Einstein-Maxwell gravity coupled to a scalar field in 2+1-dimensions

Abstract

We consider Einstein-Maxwell-self-interacting scalar field theory described by a potential $V\left(\varphi \right)$ in $2+1-$dimensions. The self-interaction potential is chosen to be a highly non-linear double-Liouville type. Exact solutions, including chargeless black holes and singularity-free non-black hole solutions are obtained in this model.

6 pages, one figure, final copy accepted for publication in The European Physical Journal - Plus

References in corpus (4)

• Casimir piston for massless scalar fields in three dimensions
• Thermodynamics of rotating black holes with scalar hair in three dimensions
• Exact radial solution in 2+1 gravity with a real scalar field
• Double-bounce domain-wall in Einstein-Yang-Mills-Scalar black holes

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• On a Particular Thin-shell Wormhole
• Cloud of strings as source in $2+1$-dimensional $f(R)=R^n$ gravity
• Quasinormal modes of charged BTZ black holes
• Thin-shell wormholes in 2+1-dimensional Einstein-Scalar Theory