Pseudo-Kerr Geometry

Details Pseudo-Kerr Geometry Pseudo-Kerr Geometry

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008mgm..conf.1119m&link_type=abstract

"THE ELEVENTH MARCEL GROSSMANN MEETING On Recent Developments in Theoretical and Experimental General Relativity, Gravitation an

Computer Science

Scientific paper

We present here a simplified approach to the study of particle dynamics around rotating black holes. We show that with a suitably modified effective potential of the central gravitating rotating object, one can carry out these studies very accurately in Newtonian formalism provided the Kerr parameter remains within -1 ≤ a ≤ 0.8. We present the geometrical quantities which are useful to study the particle dynamics from our potential and also compare it to the general relativistic result.

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