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Accelerating black holes in anti-de Sitter universe
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The parameters ε and γ do not affect the geometry of the solution, as they do not appear in any curvature invariants, and are sometimes dubbed 'kinematical parameters'.
“Notably, the parameters ϵ and γ do not affect the geometry of the solution, as they do not appear in any curvature invariants [90], and sometimes dubbed 'kinematical parameters'.”
From Three-Dimensional Quantum Black Holes: A Primer (2024) · cites this paper as [90]
The Plebanski-Demianski metric describes the most general algebraic type-D spacetime solving Einstein-Maxwell theory in vacuum with an aligned, non-zero electromagnetic field and a cosmological constant Λ.
“The PD metric describes the most general algebraic type-D spacetime solving Einstein-Maxwell theory in vacuum with an aligned, non-zero electromagnetic field and a cosmological constant Λ.”
From Three-Dimensional Quantum Black Holes: A Primer (2024) · cites this paper as [90]
The most general metric solving the Einstein-Maxwell-Λ gravity is the Plebiański-Demiański type-D metric.
“The most general metric solving the Einstein-Maxwell-Λ gravity is the Plebiański-Demiański type-D metric [90].”
From Three-Dimensional Quantum Black Holes: A Primer (2024) · cites this paper as [90]
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Cites
The Large Scale Structure of Space-Time
Hawking, S. W., & Ellis, G. F. R. (1973) · doi:10.1017/cbo9780511524646 · Cited by 10,624
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Research works printed but not linked: 28
- J. Ehlers and W. Kundt: inGravitation: an Introduction to Current Research (Ed. L. Witten), Wiley, New York, 1962, p. 49.
- D. Kramer, H. Stephani, M. MacCallum, and E. Herlt:Exact solutions of Einstein’s field equations, Cambridge University Press, Cambridge, 1980.
- J. Bičák and B. Schmidt: Phys. Rev. D40 (1989) 1827. · DOI
- W. Kinnersley and M. Walker: Phys. Rev. D2 (1970) 1359. · DOI
- H. Farhoosh and R.L. Zimmerman: Phys. Rev. D21 (1980) 317. · DOI
- A. Ashtekar and T. Dray: Commun. Math. Phys.79 (1981) 581. · DOI
- W.B. Bonnor: Gen. Relativ. Gravit.15 (1983) 535. · DOI
- F.H.J. Cornish and W.J. Uttley: Gen. Relativ. Gravit.27 (1995) 439. · DOI
- F.H.J. Cornish and W.J. Uttley: Gen. Relativ. Gravit.27 (1995) 735. · DOI
- V. Pravda and A. Pravdová: Czech. J. Phys.50 (2000) 333. · DOI
- J. Podolský and J.B. Griffiths: Gen. Relativ. Gravit.33 (2001) 105.
- R. Gleiser and J. Pullin: Class. Quantum Grav.6 (1989) L141. · DOI
- J. Bičák: Astron. Nachr.311 (1990) 189. · DOI
- P.A. Hogan: Phys. Rev. Lett.70 (1993) 117. · DOI
- J. Podolský and J.B. Griffiths: Class. Quantum Grav.17 (2000) 1401. · DOI
- A.N. Aliev and Y. Nutku: Class. Quantum Grav.18 (2001) 891. · DOI
- J.F. Plebanski and M. Demianski: Ann. Phys. (NY)98 (1976) 98. · DOI · Paper page
- B. Carter: Commun. Math. Phys.10 (1968) 280. · DOI · Paper page
- R. Debever: Bull. Soc. Math. Belg.23 (1971) 360.
- J. Bičák and V. Pravda: Phys. Rev. D60 (1999) 044004. · DOI
- P.S. Letelier and S.R. Oliveira: Phys. Rev. D64 (2001) 064005. · DOI
- R.B. Mann and S.F. Ross: Phys. Rev. D52 (1995) 2254. · DOI · Paper page
- R.B. Mann: Class. Quantum Grav.14 (1997) L109. · DOI
- J. Podolský and J.B. Griffiths: Phys. Rev. D63 (2001) 024006. · DOI
- J. Bičák and P. Krtouš: Phys. Rev. D64 (2001) 124020. · DOI
- K. Lake and R.C. Roeder: Phys. Rev. D15 (1977) 3513. · DOI
- H. Laue and M. Weiss: Phys. Rev. D16 (1977) 3376. · DOI
- J. Bičák and J. Podolský: Phys. Rev. D55 (1997) 1985. · DOI
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
- Podolský, J.
- Venue
- Czechoslovak Journal of Physics
- Published
- 2002-01
- Volume
- 52
- Issue
- 1
- Pages
- 1-10
- ISSN
- 0011-4626
- 1572-9486
- Cited by
- 73
- References
- 1
- Language
- en
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