Scalar–tensor propagation of light in the inner solar system including relevant c −4 contributions for ranging and time transfer

DOI10.1088/0264-9381/28/8/085010zbMath1216.83044arXiv1007.3942OpenAlexW3104955951WikidataQ61645707 ScholiaQ61645707MaRDI QIDQ3000814

Bertrand Chauvineau, Olivier Minazzoli

Publication date: 31 May 2011

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1007.3942

Mathematics Subject Classification ID

Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Observational and experimental questions in relativity and gravitational theory (83B05) Galactic and stellar dynamics (85A05) Equations of motion in general relativity and gravitational theory (83C10)

Related Items (3)

The second post-Newtonian light propagation and its astrometric measurement in the solar system ⋮ Light propagation in 2PN approximation in the field of one moving monopole I. Initial value problem ⋮ Light propagation in 2PN approximation in the field of one moving monopole II. Boundary value problem

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