Gravitational red-shift and deflection of slow light
arXiv:0810.4849 · doi:10.1103/PhysRevA.79.013834
Abstract
We explore the nature of the classical propagation of light through media with strong frequency-dependent dispersion in the presence of a gravitational field. In the weak field limit, gravity causes a redshift of the optical frequency, which the slow-light medium converts into a spatially-varying index of refraction. This results in the bending of a light ray in the medium. We further propose experimental techniques to amplify and detect the phenomenon using weak value measurements. Independent heuristic and rigorous derivations of this effect are given.
9 pages, 1 figure
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- Weak values and the Leggett-Garg inequality in solid-state qubits
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Cited by in corpus (5)
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- Gravitational lensing in a non-uniform plasma
- Gravitational and Relativistic Deflection of X-Ray Superradiance
- Slow light in flight imaging
- Planck scale displacement of a connected mirror pair: an energy measurement in a gravitational field