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Phys. Rev. D 26, 2549–2556 (1982)

Second-order contributions to gravitational deflection of light in the parametrized post-Newtonian formalism. II. Photon orbits and deflections in three dimensions

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Gary W. Richter
Center for Relativity, University of Texas, Austin, Texas 78712

Richard A. Matzner*
Department of Astrophysics, South Parks Road, Oxford, United Kingdom

Received 27 May 1982; published in the issue dated 15 November 1982

Using a parametrized expansion of the solar metric to second order in the Newtonian potential we calculate the trajectories of photons scattered by the Sun. In general the photon is scattered in two directions orthogonal to its initial momentum because of the anisotropic features of the solar field. We calculate both components of the deflection as measured by an observer within the solar field.

© 1982 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.26.2549
DOI:
10.1103/PhysRevD.26.2549
PACS:

*On leave from Center for Relativity, University of Texas, Austin, TX 78712.