Optical ray deflection in the gravitational field of a massive disk

Details Optical ray deflection in the gravitational field of a massive disk Optical ray deflection in the gravitational field of a massive disk

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pazh...15..654m&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 15, July 1989, p. 654-660. In Russian. In Russian. In Russian.

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Computation

Gravitational Fields, Gravitational Lenses, Light Beams, Radiation Sources, Computational Astrophysics, Gravitational Effects, Ray Tracing

Scientific paper

The deflection of optical rays in the gravitational field of a massive disk is considered for different distances between the radiation source and the observer. It is shown that the homogeneous disk functions like an ideal collecting lens only for remote sources at distances greatly exceeding the disk size. If the source is situated close to the disk, the ray trajectories are similar to those in a uniform gravitational field.

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