2005/03/02 by Troels Harmark, T. Harmark, Niels A. Obers +1 · 1 citation
Mathematics · Physics and Astronomy · #Astrophysical Phenomena and Observations #Black Holes and Theoretical Physics #Black brane #Black hole (networking) #Black hole thermodynamics #Black string #Brane cosmology #Canonical ensemble #Cosmology and Gravitation Theories #Entropy (arrow of time) #Extremal black hole #Kaluza–Klein theory #Mathematical physics #Mathematics #Minkowski space #Physics #Quantum mechanics #String (physics) #String theory #Theoretical physics #hep-th
paper · pdf · doi:10.1002/prop.200510215
published as Fortsch.Phys. 53 (2005) 536-541; Fortsch.Phys. 53 (2005) 900-905 · 9 pages, Proceedings for RTN Workshop in Kolymbari, Crete, September 5-10, 2004, and 37th International Symposium Ahrenshoop, Wernsdorf, August 23-27, 2004
arxiv created 2005/03/02 · openalex publication_date 2005/04/27 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Abstract We review the recently found map that takes any static and neutral Kaluza‐Klein black hole, i.e. any static and neutral black hole on Minkowski‐space times a circle ℳ︁ d × S 1 , and maps it to a corresponding solution for a non‐ and near‐extremal brane on a circle. This gives a precise connection between phases of Kaluza‐Klein black holes and the thermodynamic behavior of the non‐gravitational theories dual to near‐extremal branes on a circle. In particular, for the thermodynamics of strongly‐coupled supersymmetric Yang‐Mills theories on a circle we predict the existence of a new non‐uniform phase and find new information about the localized phase. We also find evidence for the existence of a new stable phase of (2,0) Little String Theory in the canonical ensemble for temperatures above its Hagedorn temperature.