Jackiw-Teitelboim gravity and rotating black holes

被引:0
作者
Upamanyu Moitra
Sunil Kumar Sake
Sandip P. Trivedi
V. Vishal
机构
[1] Tata Institute of Fundamental Research,Department of Theoretical Physics
来源
Journal of High Energy Physics | / 2019卷
关键词
2D Gravity; AdS-CFT Correspondence; Black Holes; Models of Quantum Gravity;
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摘要
We show that the free energy at low temperatures for near-extremal black holes is correctly obtained from the Jackiw-Teitelboim (JT) model of gravity. Our arguments apply to all black holes, including rotating ones, whose metric has a near-horizon AdS2 factor and the associated SL (2, ℝ) symmetry. We verify these arguments by explicit calculations for rotating black holes in 4 and 5 dimensions. Our results suggest that the JT model could prove useful in analysing the dynamics of near-extremal Kerr black holes found in nature.
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共 252 条
[1]  
Teitelboim C(1983) 1 Phys. Lett. B 126 41-undefined
[2]  
Jackiw R(1985) 2 Nucl. Phys. B 252 343-undefined
[3]  
Almheiri A(2015) 2 JHEP 11 014-undefined
[4]  
Polchinski J(2018)( JHEP 09 048-undefined
[5]  
Nayak P(2019)) JHEP 07 055-undefined
[6]  
Moitra U(1993) 0 + 1 Prog. Theor. Phys. 90 247-undefined
[7]  
Trivedi SP(2016)5 JHEP 04 001-undefined
[8]  
Vishal V(2016)undefined JHEP 07 007-undefined
[9]  
Muta T(2016)undefined Phys. Rev. D 94 106002-undefined
[10]  
Odintsov SD(2016)undefined Phys. Rev. Lett. 117 111601-undefined