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New class of accelerating black hole solutions
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No exact solutions to Einstein's equations describing accelerating black holes in dimension D = d + 1 > 4 are known.
“Notably, however, no exact solutions to Einstein's equations describing accelerating 47 Notably, the three branches described here do not coincide with branches 1a, 1b, and 2 characterizing the mass of the qBTZ [25].”
From Three-Dimensional Quantum Black Holes: A Primer (2024) · cites this paper as [192]
In D ≥ 5, the string generating the acceleration has a singularity along its symmetry axis passing through the black hole which is distinctly less mild than in D = 4.
“As reasoned in [192], this is because in D ≥ 5, the string generating the acceleration has a singularity along its symmetry axis passing through the black hole which is distinctly less mild than in D = 4.”
From Three-Dimensional Quantum Black Holes: A Primer (2024) · cites this paper as [192]
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Emparan, R., Gregory, R., & Santos, C. (2001) · Physical Review D · doi:10.1103/physrevd.63.104022 · Cited by 61
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Cited by
Sorted by citations
Three-Dimensional Quantum Black Holes: A Primer
Panella, E., Pedraza, J. F., & Svesko, A. (2024) · Universe · doi:10.3390/universe10090358 · Cited by 24
Metadata
- Authors
- Camps, J., & Emparan, R.
- Venue
- Physical Review D
- Publisher
- American Physical Society (APS)
- Published
- 2010-07-13
- Volume
- 82
- Issue
- 2
- ISSN
- 1550-7998
- 1550-2368
- Cited by
- 6
- References
- 1
- Language
- en
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