Numerical calculation of bound geodesics in the Kerr metric

Details Numerical calculation of bound geodesics in the Kerr metric Numerical calculation of bound geodesics in the Kerr metric

Sep 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974zphy..271..275g&link_type=abstract

Zeitschrift für Physik, Volume 271, Issue 3, pp.275-279

Astronomy and Astrophysics

Astronomy

3

Scientific paper

Timelike geodesics, especially bound orbits in the equatorial plane ( ϑ=π/2) and spherical orbits ( r=const), are calculated numerically. We plot the orbits using the Kerr-Schild coordinate system. The periastron advance and the dragging of nodes have the same values in any coordinate system and can be directly measured by an observer at infinity.

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