Quintessence and black holes

Abstract

We present new static spherically-symmetric exact solutions of Einstein equations with the quintessential matter surrounding a black hole charged or not as well as for the case without the black hole. A condition of additivity and linearity in the energy-momentum tensor is introduced, which allows one to get correct limits to the known solutions for the electromagnetic static field implying the relativistic relation between the energy density and pressure, as well as for the extraordinary case of cosmological constant, i.e. de Sitter space. We classify the horizons, which evidently reveal themselves in the static coordinates, and derive the Gibbons-Hawking temperatures. An example of quintessence with the state parameter w=-2/3 is discussed in detail.

11 pages, LaTeX file, 1 eps-figure, discussion and references added

Cited by in corpus (376)

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• Echoes and quasinormal modes of asymmetric black bounces
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• Anisotropic matter and nonlinear electromagnetics black holes
• Schwarzschild-AdS Black Holes with Cloud of Strings and Quintessence: Geodesics, Thermodynamic Topology, and Quasinormal Modes
• Impacts of Perfect Fluid Dark Matter on Spacetime Geometry -- the Exponential Metric
• Quasinormal modes of the Hayward black hole surrounded by quintessence: scalar, electromagnetic and gravitational perturbations
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• Some inequalities among curvature invariants
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• Kiselev Black holes in quantum fluctuation modified gravity
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• Shadows and photon spheres of static black holes embedded in a Dehnen-(1,4,5/2)-type dark matter halo with a quintessential field
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• The spacetime geodesy of perfect fluid spheres
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