On the spinning C-metric
General Relativity and Quantum Cosmology
2016-11-09 v1
Abstract
Physical interpretation of some stationary and non-stationary regions of the spinning C-metric is presented. They represent different spacetime regions of a uniformly accelerated Kerr black hole. Stability of geodesics corresponding to equilibrium points in a general stationary spacetime with an additional symmetry is also studied and results are then applied to the spinning C-metric.
Keywords
Cite
@article{arxiv.gr-qc/0201025,
title = {On the spinning C-metric},
author = {V. Pravda and A. Pravdova},
journal= {arXiv preprint arXiv:gr-qc/0201025},
year = {2016}
}
Comments
12 pages, 7 figures, RevTeX 4