Numerical Methods for Finding Stationary Gravitational Solutions
arXiv:1510.02804 · doi:10.1088/0264-9381/33/13/133001
Abstract
The wide applications of higher dimensional gravity and gauge/gravity duality have fuelled the search for new stationary solutions of the Einstein equation (possibly coupled to matter). In this topical review, we explain the mathematical foundations and give a practical guide for the numerical solution of gravitational boundary value problems. We present these methods by way of example: resolving asymptotically flat black rings, singly-spinning lumpy black holes in anti-de Sitter (AdS), and the Gregory-Laflamme zero modes of small rotating black holes in AdS. We also include several tools and tricks that have been useful throughout the literature.
Invited Topical Review for Classical and Quantum Gravity, 153 pages, 11 figures
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