Precession of Pericenter: A More Accurate Approach

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dc.creatorStergiou, Andreas
dc.date2006-10-31
dc.date.accessioned2026-07-07T07:28:04Z
dc.date.available2026-07-07T07:28:04Z
dc.descriptionIn this paper we study the orbits of massive bodies moving in the spacetime generated by a spherically symmetric and non-rotating distribution of mass. More specifically, our treatment discusses the more accurate calculation of the precession of pericenter due to general-relativistic effects. Our result is accurate up to terms of second order, while the precession met in the bibliography is accurate only up to first-order terms.
dc.description7 pages, 1 figure, BSc thesis result
dc.identifierhttps://arxiv.org/abs/gr-qc/0610158
dc.identifierhttp://arxiv.org/abs/gr-qc/0610158
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/117599
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titlePrecession of Pericenter: A More Accurate Approach
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