arXiv · 1109.0676
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.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Sumanta Chakraborty, Subenoy Chakraborty. 2011-09-04. Trajectory around a spherically symmetric non-rotating black hole. https://doi.org/10.1139/p11-032
Cite the original work for its findings. Save a collection to share your selection of sources.