31 research outputs found

    Kinematic Quantities and Raychaudhuri Equations in a 5D5D Universe

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    Based on some ideas emerged from the classical Kaluza-Klein theory, we present a 5D5D universe as a product bundle over the 4D4D spacetime. This enables us to introduce and study two categories of kinematic quantities (expansions, shear, vorticity) in a 5D5D universe. One category is related to the fourth dimension (time), and the other one comes from the assumption of the existence of the fifth dimension. The Raychaudhuri type equations that we obtain in the paper, lead us to results on the evolution of both the 4D4D expansion and 5D5D expansion in a 5D5D universe.Comment: 27 page

    A NEW POINT OF VIEW ON (1+3) THREADING OF SPACETIME

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    On Higher Dimensional Kaluza-Klein Theories

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    We present a new method for the study of general higher dimensional Kaluza-Klein theories. Our new approach is based on the Riemannian adapted connection and on a theory of adapted tensor fields in the ambient space. We obtain, in a covariant form, the fully general 4D equations of motion in a (4 + n)D general gauge Kaluza-Klein space. This enables us to classify the geodesics of the (4 + n)D space and to show that the induced motions in the 4D space bring more information than motions from both the 4D general relativity and the 4D Lorentz force equations. Finally, we note that all the previous studies on higher dimensional Kaluza-Klein theories are particular cases of the general case considered in the present paper

    Geometry of CR-submanifolds

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    Geometry of CR-Submanifolds

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    Equations of motion with respect to the

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    We continue our research work started in Bejancu (Eur Phys J C 75:346, 2015), and obtain in a covariant form the equations of motion with respect to the (1+1+3)(1+1+3) threading of a 5D universe (Mˉ,gˉ)(\bar{M}, \bar{g}). The natural splitting of the tangent bundle of Mˉ\bar{M} leads to the study of three categories of geodesics: spatial geodesics, temporal geodesics, and vertical geodesics. As an application of the general theory, we introduce and study what we call the 5D Robertson–Walker universe

    FIELD EQUATIONS FOR SPACE–TIME–MATTER THEORY

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    Real hypersurfaces of CPnCP^n with non-negative Ricci curvature

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    Semi-invariant submanifolds of a Sasakian space form

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