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

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.

arXiv comment16 pages, journal accepted version

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Cited by in corpus (3)

• On non-degeneracy of Riemannian Schwarzschild-anti de Sitter metrics
• Non-degeneracy of Riemannian Schwarzschild-anti de Sitter metrics: Birkhoff-type results in linearized gravity
• On periodic solutions of nonlinear wave equations, including Einstein equations with a negative cosmological constant