Abstract
We discuss the effects of an isolated gravitational lens on the rotation of the plane of polarization of linearly polarized light rays, so-called gravitational Faraday rotation, in metric theories of gravity. By applying the thin-lens approximation, we derive simple expressions for extended, rotating astrophysical systems deflecting electromagnetic radiation from background sources. Higher-order corrections and the case of a Kerr black hole are also considered to show how the rotation of polarization is a purely gravitomagnetic effect. Prospects for future detection of gravitational Faraday rotation are examined.
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Sereno, M. (2005). Detecting gravitomagnetism with rotation of polarization by a gravitational lens. Monthly Notices of the Royal Astronomical Society, 356(1), 381–385. https://doi.org/10.1111/j.1365-2966.2004.08456.x
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