Cardy-Verlinde Formula and Achucarro-Ortiz Black Hole

Abstract

In this paper it is shown that the entropy of the black hole horizon in the Achucarro-Ortiz spacetime, which is the most general two-dimensional black hole derived from the three-dimensional rotating BTZ black hole, can be described by the Cardy-Verlinde formula. The latter is supposed to be an entropy formula of conformal field theory in any dimension.

arXiv comment10 pages, LaTeX, v2: minor changes, references added, to appear in Phys. Rev. D

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• Self-Gravitational Corrections to the Cardy-Verlinde Formula of Achucarro-Ortiz Black Hole
• Glassy Phase Transition and Stability in Black Holes
• Self-Gravitational Corrections to the Cardy-Verlinde Formula and the FRW Brane Cosmology in SdS_5 Bulk
• Logarithmic correction to the Cardy-Verlinde formula in Achucarro-Oritz Black Hole
• PV criticality of Achucarro-Ortiz black hole in the presence of higher order quantum and GUP corrections
• Bouncing Cosmologies and Self-Gravitational Corrections
• Cardy-Verlinde Formula of Non-Commutative Schwarzschild Black Hole
• Casimir densities for a spherical brane in Rindler-like spacetimes
• The Self-Gravitational Corrections as the Source for Stiff Matter on the Brane in $SAd{S}_5$ Bulk
• Cardy-Verlinde Formula in Taub-NUT/Bolt-(A)dS space
• A CFT description of the BTZ black hole: topology versus geometry (or thermodynamics versus statistical mechanics
• Self-gravitational corrections to the Cardy-Verlinde formula of charged BTZ black hole
• Cardy-Verlinde formula of Kehagias-Sfetsos black hole
• Bouncing cosmological solutions and their stability
• A note on the Cardy formula and black holes in 3d (massive) bigravity
• Cardy-Verlinde formula for an axially symmetric dilaton-axion black hole