Earth's rotation in the framework of general relativity: rigid multipole moments

Simple item page
dc.creatorKlioner, S. A.
dc.creatorSoffel, M.
dc.creatorXu, Ch.
dc.creatorWu, X.
dc.date2003-03-17
dc.date.accessioned2026-07-07T02:07:59Z
dc.date.available2026-07-07T02:07:59Z
dc.descriptionA set of equations describing the rotational motion of the Earth relative to the GCRS is formulated in the approximation of rigidly rotating multipoles. The external bodies are supposed to be mass monopoles. The derived set of formulas is supposed to form the theoretical basis for a practical post-Newtonian theory of Earth precession and nutation.
dc.description7 pages, Proceeding of Les Journees, ed. N. Capitain, Paris Observatory
dc.identifierhttps://arxiv.org/abs/astro-ph/0303377
dc.identifierhttp://arxiv.org/abs/astro-ph/0303377
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5882
dc.subjectAstrophysics
dc.titleEarth's rotation in the framework of general relativity: rigid multipole moments
dc.typetext

Files

Collections

arXiv