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Ultraspinning limits and super-entropic black holes

  • Robie A. Hennigar
  • David Kubizňák
  • Robert B. Mann
  • Nathan Musoke
Open Access
Regular Article - Theoretical Physics

Abstract

By employing the new ultraspinning limit we construct novel classes of black holes with non-compact event horizons and finite horizon area and study their thermo-dynamics. Our ultraspinning limit can be understood as a simple generating technique that consists of three steps: i) transforming the known rotating AdS black hole solution to a special coordinate system that rotates (in a given 2-plane) at infinity ii) boosting this rotation to the speed of light iii) compactifying the corresponding azimuthal direction. In so doing we qualitatively change the structure of the spacetime since it is no longer pos-sible to return to a frame that does not rotate at infinity. The obtained black holes have non-compact horizons with topology of a sphere with two punctures. The entropy of some of these exceeds the maximal bound implied by the reverse isoperimetric inequality, such black holes are super-entropic.

Keywords

Black Holes in String Theory Black Holes 

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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Copyright information

© The Author(s) 2015

Authors and Affiliations

  • Robie A. Hennigar
    • 1
  • David Kubizňák
    • 1
    • 2
  • Robert B. Mann
    • 1
  • Nathan Musoke
    • 2
  1. 1.Department of Physics and AstronomyUniversity of WaterlooWaterlooCanada
  2. 2.Perimeter InstituteWaterlooCanada

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