On the anomalous acceleration in the solar system

Simple item page
dc.creatorPalle, D.
dc.date2004-02-12
dc.date2005-02-22
dc.date.accessioned2026-07-07T02:12:16Z
dc.date.available2026-07-07T02:12:16Z
dc.descriptionWe study the impact of the cosmological environment on the solar gravitational system by the imbedding formalism of Gautreau. It appears that the cosmic mean-mass density and the cosmological constant give negligibly small contribution to gravity potentials. On the contrary, the cosmic acceleration beyond the Robertson-Walker geometry can considerably influence the curvature of spacetime in the solar system. The resulting anomalous constant acceleration towards the Sun is an order of magnitude smaller than that measured by Pioneer 10 and 11. However, it is larger than second order terms of potentials, thus well within the sensitivity of new gravity probes such as the LATOR mission.
dc.descriptionLaTeX style, 4 pages; version to be published
dc.identifierhttps://arxiv.org/abs/astro-ph/0402304
dc.identifierhttp://arxiv.org/abs/astro-ph/0402304
dc.identifierActa Phys.Slov. 55 (2005) 237
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7390
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.titleOn the anomalous acceleration in the solar system
dc.typetext

Files

Collections

arXiv