arXiv · hep-th/0210252
Holographic Thermodynamic on the Brane in Topological Reissner-Nordström de Sitter Space
Abstract
We consider the brane universe in the bulk background of the topological Reissner-Nordström de Sitter black holes. We show that the thermodynamic quantities (including entropy) of the dual CFT take usual special forms expressed in terms of Hubble parameter and its time derivative at the moment, when the brane crosses the black hole horizon or the cosmological horizon. We obtain the generalized Cardy-Verlinde formula for the CFT with an charge and cosmological constant, for any values of the curvature parameter $k$ in the Friedmann equations.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
M. R. Setare, R. Mansouri. 2002-10-26. Holographic Thermodynamic on the Brane in Topological Reissner-Nordström de Sitter Space. https://doi.org/10.1142/s0217751x0301512x
Cite the original work for its findings. Save a collection to share your selection of sources.