Deflection of light and time delay in closed Einstein-Straus solution
arXiv:1803.10905 · doi:10.1103/PhysRevD.98.123508
Abstract
We investigate strong lensing by a spherically symmetric mass distribution in the framework of the Einstein-Straus solution with positive cosmological constant and concentrate on the case of a spatially closed Universe (). We develop a method based on integration of differential equations in order to make possible the computation of light deflection and time delay. By applying our results to the lensed quasar SDSS J1004+4112, we find that the bending of light and time delay depend on wether the present value of the scale factor is or is not much smaller than a value close to $9.1 \cdot 10^{26} \mbox{m}$. Beyond this value, the results are almost the same as for the spatially flat Universe. Moreover, it turns out that a positive cosmological constant attenuates the light bending in agreament with Rindler and Ishak's finding.
23 pages, 01 figure and 06 tables
References in corpus (13)
- 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 Rewards of Patience: An 822 Day Time Delay in the Gravitational Lens SDSS J1004+4112
- The role of Lambda in the cosmological lens equation
- Rigorous Approach to the Gravitational Lensing
- A New Independent Limit on the Cosmological Constant/Dark Energy from the Relativistic Bending of Light by Galaxies and Clusters of Galaxies
- Does Cosmological Term Influence Gravitational Lensing?
- Cosmological constant and lensing
- Light Deflection, Lensing, and Time Delays from Gravitational Potentials and Fermat's Principle in the Presence of a Cosmological Constant
- Strong lensing in the Einstein-Straus solution
- Cosmological constant and time delay
- Time delay in the Einstein-Straus solution
- Strong lensing with positive cosmological constant
Cited by in corpus (6)
- Bending of light in novel 4 Gauss-Bonnet-de Sitter black holes by Rindler-Ishak method
- Generalized Gibbons-Werner method for stationary spacetimes
- Light bending by the 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
- Lensing in matched exterior and interior Kottler solutions