The second post-Newtonian light propagation and its astrometric measurement in the solar system
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Publication:2946270
DOI10.1142/S021827181550056XzbMath1320.83020arXiv1504.04084OpenAlexW2155659415MaRDI QIDQ2946270
Publication date: 16 September 2015
Published in: International Journal of Modern Physics D (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1504.04084
Observational and experimental questions in relativity and gravitational theory (83B05) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)
Related Items (7)
Uniqueness of First Order Post-Newtonian Collinear Solutions for Three-Body Problem under a Scalar-Tensor Theory ⋮ Light propagation in 2PN approximation in the field of one moving monopole I. Initial value problem ⋮ Post-Minkowskian solution for the small-deflection motion of test particles in Kerr–Newman spacetime ⋮ Weak deflection angle by Casimir wormhole using Gauss-Bonnet theorem and its shadow ⋮ Light propagation in 2PN approximation in the field of one moving monopole II. Boundary value problem ⋮ Parameterized Post-Post-Newtonian Light Propagation in the Field of One Spherically-Symmetric Body* ⋮ Weak and strong deflection gravitational lensings by a charged Horndeski black hole
Cites Work
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- Scalar–tensor propagation of light in the inner solar system including relevant c −4 contributions for ranging and time transfer
- The laser astrometric test of relativity mission
- World function and time transfer: general post-Minkowskian expansions
- A SEARCH FOR NEW PHYSICS WITH THE BEACON MISSION
- General post-Minkowskian expansion of time transfer functions
- Numerical versus analytical accuracy of the formulae for light propagation
- Time transfer functions as a way to validate light propagation solutions for space astrometry
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