2007/07/31 by Manavendra Mahato, Leopoldo A. Pando Zayas, Cesar A. Terrero-Escalante +1
Physics and Astronomy · #Black Holes and Theoretical Physics #High-Energy Particle Collisions Research #Pulsars and Gravitational Waves Research #gr-qc #hep-ph #hep-th
paper · pdf · doi:10.1088/1126-6708/2007/09/083
published as JHEP0709:083,2007 · 34 pages, 7 figures. Version to be published by JHEP
arxiv created 2007/09/19 · openalex publication_date 2007/09/20 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/04
We present numerical evidence for a transition between the Klebanov-Strassler background and a solution describing a black hole in the class of cascading solutions in the chirally restored phase. We also present a number of properties of this solution, including the running of the coupling constant, the viscosity to entropy ratio and the drag force on a quark moving in this background.