Visualizing circular motion around a Schwarzschild black hole

Details Visualizing circular motion around a Schwarzschild black hole Visualizing circular motion around a Schwarzschild black hole

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011amjph..79...63m&link_type=abstract

American Journal of Physics, Volume 79, Issue 1, pp. 63-73 (2011).

Statistics

Computation

1

Black Holes, Differential Geometry, Interactive Programming, Observers, Physics Education, Schwarzschild Metric, Teaching, Computational Techniques, Simulations, General Relativity And Gravitation

Scientific paper

An observer who moves on a circular orbit around a Schwarzschild black hole with a constant but arbitrary velocity must compensate for the gravitational and centrifugal acceleration to stay on this orbit. The local reference frame of the observer undergoes a geodesic precession, which depends on the radius of the orbit and the velocity. We describe the details of this circular motion and an interactive program that shows what the observer would see.

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