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Accelerating black holes in anti-de Sitter universe

Jiri Podolsky
(
- Charles U., Inst. Theor. Phys.
)

Feb, 2002

9 pages

Published in:

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

e-Print:

gr-qc/0202033 [gr-qc]

DOI:

10.1023/A:1013961411430

View in:

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Abstract: (arXiv)

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.

Note:

Dedicated to J. Bicak on occasion of his 60th birthday

black hole: acceleration
space-time: anti-de Sitter
cosmological constant
Einstein equation: solution

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Figures(0)

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