Post-post-Newtonian Amendments for Radar Echo Delay Test in the Reissner-Nordström Field

Details Post-post-Newtonian Amendments for Radar Echo Delay Test in the Reissner-Nordström Field Post-post-Newtonian Amendments for Radar Echo Delay Test in the Reissner-Nordström Field

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010acasn..51....1g&link_type=abstract

Acta Astronomica Sinica, vol. 51, no. 1, p. 1-7

Astronomy and Astrophysics

Astronomy

Gravitation, Sun, Earth, Waves, Methods: Analytical

Scientific paper

From the kinetic differential equations of the photon in the equatorial plane of the spherical symmetrical gravity field, the post-post-Newtonian amendments for radar echo delay test in the Reissner-Nordström field are discussed using the post-Newtonian approximation method. The amendatory results of post-Newtonian order and post-post-Newtonian order are deduced in this paper. When the charge Q is equal to zero, the results are applicable to neutral celestial objects. The post-Newtonian amendatory parts are consistent with the classical literature. The approximation method used in this paper can also be used to discuss the amendments with higher orders. The high-order amendments for radar echo delay test have important significances to the ongoing high-precision spatial gravitation test.

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