One-Loop Corrected Thermodynamics of the Extremal and Non-Extremal Spinning BTZ Black Hole
arXiv:hep-th/0009050 · doi:10.1103/PhysRevD.63.104005
Abstract
We consider the one-loop corrected geometry and thermodynamics of a rotating BTZ black hole by way of a dimensionally reduced dilaton model. The analysis begins with a comprehensive study of the non-extremal solution after which two different methods are invoked to study the extremal case. The first approach considers the extremal limit of the non-extremal calculations, whereas the second treatment is based on the following conjecture: extremal and non-extremal black holes ae qualitatively distinct entities. We show that only the latter method yields regularity and consistency at the one-loop level. This is suggestive of a generalized third law of thermodynamics that forbids continuous evolution from non-extremal to extremal black hole geometries.
26 pages, Latex, some new references added
References in corpus (6)
- Nonthermal nature of incipient extremal black holes
- The Dimensional-Reduction Anomaly
- Two-dimensional effective action for matter fields coupled to the dilaton
- Evidence for a null entropy of extremal black holes
- Quantum corrections for the Reisner-Nordstrom black hole
- The Dimensional-Reduction Anomaly in Spherically Symmetric Spacetimes
Cited by in corpus (39)
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