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 that describe not-slowly rotating black holes. For the next-to-leading-order solutions in the expansion, we discuss the physical aspects such as thermodynamics and the phase diagram.
- Received 3 March 2022
- Accepted 24 June 2022
DOI:https://doi.org/10.1103/PhysRevD.106.024018
Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.
Published by the American Physical Society