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arXiv · 1708.04947

Non-singular spacetimes with a negative cosmological constant: IV. Stationary black hole solutions with matter fields

Piotr T. Chruściel·Erwann Delay·Paul Klinger
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Abstract

We use an elliptic system of equations with complex coefficients for a set of complex-valued tensor fields as a tool to construct infinite-dimensional families of non-singular stationary black holes, real-valued Lorentzian solutions of the Einstein-Maxwell-dilaton-scalar fields-Yang-Mills-Higgs-Chern-Simons-$f(R)$ equations with a negative cosmological constant. The families include an infinite-dimensional family of solutions with the usual AdS conformal structure at conformal infinity.

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Piotr T. Chruściel, Erwann Delay, Paul Klinger. 2017-12-12. Non-singular spacetimes with a negative cosmological constant: IV. Stationary black hole solutions with matter fields. https://doi.org/10.1088/1361-6382%2Faa9e0c

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