Trajectory around a spherically symmetric non-rotating black hole

Abstract

Trajectory of a test particle or a photon around a general spherical black hole is studied and bending of light trajectory is investigated. Pseudo-Newtonian gravitational potential describing the gravitational field of the black hole is determined and is compared with the related effective potential for test particle motion. As an example, results are presented for Reissner-Nordström black hole.

13 pages, 6 figures

References in corpus (1)

• Pseudo-Newtonian gravitational potential for Schwarzschild-de Sitter spacetimes

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