Post-post-Newtonian light propagation without integrating the geodesic equations

Details Post-post-Newtonian light propagation without integrating the geodesic equations Post-post-Newtonian light propagation without integrating the geodesic equations

2010-12-24

arxiv.org/abs/1012.5402v3

Proceedings of the Journ\'ees 2010 "Syst\`emes de R\'ef\'erence Spatio-Temporels", N. Capitaine (ed.), Observatoire de Paris,

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

4 pages; better written, new expression for the impact parameter; presented at the Journ\'ees 2010 "Syst\`emes de R\'ef\'erenc

Scientific paper

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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