Rotating and accelerating black holes with cosmological constant
General Relativity and Quantum Cosmology
2016-08-10 v2
Abstract
We propose a new form of the rotating C-metric with cosmological constant, which generalises the form found by Hong and Teo for the Ricci-flat case. This solution describes the entire class of spherical black holes undergoing rotation and acceleration in dS or AdS space-time. The new form allows us to identify the complete ranges of coordinates and parameters of this solution. We perform a systematic study of its geometrical and physical properties, and of the various limiting cases that arise from it.
Cite
@article{arxiv.1606.02415,
title = {Rotating and accelerating black holes with cosmological constant},
author = {Yu Chen and Cheryl Ng and Edward Teo},
journal= {arXiv preprint arXiv:1606.02415},
year = {2016}
}
Comments
36 pages, 5 figures; v2: references added; as accepted for publication in Phys. Rev. D