A New Independent Limit on the Cosmological Constant/Dark Energy from the Relativistic Bending of Light by Galaxies and Clusters of Galaxies
arXiv:0710.4726 · doi:10.1111/j.1365-2966.2008.13468.x
Abstract
We derive new limits on the value of the cosmological constant, , based on the Einstein bending of light by systems where the lens is a distant galaxy or a cluster of galaxies. We use an amended lens equation in which the contribution of to the Einstein deflection angle is taken into account and use observations of Einstein radii around several lens systems. We use in our calculations a Schwarzschild-de Sitter vacuole exactly matched into a Friedmann-Robertson-Walker background and show that a -contribution term appears in the deflection angle within the lens equation. We find that the contribution of the -term to the bending angle is larger than the second-order term for many lens systems. Using these observations of bending angles, we derive new limits on the value of . These limits constitute the best observational upper bound on after cosmological constraints and are only two orders of magnitude away from the value determined by those cosmological constraints.
5 pages, 1 figure, matches version published in MNRAS
References in corpus (6)
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- Report of the Dark Energy Task Force
- Combining Strong and Weak Gravitational Lensing in Abell 1689
- The Contribution of the Cosmological Constant to the Relativistic Bending of Light Revisited
- Solar system effects in Schwarzschild--de Sitter spacetime
- Solar and stellar system tests of the cosmological constant
Cited by in corpus (17)
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- The Vacuole Model: New Terms in the Second Order Deflection of Light
- Newtonian analogue of Schwarzschild de-Sitter spacetime: Influence on the local kinematics in galaxies
- Light bending by the cosmological constant
- Leading-order deflection of particles by a moving Schwarzschild lens with a two-dimensional velocity
- Dark Energy on Astrophysical Scales and Its Detection in the Milky Way
- Total light bending in non-asymptotically flat black hole spacetimes
- Mass decomposition of SLACS lens galaxies in Weyl conformal gravity
- Gravitational Lensing from a Spacetime Perspective
- Strong lensing with positive cosmological constant
- Effect of the spatial curvature on light bending and time delay in curved Einstein-Straus--de Sitter spacetime
- Probing dark fluids and modified gravity with gravitational lensing
- Leading-order gravitational time delay of massive particles by a moving Schwarzschild lens
- Deflection of light and time delay in hyperbolic Einstein-Straus--de Sitter solution
- Deflection and gravitational lensing of null and timelike signals in general asymptotically (anti-)de Sitter spacetimes