Covariance, Geometricity, Setting, and Dynamical Structures on Cosmological Manifold

dc.creatorMashkevich, Vladimir S.
dc.date2006-03-14
dc.date.accessioned2026-07-07T07:05:59Z
dc.date.available2026-07-07T07:05:59Z
dc.descriptionThe treatment of the principle of general covariance based on coordinate systems, i.e., on classical tensor analysis suffers from an ambiguity. A more preferable formulation of the principle is based on modern differential geometry: the formulation is coordinate-free. Then the principle may be called ``principle of geometricity.'' In relation to coordinate transformations, there had been confusions around such concepts as symmetry, covariance, invariance, and gauge transformations. Clarity has been achieved on the basis of a group-theoretical approach and the distinction between absolute and dynamical objects. In this paper, we start from arguments based on structures on cosmological manifold rather than from group-theoretical ones, and introduce the notion of setting elements. The latter create a scene on which dynamics is performed. The characteristics of the scene and dynamical structures on it are considered.
dc.description12 pages
dc.identifierhttps://arxiv.org/abs/gr-qc/0603053
dc.identifierhttp://arxiv.org/abs/gr-qc/0603053
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/109865
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleCovariance, Geometricity, Setting, and Dynamical Structures on Cosmological Manifold
dc.typetext

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