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New method for determining the light travel time in static, spherically symmetric spacetimes. Calculation of the terms of order G 3

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Publication:2854162
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DOI10.1088/0264-9381/30/17/175008zbMath1273.83032arXiv1304.3683OpenAlexW3102997643MaRDI QIDQ2854162

B. Linet, Pierre Teyssandier

Publication date: 17 October 2013

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

Full work available at URL: https://arxiv.org/abs/1304.3683



Mathematics Subject Classification ID

Black holes (83C57) Galactic and stellar dynamics (85A05) Equations of motion in general relativity and gravitational theory (83C10) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)


Related Items (2)

Relativistic tidal effects on clock-comparison experiments ⋮ Light propagation in 2PN approximation in the field of one moving monopole II. Boundary value problem




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