Asymptotically locally AdS and flat black holes in the presence of an electric field in the Horndeski scenario

Abstract

Asymptotically locally AdS and asymptotically flat black hole solutions are found for a particular case of the Horndeski action. The action contains the Einstein-Hilbert term with a cosmological constant, a real scalar field with a non minimal kinetic coupling given by the Einstein tensor, the minimal kinetic coupling and the Maxwell term. There is no scalar potential. The solution has two integration constants related with the mass and the electric charge. The solution is given for all dimensions. A new class of asymptotically locally flat spherically symmetric black holes is found when the minimal kinetic coupling vanishes and the cosmological constant is present. In this case we get a solution which represents an electric Universe. The electric field at infinity is only supported by $\Lambda$. When the cosmological constant vanishes the black hole is asymptotically flat.

arXiv admin note: text overlap with arXiv:1312.3597

References in corpus (11)

• Resummation of Massive Gravity
• Covariant Galileon
• Generalized Galileons: All scalar models whose curved background extensions maintain second-order field equations and stress tensors
• Imperfect Dark Energy from Kinetic Gravity Braiding
• Black holes with non-minimal derivative coupling
• Quintessence and phantom cosmology with non-minimal derivative coupling
• UV-Protected Inflation
• Unified Dark Matter in Scalar Field Cosmologies
• Fab Four: When John and George play gravitation and cosmology
• Inflationary Cosmology Connecting Dark Energy and Dark Matter
• Interacting dark energy: generic cosmological evolution for two scalar fields

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