Time Delay in Swiss Cheese Gravitational Lensing
arXiv:1006.3500 · doi:10.1103/PhysRevD.82.043005
Abstract
We compute time delays for gravitational lensing in a flat LambdaCDM Swiss cheese universe. We assume a primary and secondary pair of light rays are deflected by a single point mass condensation described by a Kottler metric (Schwarzschild with Lambda) embedded in an otherwise homogeneous cosmology. We find that the cosmological constant's effect on the difference in arrival times is non-linear and at most around 0.002% for a large cluster lens; however, we find differences from time delays predicted by conventional linear lensing theory that can reach ~4% for these large lenses. The differences in predicted delay times are due to the failure of conventional lensing to incorporate the lensing mass into the mean mass density of the universe.
10 pages, 2 figures, submitted
References in corpus (7)
- The Contribution of the Cosmological Constant to the Relativistic Bending of Light Revisited
- On the influence of the cosmological constant on gravitational lensing in small systems
- The role of Lambda in the cosmological lens equation
- Cosmological constant and lensing
- Light Deflection, Lensing, and Time Delays from Gravitational Potentials and Fermat's Principle in the Presence of a Cosmological Constant
- Cosmological constant and time delay
- Gravitational Lensing Corrections in Flat LambdaCDM Cosmology
Cited by in corpus (12)
- Bending of light in novel 4 Gauss-Bonnet-de Sitter black holes by Rindler-Ishak method
- Influences of Dark Energy and dark matter on Gravitational Time Advancement
- Large-Distance Lens Uncertainties and Time-Delay Measurements of
- Deflection of light and time delay in closed Einstein-Straus solution
- The Gravitational Lens Equation for Embedded Lenses; Magnification and Ellipticity
- The Embedded Transparent Lens and Fermat's Least-Time Principle
- Image Properties of Embedded Lenses
- Dynamic Black Holes in a FRW background: Lemaitre transformations
- A Simple Gravitational Lens Model For Cosmic Voids
- An integrated Sachs-Wolfe effect vs redshift test for the cosmological parameters
- Effect of the spatial curvature on light bending and time delay in curved Einstein-Straus--de Sitter spacetime
- Probing the integrated Sachs-Wolfe effect using embedded lens models