Constructing black holes in Einstein-Maxwell-scalar theory

Abstract

Exact black hole solutions in the Einstein-Maxwell-scalar theory are constructed. They are the extensions of dilaton black holes in de Sitter or anti de Sitter universe. As a result, except for a scalar potential, a coupling function between the scalar field and the Maxwell invariant is present. Then the corresponding Smarr formula and the first law of thermodynamics are investigated.

arXiv comment25 pages,8 figures

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• Shadows and weak gravitational lensing by the black hole in Einstein-Maxwell-scalar theory
• Dynamic phase transition of charged dilaton black holes
• Adiabatic accretion onto black holes in Einstein-Maxwell-scalar theory
• Thin accretion disk around black hole in Einstein-Maxwell-scalar theory
• Radiation properties of the accretion disk around a black hole in Einstein-Maxwell-scalar theory
• Slowly rotating black holes in the Einstein-Maxwell-scalar theory
• Extraction of energy from a black hole in Einstein-Maxwell-scalar theory
• Probing Einstein-Maxwell-Scalar Black hole via Thin Accretion Disks and Shadows with EHT Observations of M87* and Sgr A*
• General Framework for the Spontaneous Scalarization of Regular Black Holes
• Quasinormal modes for charged Lifshitz black holes with scalar hair
• Electric and dilatonic fields of a charged massive particle at rest in the field of a charged dilaton black hole
• Causal structure and the geodesics in the hairy extension of the Bertotti-Robinson spacetime
• Constructing higher dimensional exact black holes in Einstein-Maxwell-scalar-theory