Discrete fields and the Pioneer anomalous acceleration

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dc.creatorde Souza, Manoelito M.
dc.date2001-06-14
dc.date.accessioned2026-07-07T03:26:00Z
dc.date.available2026-07-07T03:26:00Z
dc.descriptionThe dominant contributions from a discrete gravitational interaction produce the standard potential as an effective continuous field. The sub-dominant contributions are, in a first approximation, linear on n, the accumulated number of (discrete) interaction events along the test-body trajectory. For a nearly radial trajectory n is proportional to the traversed distance and its effects may have been observed as the Pioneer anomalous constant radial acceleration, which cannot be observed on the nearly circular planetary orbits.
dc.description8 pages
dc.identifierhttps://arxiv.org/abs/gr-qc/0106046
dc.identifierhttp://arxiv.org/abs/gr-qc/0106046
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/33930
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleDiscrete fields and the Pioneer anomalous acceleration
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