On the Entropy of Four-Dimensional Near-Extremal N=2 Black Holes with R^2-Terms
arXiv:0708.2554 · doi:10.1088/1126-6708/2007/12/050
Abstract
We consider the entropy of four-dimensional near-extremal N=2 black holes. Without R^2-terms, the Bekenstein-Hawking entropy formula has the structure of the extremal black holes entropy with a shift of the charges depending on the non-extremality parameter and the moduli at infinity. We derive a generalized Wald entropy formula for non-extremal N=2 black holes with R^2-terms. We construct a class of small near-extremal horizon solutions with R^2-terms. In this case the entropy is the same as in the extremal case to order O(mu^2), and does not exhibit the charge shift behavior.
20 pages. v2: appendix added. references added. minor fixes. v3: minor comments. up to date with JHEP version. v4: significant revision, fixed error in main result (shift in entropy should vanish), fixed equations of motion (not affecting other results). v5: fixed abstract and references
References in corpus (7)
- Black Hole Microstates and Attractor Without Supersymmetry
- Higher Derivative Corrections to Non-supersymmetric Extremal Black Holes in N=2 Supergravity
- Lectures on on Black Holes, Topological Strings and Quantum Attractors (2.0)
- Non-Supersymmetric Attractors and Entropy Function
- BPS Black Holes
- Non-Supersymmetric Attractors in Gravities
- Supersymmetric black holes in string theory
Cited by in corpus (7)
- The Phase Structure of Higher-Dimensional Black Rings and Black Holes
- Geometric Engineering 5d Black Holes with Rod Diagrams
- Caged black hole thermodynamics: Charge, the extremal limit, and finite size effects
- On the off-shell formulation of N=2 supergravity with tensor multiplets
- Large Charge Four-Dimensional Extremal N=2 Black Holes with R^2-Terms
- Supergravity on an Atiyah-Hitchin Base
- Large Charge Four-Dimensional Non-Extremal N=2 Black Holes with R^2-Terms