Relativistic Rotation in the Large Radius, Small Angular Velocity Limit

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dc.creatorKlauber, Robert D.
dc.date2002-09-09
dc.date.accessioned2026-07-07T03:27:09Z
dc.date.available2026-07-07T03:27:09Z
dc.descriptionRelativistic rotation is considered in the limit of angular velocity approaching zero and radial distance approaching infinity, such that centrifugal acceleration is immeasurably small while tangent velocity remains close to the speed of light. For this case, the predictions of the traditional approach to relativistic rotation using local co-moving Lorentz frames are compared and contrasted with those of the differential geometry based non-time-orthogonal analysis approach. Different predictions by the two approaches imply that only the non-time-orthogonal approach is valid.
dc.description10 pages including 2 figures, 1 table and references
dc.identifierhttps://arxiv.org/abs/gr-qc/0209025
dc.identifierhttp://arxiv.org/abs/gr-qc/0209025
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/34323
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleRelativistic Rotation in the Large Radius, Small Angular Velocity Limit
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