Jackiw-Teitelboim gravity and rotating black holes

被引：65
|
作者：
Moitra, Upamanyu [1 ]
Sake, Sunil Kumar [1 ]
Trivedi, Sandip P. [1 ]
Vishal, V. [1 ]
机构：
[1] Tata Inst Fundamental Res, Dept Theoret Phys, Mumbai 400005, Maharashtra, India
来源：
JOURNAL OF HIGH ENERGY PHYSICS | 2019年 / 2019卷 / 11期
关键词：
2D Gravity; AdS-CFT Correspondence; Black Holes; Models of Quantum Gravity; THERMODYNAMICS; SPIN; FIELD; MASS;
D O I：
10.1007/JHEP11(2019)047
中图分类号：
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号：
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 AdS(2) 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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页数：51
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