Equations of motion according to the asymptotic post-Newtonian scheme for general relativity

dc.creatorArminjon, Mayeul
dc.date2005-10-07
dc.date.accessioned2026-07-07T08:43:27Z
dc.date.available2026-07-07T08:43:27Z
dc.descriptionWe summarize a recent work done on the title's subject. First, we present the asymptotic scheme of post-Newtonian (PN) approximation for general relativity in the harmonic gauge. Then, we discuss the definition of the mass centers and the derivation of equations for their motion, following that scheme. Finally, we briefly analyze the reason why a new term has thus been found in the equations of motion.
dc.description8 pages, no figure. Text of talks given at the 3rd Workshop "Gravity, Astrophysics and Strings at the Black Sea" (Kiten, Bulgaria, June 13-20, 2005). Submitted to the Proceedings (P. Fiziev and M. Todorov, eds.)
dc.identifierhttps://arxiv.org/abs/gr-qc/0510026
dc.identifierhttp://arxiv.org/abs/gr-qc/0510026
dc.identifierGravity, Astrophysics and Strings at the Black Sea (P. Fiziev & M. Todorov, eds.), St. Kliment Ohridski University Press, Sofia (2006), pp. 1-9
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/142322
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titleEquations of motion according to the asymptotic post-Newtonian scheme for general relativity
dc.typetext

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