2013/04/30 by Sebastian Fischetti, Jorge E. Santos
Physics and Astronomy · #Angular momentum #Angular velocity #Black Holes and Theoretical Physics #Black hole (networking) #Cauchy stress tensor #Cosmology and Gravitation Theories #Coupling (piping) #Extremal black hole #Horizon #Quantum Electrodynamics and Casimir Effect #Rotating black hole #Tensor (intrinsic definition) #Unruh effect #gr-qc #hep-th
paper · pdf · doi:10.1007/jhep07(2013)156
published as JHEP 07 (2013) 156 · 29 pages. v2: Updated to correct a mistake and address referee's comments
openalex publication_date 2013/07/01 · arxiv created 2013/07/31 · arxiv updated 2013/08/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
We construct the gravitational dual, in the Unruh state, of the "jammed" phase of a CFT at strong coupling and infinite N on a fixed five-dimensional rotating Myers-Perry black hole with equal angular momenta. When the angular momenta are all zero, the solution corresponds to the five-dimensional generalization of the solution first studied by Figueras, Lucietti, and Wiseman. In the extremal limit, when the angular momenta of the Myers-Perry black hole are maximum, the Unruh, Boulware and Hartle-Hawking states degenerate. We give a detailed analysis of the corresponding holographic stress energy tensor for all values of the angular momenta, finding it to be regular at the horizon in all cases. We compare our results with existent literature on thermal states of free field theories on black hole backgrounds.