Rotating black holes at large in Einstein-Gauss-Bonnet theory
arXiv:2202.12649 · doi:10.1103/PhysRevD.106.024018
Abstract
Applying the large approach to the Einstein-Gauss-Bonnet theory, we construct equally rotating black hole solutions in odd dimensions. This provides the first example of the analytic solutions which describes not-slowly rotating black holes. For the next-leading order solutions in the expansion, we discuss the physical aspects such as thermodynamics and the phase diagram.
arXiv comment5 pages, 1 figure
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