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Cardy-verlinde formula and asymptotically flat rotating charged black holes (202).
| Content Provider | CiteSeerX |
|---|---|
| Author | Jing, Jiliang |
| Abstract | The Cardy-Verlinde formula is generalized to the asymptotically flat rotating charged black holes in the Einstein-Maxwell theory and low-energy effective field theory describing string by using some typical spacetimes, such as the Kerr-Newman, Einstein-Maxwell-dilaton-axion, Kaluza-Klein, and Sen black holes. For the Kerr-Newman black hole, the definition of the Casimir energy takes the same form as that of the Kerr-Newman-AdS4 and Kerr-Newman-dS4 black holes, while the Cardy-Verlinde formula possesses different from since the Casimir energy does not appear in the extensive energy. The Einstein-Maxwell-dilaton-axion, Kaluza-Klein, and Sen black holes have special property: The definition of the Casimir energy for these black holes is similar to that of the Kerr-Newman black hole, but the Cardy-Verlinde formula takes the same form as that of the Kerr black hole. |
| File Format | |
| Access Restriction | Open |
| Subject Keyword | Cardy-verlinde Formula Casimir Energy Kerr-newman Black Hole Sen Black Hole Cardy-verlinde Formula Posse Typical Spacetimes Einstein-maxwell Theory Kerr-newman-ds4 Black Hole Low-energy Effective Field Theory Special Property Kerr Black Hole Extensive Energy |
| Content Type | Text |