General Relativistic Elastic Perturbation Theory and PN J-V Equation

Physics

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After pioneering works by Brumberg and Kopejkin1, Damour, Soffel and Xu2,3,4 (called DSX in the following) laid the foundation for a modern theory of general relativistic celestial mechanics at the first post-Newtonian approximation of Einstein's theory of gravity. This general relativistic DSX-formalism is not complete unless the time evolution of the (mass- and current-) multipole moments of the various astronomical bodies is completely specified2,5 ...

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