Astrometry in the Kerr field in PPN approximation

Details Astrometry in the Kerr field in PPN approximation Astrometry in the Kerr field in PPN approximation

Apr 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.214...71p&link_type=abstract

Astrophysics and Space Science, Vol. 214, No. 1-2, Proceedings of the second United Nations/European Space Agency Workshop, Bogo

Astronomy and Astrophysics

Astrophysics

1

Astrometry, Gravitational Lenses, Relativistic Effects, Solar Gravitation, Beams (Radiation), Deflection, Optical Measurement, Time Lag

Scientific paper

The equation of motion written down using a metric obtained from the Kerr metric allows us to get both the deflection angle of light ray bending by the gravitational field of the Sun and its corresponding time delay. We reproduce the experimental data of Epstein-Shapiro and also it is in accordance with the theoretical results obtained by Brumberg et al. (1990) using another approach to this problem.

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