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Higher Dimensional Charged AdS Black Holes at Ultra-spinning Limit and Their 2d CFT Duals

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arxiv 1702.03448 v2 pith:EBMBGRXH submitted 2017-02-11 hep-th gr-qc

classification hep-thgr-qc
keywords blackcftschargeddimensionaldualentropyholeshorizon
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abstract

By using the ultra-spinning limit as a generating solution technique, we construct a novel class of charged rotating asymptotic AdS black holes. That describes the exact D-dimnsioanl solutions of Einstein-Maxwell dilaton theory in the presence of negative cosmological constant. The obtained geometries possess some punctures, describing a noncompact horizon, but has a finite area. We then explicitly investigate the validity of the Kerr/CFT correspondence for all dimensional cases. We find a main result for the central charges associated to $[(d-1)/2]$ copies of dual $2D$ CFTs. We then argue the existence of a precise agreement between the microscopic entropy of dual CFTs and the entropy of the noncompact horizon.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Dimensional structure of thermodynamic topology in ultraspinning Kerr-AdS black holes

    hep-th 2026-02 conditional novelty 6.0 of 10

    Ultraspinning Kerr-AdS black holes fall into two thermodynamic-topology classes: W^{1+} for all even dimensions and odd dimensions with fewer rotations, and tilde W^{1+} for odd dimensions with maximal rotations.

  2. Thermodynamic Instabilities of Generalized Exotic BTZ Black Holes

    gr-qc 2019-08 accept novelty 6.0 of 10

    Generalized exotic BTZ black holes can have positive specific heat at constant volume despite violating the reverse isoperimetric inequality, countering a recent conjecture.

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