerr Metric

Scientific paper

In this work we present the Kerr space-time in a coordinate system compatible with the general expression for the stationary axial symmetric space times described in the Papapetrou form of the line element. We show that in these coordinates the metric coefficients are regular at least up to the external horizon, thus making it an adequate description for the analysis of phenomena near or at the horizon. Furthermore, we construct a null tetrad and present the equations for the perturbed Ψ4 Weyl component, which again shows no divergences in the present description.

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