Deformation of the Planetary Orbits Caused by the Time Dependent Gravitational Potential in the Universe

dc.creatorTrencevski, Kostadin
dc.date2004-03-15
dc.date2004-05-20
dc.date.accessioned2026-07-07T06:30:34Z
dc.date.available2026-07-07T06:30:34Z
dc.descriptionIn the paper are studied the deformations of the planetary orbits caused by the time dependent gravitational potential in the universe. It is shown that the orbits are not axially symmetric and the time dependent potential does not cause perihelion precession. It is found a simple formula for the change of the orbit period caused by the time dependent gravitational potential and it is tested for two binary pulsars.
dc.description7 pages
dc.identifierhttps://arxiv.org/abs/gr-qc/0403067
dc.identifierhttp://arxiv.org/abs/gr-qc/0403067
dc.identifierGen.Rel.Grav. 37 (2005) 507-519
dc.identifierdoi:10.1007/s10714-005-0039-6
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/98374
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleDeformation of the Planetary Orbits Caused by the Time Dependent Gravitational Potential in the Universe
dc.typetext

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