Light bending in the galactic halo by Rindler-Ishak method
arXiv:0910.1112 · doi:10.1088/1475-7516/2010/09/004
Abstract
After the work of Rindler and Ishak, it is now well established that the bending of light is influenced by the cosmological constant Λ appearing in the Schwarzschild-de Sitter spacetime. We show that their method, when applied to the galactic halo gravity parametrized by a constant γ, yields exactly the same γ- correction to Schwarzschild bending as obtained by standard methods. Different cases are analyzed, which include some corrections to the special cases considered in the original paper by Rindler and Ishak.
arXiv comment15 pages
References in corpus (14)
- 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
- Classical tests for Weyl gravity: deflection of light and time delay
- The role of Lambda in the cosmological lens equation
- Rigorous Approach to the Gravitational Lensing
- The Relevance of the Cosmological Constant for Lensing
- A New Independent Limit on the Cosmological Constant/Dark Energy from the Relativistic Bending of Light by Galaxies and Clusters of Galaxies
- On lensing by a cosmological constant
- More on Lensing by a Cosmological Constant
- Does Cosmological Term Influence Gravitational Lensing?
- Cosmological constant and lensing
- Light deflection in Weyl gravity: constraints on the linear parameter
- Strong lensing in the Einstein-Straus solution
- Gravitational Lensing Corrections in Flat LambdaCDM Cosmology
Cited by in corpus (21)
- Gravitoelectromagnetism, Solar System Test and Weak-Field Solutions in Gravity with Observational Constraints
- Bending of light in novel 4 Gauss-Bonnet-de Sitter black holes by Rindler-Ishak method
- Probing the Lorentz Invariance Violation via Gravitational Lensing and Analytical Eigenmodes of Perturbed Slowly Rotating Bumblebee Black Holes
- Geodesic equations in the static and rotating dilaton black holes: Analytical solutions and applications
- Strong field lensing by Damour-Solodukhin wormhole
- Detailed study of geodesics in the Kerr-Newman-(A)dS spactime and the rotating charged black hole spacetime in gravity
- Determination of Angle of Light Deflection in Higher-Derivative Gravity Theories
- Gravitational Lensing in Weyl Gravity
- The Vacuole Model: New Terms in the Second Order Deflection of Light
- Determination of Bending Angle of Light Deflection Subject to Possible Weak and Strong Quantum Gravity Effects
- On the Null Trajectories in Conformal Weyl Gravity
- Gravitational Lensing in Kerr-Newman Anti de Sitter Spacetime
- Linear Weyl Gravity in de Sitter Universe
- Exploring light deflection and black hole shadows in Rastall theory with plasma effects
- Constraint on dark matter central density in the Eddington inspired Born-Infeld (EiBI) gravity with input from Weyl gravity
- Analytical solutions of the geodesic equation in the space-time of a black hole surrounded by perfect fluid in Rastall theory
- Gravitational lens on a static optical constant-curvature background: Its application to Weyl gravity model
- Total light bending in non-asymptotically flat black hole spacetimes
- Sagnac delay in the Kerr-dS space-time: Implications for Mach's principle
- Mass decomposition of SLACS lens galaxies in Weyl conformal gravity
- Test of conformal theory of gravity as an alternative paradigm to dark matter hypothesis from gravitational lensing studies