Non-singular spacetimes with a negative cosmological constant: IV. Stationary black hole solutions with matter fields
General Relativity and Quantum Cosmology
2017-12-13 v2 High Energy Physics - Theory
Differential Geometry
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- equations with a negative cosmological constant. The families include an infinite-dimensional family of solutions with the usual AdS conformal structure at conformal infinity.
Keywords
Cite
@article{arxiv.1708.04947,
title = {Non-singular spacetimes with a negative cosmological constant: IV. Stationary black hole solutions with matter fields},
author = {Piotr T. Chruściel and Erwann Delay and Paul Klinger},
journal= {arXiv preprint arXiv:1708.04947},
year = {2017}
}
Comments
16 pages, journal accepted version