Gravitational light bending in Euclidean space

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dc.creatorBulyzhenkov, Igor
dc.date1998-05-08
dc.date2000-03-30
dc.date.accessioned2026-07-07T03:32:22Z
dc.date.available2026-07-07T03:32:22Z
dc.descriptionBoth the non-homogeneous slowness of electromagnetic waves in gravitational fields and the frequency red shift contribute to the gravitational light bending. This twofold contribution explains the measured deflection of light rays by the Sun under Euclidean geometry of space.
dc.description2 pages, Latex
dc.identifierhttps://arxiv.org/abs/gr-qc/9805025
dc.identifierhttp://arxiv.org/abs/gr-qc/9805025
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/36209
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleGravitational light bending in Euclidean space
dc.typetext

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