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Exact solutions of topologically massive gravity with a cosmological constant
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These limiting geometries have the same qualitative features as (warped) dS3 black hole solutions to topologically massive gravity.
“These limiting geometries, moreover, have the same qualitative features as (warped) dS 3 black hole solutions to topologically massive gravity, cf.[37,38,110].”
From Three-Dimensional Quantum Black Holes: A Primer (2024) · cites this paper as [37]
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Research works printed but not linked: 11
- 10.1103/PhysRevLett.48.975 · DOI
- Deser S, 1982, Ann. Phys., NY, 140, 372, 10.1016/0003-4916(82)90164-6 · DOI
- Nutku Y, 1989, Ann. Phys., NY, 195, 16, 10.1016/0003-4916(89)90094-8 · DOI
- 10.1016/0370-2693(85)90199-6 · DOI
- Percacci R, 1986, Ann. Phys., NY, 176, 344, 10.1016/0003-4916(87)90006-6 · DOI
- Oritz M, 1990, Ann. Phys., NY, 200, 345, 10.1016/0003-4916(90)90278-V · DOI
- 10.1063/1.527978 · DOI
- 10.1063/1.529956 · DOI
- Hall G S, 1987, Gen. Rel. Grav., 19, 1137, 10.1007/BF00759150 · DOI
- Dereli T, 1988, Class. Quantum Grav., 5, 951, 10.1088/0264-9381/5/7/004 · DOI
- 10.1103/PhysRevLett.69.1849 · DOI · Paper page
Cited by
Sorted by citations
The (2 + 1)-dimensional black hole
Carlip, S. (1995) · Classical and Quantum Gravity · doi:10.1088/0264-9381/12/12/005 · Cited by 609
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
- Nutku, Y.
- Venue
- Classical and Quantum Gravity
- Publisher
- IOP Publishing
- Published
- 1993-12-01
- Volume
- 10
- Issue
- 12
- Pages
- 2657-2661
- ISSN
- 0264-9381
- 1361-6382
- Cited by
- 93
- References
- 0
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