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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.
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P.T. Chruściel, On analyticity of static vacuum metrics at non-degenerate horizons , Acta Phys. Pol. B36
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P.T. Chruściel and E. Delay, Non-singular, vacuum, stationary space-times with a negative cosmological constant , Ann. Henri Poincaré 8
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R. Beig and P.T. Chruściel, On analyticity of stationary vacuum metrics at non-degenerate Killing horizons , in preparation
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2016
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2016
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P.T. Chruściel, E. Delay, and P. Klinger, Non-singular spacetimes with a negative cosmological constant: III. Stationary solutions with matter fields , (2017)
2017
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2017
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P.T. Chruściel, E. Delay, P. Klinger, A. Kriegl, P.W. Michor, and A. Rainer, Non-singular spacetimes with a negative cosmological constant: V. Boson stars , (2017)
2017
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