An alternative derivation of the Lense-Thirring drag on the orbit of a test body

dc.creatorIorio, Lorenzo
dc.date1999-08-31
dc.date2001-11-14
dc.date.accessioned2026-07-07T07:56:25Z
dc.date.available2026-07-07T07:56:25Z
dc.descriptionA new strategy in deriving the Lense-Thirring effect, in the weak field and slow motion approximation of general relativity, on the orbital elements of a test body in the field of different central rotating sources exhibiting axial symmetry is presented. The approach adopted in the present work, in the case of a perfectly spherical source, leads for all the Keplerian orbital elements of the freely falling particle to the well known Lense-Thirring equations. The case of a central nonspherical body is also worked out.
dc.descriptionLaTex2e, no figures, no tables, 13 pages, cimento.cls used
dc.identifierhttps://arxiv.org/abs/gr-qc/9908080
dc.identifierhttp://arxiv.org/abs/gr-qc/9908080
dc.identifierNuovo Cim. B116 (2001) 777-789
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/127299
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectGeophysics
dc.subjectSpace Physics
dc.titleAn alternative derivation of the Lense-Thirring drag on the orbit of a test body
dc.typetext

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