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Quantum Kerr-de Sitter black holes in three dimensions
Abstract
A bstract: We use braneworld holography to construct a three-dimensional quantum-corrected Kerr-de Sitter black hole, exactly accounting for semi-classical backreaction effects due to a holographic conformal field theory. By contrast, classically there are no de Sitter black holes in three-dimensions, only geometries with a single cosmological horizon. The quantum Kerr black hole shares many qualitative features with the classical four-dimensional Kerr-de Sitter solution. Of note, backreaction induces inner and outer black hole horizons which hide a ring singularity. Moreover, the quantum-corrected geometry has extremal, Nariai, and ultracold limits, which appear as fibered products of a circle and two-dimensional anti-de Sitter, de Sitter, and Minkowski space, respectively. The thermodynamics of the classical bulk black hole, described by the rotating four-dimensional anti-de Sitter C-metric, has an interpretation on the brane as thermodynamics of the quantum black hole, obeying a semi-classical first law where the Bekenstein-Hawking area entropy is replaced by the generalized entropy. For purposes of comparison, we derive the renormalized quantum stress-tensor due to a free conformally coupled scalar field in the classical Kerr-de Sitter conical geometry and perturbatively solve for its backreaction.
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The rotating and charged holographic quantum black holes do not match the non-holographic perturbatively-corrected counterparts.
“The rotating and charged holographic quantum black holes, meanwhile, do not match to the non-holographic perturbatively-corrected counterparts (cf.[27,40,45]).”
From Three-Dimensional Quantum Black Holes: A Primer (2024) · cites this paper as [27]
Starting from the rotating C-metric (4.40) with κ = +1 and replacing a → -a, and imposing bulk regularity, the metric on the brane in canonically normalized coordinates is (4.114).
“Starting from the rotating C-metric (4.40) with κ = +1 and replacing a → -a, and imposing bulk regularity, the metric on the brane in canonically normalized coordinates is [27] foot_14”
From Three-Dimensional Quantum Black Holes: A Primer (2024) · cites this paper as [27]
The radial dependence of the renormalized stress-tensor due to a conformally coupled scalar field is significantly more complicated than the holographic stress-tensor.
“Further, as in the qBTZ case, the radial dependence of the renormalized stress-tensor due to a conformally coupled scalar field (found perturbatively in [27]) is significantly more complicated than the holographic stress-tensor.”
From Three-Dimensional Quantum Black Holes: A Primer (2024) · cites this paper as [27]
Substituting the geometry (4.114) into the gravity field equations results in a holographic stress-tensor with components of essentially the same form as (4.64).
“Substituting the geometry (4.114) into the gravity field equations results in a holographic stress-tensor with components of essentially the same form as (4.64) -see [27] for explicit details.”
From Three-Dimensional Quantum Black Holes: A Primer (2024) · cites this paper as [27]
In the near-horizon regime, the limiting geometries appear as fibered products of a circle and two-dimensional anti-de Sitter, de Sitter, and Minkowski space, respectively.
“In the near-horizon regime, the geometries appear as fibered products of a circle and two-dimensional anti-de Sitter, de Sitter, and Minkowski space, respectively.”
From Three-Dimensional Quantum Black Holes: A Primer (2024) · cites this paper as [27]
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Surface terms as counterterms in the AdS-CFT correspondence
Emparan, R., Johnson, C. V., & Myers, R. C. (1999) · Physical Review D · doi:10.1103/physrevd.60.104001 · Cited by 703
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Three-Dimensional Quantum Black Holes: A Primer
Panella, E., Pedraza, J. F., & Svesko, A. (2024) · Universe · doi:10.3390/universe10090358 · Cited by 24
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- Authors
- Panella, E., & Svesko, A.
- Venue
- Journal of High Energy Physics
- Published
- 2023-06-21
- Volume
- 2023
- Issue
- 6
- ISSN
- 1029-8479
- Cited by
- 33
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