Gravitational frequency shift of light in equatorial plane of a radially moving Schwarzschild black hole
arXiv:2007.08118 · doi:10.1093/mnras/stx1539
Abstract
The kinematical effect induced by the transversal motion of a gravitational lens on the frequency shift of light has been investigated in detail, while the effect of the radial motion is thought to be much smaller than the transversal one and thus has usually been neglected. In this work, we find that the radial velocity effect on the frequency shift has the same order of magnitude as that of the transversal velocity effect, when the light emitter (or the receiver) is close to the gravitational lens with the distance between them being an impact parameter scale. The significant velocity effect is usually transient due to the motion of the gravitational lens relative to the light emitter or the receiver.
References in corpus (8)
- Lorentz Covariant Theory of Light Propagation in Gravitational Fields of Arbitrary-Moving Bodies
- Null Geodesics in Perturbed Spacetimes
- Deflection of light and particles by moving gravitational lenses
- Determining Tangential Peculiar Velocities of Clusters of Galaxies using Gravitational Lensing
- Second-order time delay by a radially moving Kerr-Newman black hole
- Tangential Velocity of the Dark Matter in the Bullet Cluster from Precise Lensed Image Redshifts
- Lyman alpha absorbers in motion: consequences of gravitational lensing for the cosmological redshift drift experiment
- Effects of Lens Motion and Uneven Magnification on Image Spectra