arXiv · 1903.09987
Periastron precession for an extremal spherically symmetric dilaton black hole
Abstract
The purpose of this article is to obtain the periastron precession of a free particle moving around an extremal spherically symmetric dilaton black hole. To get the formulae for the periastron precession we use the phase-plane analysis of the general relativistic equations of motion.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Paul Blaga, Cristina Blaga. 2019-03-24. Periastron precession for an extremal spherically symmetric dilaton black hole. https://arxiv.org/abs/1903.09987
Cite the original work for its findings. Save a collection to share your selection of sources.