Accelerating Black Holes in Anti-de Sitter Universe

Article

Accelerating Black Holes in Anti-de Sitter Universe

Podolský, J.

Czech. J. Phys. 52, 1-10 (2002)

doi ↗ arXiv:gr-qc/0202033 ↗ link ↗

Abstract

A physical interpretation of the C-metric with a negative cosmological constant $\Lambda$ is suggested. Using a convenient coordinate system it is demonstrated that this class of exact solutions of Einstein's equations describes uniformly accelerating (possibly charged) black holes in anti-de Sitter universe. Main differences from the analogous de Sitter case are emphasised.

Keywords

C-metric - anti-de Sitter - black holes - acceleration

Institute authors

Podolský, Jiří

Supported by

GACR 202/99/0261 — Relativistic physics and astrophysics
GAUK 141/2000 — Relativistická teorie gravitace, astrofyzika a kosmologie

BibTeX

@article{UTF297,
  author        = {Podolský, J.},
  title         = {{Accelerating Black Holes in Anti-de Sitter Universe}},
  journal       = {Czech. J. Phys.},
  volume        = {52},
  pages         = {1-10},
  year          = {2002},
  doi           = {10.1023/A:1013961411430},
  eprint        = {gr-qc/0202033},
  archivePrefix = {arXiv},
  url           = {http://www.springerlink.com/content/t6ucn3y2p80bjy1x/fulltext.pdf},
}