Dark Energy Accretion onto black holes in a cosmic scenario
arXiv:0803.2005 · doi:10.1007/s10714-009-0808-8
Abstract
In this paper we study the accretion of dark energy onto a black hole in the cases that dark energy is equipped with a positive cosmological constant and when the space-time is described by a Schwarzschild-de Sitter metric. It is shown that, if confronted with current observational data, the results derived when no cosmological constant is present are once again obtained in both cases.
7 pages, 3 figures
References in corpus (9)
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- The final state and thermodynamics of dark energy universe
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Cited by in corpus (11)
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- Thermodynamics in Closed Universe with Entropy Corrections
- Evolving Black Holes in Inflation
- Accretion of nonminimally coupled scalar fields into black holes
- Adiabatic accretion onto black holes in Einstein-Maxwell-scalar theory
- Deforming regular black holes
- Isotropic extensions of the vacuum solutions in general relativity
- Black hole in a generalized Chaplygin-Jacobi dark fluid: shadow and light deflection angle
- Fate of an Accretion Disc around a Black Hole when both the Viscosity and Dark Energy is Effecting
- On accretion of dark energy onto black- and worm-holes
- Interaction of a black hole with scalar field in cosmology background