Black Holes in Cascading Theories: Confinement/Deconfinement Transition and other Thermal Properties
arXiv:0707.2737 · doi:10.1088/1126-6708/2007/09/083
Abstract
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.
34 pages, 7 figures. Version to be published by JHEP