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Journal of High Energy Physics

, 2019:47 | Cite as

Jackiw-Teitelboim gravity and rotating black holes

  • Upamanyu MoitraEmail author
  • Sunil Kumar Sake
  • Sandip P. Trivedi
  • V. Vishal
Open Access
Regular Article - Theoretical Physics
  • 37 Downloads

Abstract

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.

Keywords

2D Gravity AdS-CFT Correspondence Black Holes Models of Quantum Gravity 

Notes

Open Access

This article is distributed under the terms of the Creative Commons Attribution License (CC-BY 4.0), which permits any use, distribution and reproduction in any medium, provided the original author(s) and source are credited

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© The Author(s) 2019

Authors and Affiliations

  1. 1.Department of Theoretical PhysicsTata Institute of Fundamental ResearchMumbaiIndia

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