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The second post-Newtonian light propagation and its astrometric measurement in the Solar System: Light time and frequency shift

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Publication:2818115
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DOI10.1142/S0218271816500826zbMath1344.83009MaRDI QIDQ2818115

Xue-Mei Deng

Publication date: 6 September 2016

Published in: International Journal of Modern Physics D (Search for Journal in Brave)


zbMATH Keywords

relativityastrometryreference systems


Mathematics Subject Classification ID

Observational and experimental questions in relativity and gravitational theory (83B05) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)


Related Items (4)

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 ⋮ 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

  • Relativistic Celestial Mechanics of the Solar System
  • Solar System Dynamics
  • Unnamed Item


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