Kimpson, T;
Wu, K;
Zane, S;
(2019)
Spatial dispersion of light rays propagating through a plasma in Kerr spacetime.
Monthly Notices of the Royal Astronomical Society
, Article stz138. 10.1093/mnras/stz138.
(In press).
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Abstract
We investigate the propagation of light through a plasma on a background Kerr spacetime via a Hamiltonian formulation. The behaviour of light when propagating through a vacuum and through a plasma is not the same; the convolution of gravitational and plasma effects gives rise to a dispersion in both space and time. The magnitude of the dispersion is a strong function of both the ray frequency and impact parameter. We discuss implications for the detection of gravitationally bent pulsar beams near the Galactic centre.
Type: | Article |
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Title: | Spatial dispersion of light rays propagating through a plasma in Kerr spacetime |
Open access status: | An open access version is available from UCL Discovery |
DOI: | 10.1093/mnras/stz138 |
Publisher version: | https://doi.org/10.1093/mnras/stz138 |
Language: | English |
Additional information: | This version is the author accepted manuscript. For information on re-use, please refer to the publisher’s terms and conditions. |
Keywords: | gravitation – pulsars – black hole physics |
UCL classification: | UCL UCL > Provost and Vice Provost Offices > UCL BEAMS UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics |
URI: | https://discovery-pp.ucl.ac.uk/id/eprint/10065759 |
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