Gravoelectromagnetic approach to the gravitational Faraday rotation in stationary spacetimes
arXiv:gr-qc/9901011 · doi:10.1103/PhysRevD.60.024013
Abstract
Using the 1+3 formulation of stationary spacetimes we show, in the context of gravoelectromagnetism, that the plane of the polarization of light rays passing close to a black hole undergoes a rotation. We show that this rotation has the same integral form as the usual Faraday effect, i.e. it is proportional to the integral of the component of the gravomagnetic field along the propagation path. We apply this integral formula to calculate the Faraday rotation induced by the Kerr and NUT spaces using the quasi-Maxwell form of the vacuum Einstein equations.
13 pages including one figure. Latex. Section 6 has been removed and included in the conclusion section. Some typos has been corrected and new reference has been added
References in corpus (1)
Cited by in corpus (41)
- Polarized Image of Equatorial Emission in the Kerr Geometry
- Gravito-electromagnetic analogies
- Testing strong gravitational lensing effects by supermassive compact objects with regular spacetimes
- Spinoptics in a stationary spacetime
- Gravitational Faraday rotation in a weak gravitational field
- Gravitational lensing by stars with angular momentum
- Gravitational Faraday effect from on-shell amplitudes
- Maxwell equations in a curved spacetime: Spin optics approximation
- Photon polarization and geometric phase in general relativity
- Post-Newtonian gravitational effects in quantum interferometry
- Notes on Spinoptics in a Stationary Spacetime
- Detecting gravito-magnetism with rotation of polarization by a gravitational lens
- Gravitational Faraday rotation of gravitational waves by a Kerr black hole
- Polarization rotation, reference frames and Mach's principle
- Gravitational Faraday and Spin-Hall Effects of Light
- Rotation of the cosmic microwave background polarization from weak gravitational lensing
- Separability of Rotational Effects on a Gravitational Lens
- Evolution of polarization orientations in a flat universe with vector perturbations: CMB and quasistellar objects
- Massless polarized particle and Faraday rotation of light in the Schwarzschild spacetime
- Quantum corrections to frame-dragging in scattering amplitudes
- Spin Hall effects in the sky
- Electromagnetic waves in a wormhole geometry
- Spin wave optics for gravitational waves lensed by a Kerr black hole
- Gravitational analog of Faraday rotation in the magnetized Kerr and Reissner-Nordström spacetimes
- On spin optics for gravitational waves lensed by a rotating object
- Gravitational Larmor precession
- Gravitational Faraday Rotation in Binary Pulsar Systems
- General relativistic analogs of Poisson's equation and gravitational binding energy
- Gauged motion in general relativity and in Kaluza-Klein theories
- Fiber optics in curved space-times
- Gravitational Lensing from a Spacetime Perspective
- An overview of the gravitational spin Hall effect
- Papapetrou field as the gravitoelectromagnetic field tensor in stationary spacetimes
- Static and stationary dark fluid universes: A gravitoelectromagnetic perspective
- Gravitational Faraday rotation of light propagation in the Kerr-Newman-Taub-NUT space-time
- Polarization rotation and near-Earth quantum communications
- An angular rainbow of light from curved spacetime
- Light rays in the Solar system experiments: phases and displacements
- Achromatic, spin-odd Kerr EVPA as a null Frenet-Serret torsion integral on the photon ring
- Observables for the Effect of Gravity on Electromagnetic Polarization
- Sensing Gravity with Polarized Electromagnetic Radiation