Scattering of circularly polarized light by a rotating black hole
We study scattering of polarized light by a rotating (Kerr) black hole of mass M and angular momentum J. In order to keep trace of the polarization dependence of photon trajectories one can use the following dimensionless parameter: epsilon = + or -( omega M) super(-1), where omega is the photon fre...
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Veröffentlicht in: | Physical review. D, Particles, fields, gravitation, and cosmology Particles, fields, gravitation, and cosmology, 2012-07, Vol.86 (2), Article 024010 |
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Hauptverfasser: | , |
Format: | Artikel |
Sprache: | eng |
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Online-Zugang: | Volltext |
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Zusammenfassung: | We study scattering of polarized light by a rotating (Kerr) black hole of mass M and angular momentum J. In order to keep trace of the polarization dependence of photon trajectories one can use the following dimensionless parameter: epsilon = + or -( omega M) super(-1), where omega is the photon frequency and the sign + (-) corresponds to the right (left) circular polarization. We assume that epsilon |
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ISSN: | 1550-7998 1550-2368 |
DOI: | 10.1103/PhysRevD.86.024010 |