Theory of Local Times II. Another formulation and examples

dc.creatorKitada, Hitoshi
dc.date1994-03-02
dc.date1995-05-22
dc.date.accessioned2026-07-07T08:59:23Z
dc.date.available2026-07-07T08:59:23Z
dc.descriptionThe model of a stationary universe and the notion of local times presented in [10] are reviewed with some alternative formulation of the consistent unification of the Riemannian and Euclidean geometries of general relativity and quantum mechanics. The method of unification adopted in the present paper is by constructing a vector bundle $X\times R^6$ or $X\times R^4$ with $X$ being the observer's reference frame and $R^6$ or $R^4$ being the unobservable inner space(-time) within each observer's local system. Some applications of our theory to two concrete examples of human size and of cosmological size are discussed, as well as the uncertainty of time in our context is calculated.
dc.description22 pages, LaTeX, revised in minor descriptions
dc.identifierhttps://arxiv.org/abs/gr-qc/9403007
dc.identifierhttp://arxiv.org/abs/gr-qc/9403007
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/147688
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleTheory of Local Times II. Another formulation and examples
dc.typetext

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