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Post-post-Newtonian light propagation without integrating the geodesic equations
Published 24 Dec 2010 in gr-qc and astro-ph.IM | (1012.5402v3)
Abstract: A new derivation of the propagation direction of light is given for a 3-parameter family of static, spherically symmetric space-times within the post-post-Newtonian framework. The emitter and the observer are both located at a finite distance. The case of a ray emitted at infinity is also treated.
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