2004/11/25 by Dietmar Klemm, Luciano Vanzo · 21 citations
Physics and Astronomy · #Black Holes and Theoretical Physics #Black hole (networking) #Black hole information paradox #Black hole thermodynamics #Computer science #Cosmology and Gravitation Theories #Entropy (arrow of time) #Mathematical physics #Micro black hole #Noncommutative and Quantum Gravity Theories #Physics #String theory #Theoretical physics #Thermodynamics #hep-th
paper · pdf · doi:10.1002/prop.200410241
published in Fortschritte der Physik 53(7-8), 919-925 (Wiley) · 7 pages, 2 figures, uses w-art.cls. Talk given by D. K. at the RTN Workshop on the Quantum Structure of Spacetime and the Geometric Nature of Fundamental Interactions and EXT Workshop on Fundamental Interactions and the Structure of Spacetime, Kolymbari, Crete, Greece, 5-10 Sep 2004. To be published in Fortsch.Phys
arxiv created 2004/11/25 · openalex publication_date 2005/06/30 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
Abstract After a brief review of Gödel‐type universes in string theory, we discuss some intriguing properties of black holes immersed in such backgrounds. Among these are the upper bound on the entropy that points towards a finite‐dimensional Hilbert space of a holographically dual theory, and the minimum black hole temperature that is reminiscent of the Hawking‐Page transition. Furthermore, we discuss several difficulties that are encountered when one tries to formulate a consistent thermodynamics of Gödel black holes, and point out how they may be circumvented.