Cosmological constant and lensing
arXiv:0712.1559 · doi:10.1007/s10714-008-0652-2
Abstract
The effect of the cosmological constant on the curvature of light due to an isolated spherical mass is recalculated without using the lens equation and compared to a lensing cluster.
9 pages,4 figures
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Cited by in corpus (28)
- The Relevance of the Cosmological Constant for Lensing
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- Gravitational deflection of light in the Schwarzschild -de Sitter space time
- Geometrization of light bending and its application to SdSw spacetime
- More on Lensing by a Cosmological Constant
- Direct Probe of Dark Energy through Gravitational Lensing Effect
- Strong gravitational lensing and black hole quasinormal modes: Towards a semiclassical unified description
- Strong lensing in the Einstein-Straus solution
- Light bending in the galactic halo by Rindler-Ishak method
- Beyond lensing by the cosmological constant
- The Cosmological Constant and the Gravitational Light Bending
- Gravitational Lensing in Weyl Gravity
- Gravitational Lensing Corrections in Flat LambdaCDM Cosmology
- Lambda does not Lens: Deflection of Light in the Schwarzschild-de Sitter Spacetime
- Lensing in an interior Kottler solution
- Time Delay in Swiss Cheese Gravitational Lensing
- On the effect of the cosmological expansion on the gravitational lensing by a point mass
- Effect of a positive cosmological constant on cosmic strings
- Cosmological applications of the Brown-York quasilocal mass
- Time delay in the Einstein-Straus solution
- Deflection of light and time delay in closed Einstein-Straus solution
- The Embedded Transparent Lens and Fermat's Least-Time Principle
- Light bending, static dark energy and related uniqueness of Schwarzschild-de Sitter spacetime
- The Gravitational Lens Equation for Embedded Lenses; Magnification and Ellipticity
- Image Properties of Embedded Lenses
- Strong lensing with positive cosmological constant
- Effect of the spatial curvature on light bending and time delay in curved Einstein-Straus--de Sitter spacetime
- Deflection of light and time delay in hyperbolic Einstein-Straus--de Sitter solution