The extremal Kerr entropy in higher-derivative gravities
arXiv:2303.13286 · doi:10.1007/JHEP05(2023)219
Abstract
We investigate higher derivative corrections to the extremal Kerr black hole in the context of heterotic string theory with corrections and of a cubic-curvature extension of general relativity. By analyzing the near-horizon extremal geometry of these black holes, we are able to compute the Iyer-Wald entropy as well as the angular momentum via generalized Komar integrals. In the case of the stringy corrections, we obtain the physically relevant relation at order . On the other hand, the cubic theories, which are chosen as Einsteinian cubic gravity plus a new odd-parity density with analogous features, possess special integrability properties that enable us to obtain exact results in the higher-derivative couplings. This allows us to find the relation at arbitrary orders in the couplings and even to study it in a non-perturbative way. We also extend our analysis to the case of the extremal Kerr-(A)dS black hole.
33 pages+appendices, one figure
References in corpus (13)
- Dynamical Chern-Simons Modified Gravity I: Spinning Black Holes in the Slow-Rotation Approximation
- Rotating Black Holes in Dilatonic Einstein-Gauss-Bonnet Theory
- Einsteinian cubic gravity
- Black Hole Microstates and Attractor Without Supersymmetry
- Four-dimensional black holes in Einsteinian cubic gravity
- Aspects of general higher-order gravities
- Entropy function and attractors for AdS black holes
- Komar Integrals in Higher (and Lower) Derivative Gravity
- Corrections to AdS Black Hole Thermodynamics from Higher-Derivative Supergravity
- Slowly rotating black holes in Einsteinian cubic gravity
- Bounce Universe and Black Holes from Critical Einsteinian Cubic Gravity
- Extremal Rotating Black Holes in Einsteinian Cubic Gravity
- Local String Models and Moduli Stabilisation