Aberration by gravitational lenses in motion
arXiv:astro-ph/0311189 · doi:10.1046/j.1365-8711.2003.07095.x
Abstract
It is known that a fully relativistic integration of the null geodesics of a weak perturbation of flat spacetime leads to a correction of order to the bending angle and time delay due to a gravitational lens in slow motion with small acceleration. The existence of the correction was verified by the VLBI experiment of the bending of light by Jupiter on September 8, 2002. Here the correction is interpreted by means of standard aberration of light in an optically active medium with an effective index of refraction induced by the gravitational field of a lens in motion.
3 pages
References in corpus (6)
- Gravitational Microlensing in the Local Group
- Lorentz Covariant Theory of Light Propagation in Gravitational Fields of Arbitrary-Moving Bodies
- The Measurement of the Light Deflection from Jupiter: Experimental Results
- Propagation Speed of Gravity and the Relativistic Time Delay
- Null Geodesics in Perturbed Spacetimes
- On bending angles by gravitational lenses in motion
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- Gravimagnetism, Causality, and Aberration of Gravity in the Gravitational Light-Ray Deflection Experiments
- Aberration and the Fundamental Speed of Gravity in the Jovian Deflection Experiment
- Gravitomagnetism and the Speed of Gravity
- Analytical Derivation of Second-Order Deflection in Equatorial Plane of a Radially Moving Kerr-Newman Black Hole
- Second-order time delay by a radially moving Kerr-Newman black hole
- On gravitational lensing by deflectors in motion
- Light propagation in 2PN approximation in the field of one moving monopole II. Boundary value problem
- On aberration in gravitational lensing
- Kerr-Schild Form of the Exact Metric for a Constantly Moving Kerr Black Hole and Null Gravitational Deflection
- Leading-order gravitational time delay of massive particles by a moving Schwarzschild lens