Non-singular spacetimes with a negative cosmological constant: IV. Stationary black hole solutions with matter fields - Avignon Université Access content directly
Preprints, Working Papers, ... Year : 2017

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.

Dates and versions

hal-01581652 , version 1 (04-09-2017)

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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⟩

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UNIV-AVIGNON INSMI
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