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

Piotr T. Chruściel (1) , Erwann Delay (2) , Paul Klinger (1)

1 Universität Wien = University of Vienna
2 AU - Avignon Université

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.

Domaines: Relativité Générale et Cosmologie Quantique [gr-qc]; Géométrie différentielle [math.DG]

Piotr T. Chruściel, Erwann Delay, Paul Klinger. Non-singular spacetimes with a negative cosmological constant: IV. Stationary black hole solutions with matter fields. 2017. ⟨hal-01581652⟩