Observation of gravitational waves by light polarization
arXiv:2012.04243 · doi:10.1140/epjc/s10052-021-08893-4
Abstract
We provide analysis to determine the effects of gravitational waves on electromagnetic waves, using perturbation theory in general relativity. Our analysis is performed in a completely covariant manner without invoking any coordinates. For a given observer, in the geometrical-optics approximation, we work out the perturbations of the phase, amplitude, frequency and polarization properties--axes of ellipse and ellipticity of light, due to gravitational waves. With regard to the observation of gravitational waves, we discuss the measurement of Stokes parameters, through which the antenna patterns are presented to show the detectability of the gravitational wave signals.
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Cited by in corpus (4)
- The Response of Laser Interferometric Gravitational Wave Detectors Beyond the Eikonal Equation
- Observation of Gravitational Waves by Invariants for Electromagnetic Waves
- Gravitational Faraday rotation of light propagation in the Kerr-Newman-Taub-NUT space-time
- Extending the Observational Frequency Range for Gravitational Waves in a Pulsar Timing Array