A first course in geometric topology and differential geometry
A first course in geometric topology and differential geometry
Numerical experience with the finite speed of gravitational interaction
Mathematics and Computers in Simulation - Special issue from IMACS sponsored conference: “Modelling '98”
Modern Differential Geometry of Curves and Surfaces with Mathematica
Modern Differential Geometry of Curves and Surfaces with Mathematica
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According to the Einstein cosmological principle, our universe is homogeneous and isotropic, i.e. its curvature is constant at any point and in any direction. On large scales, when all local irregularities are ignored, this assumption has been confirmed by astronomers. We show that there is no reasonable hyperbolic geometry model in R4 of a homogeneous and isotropic universe for a fixed time which would fit the cosmological principle. Hence, there does not exist any model in R4 of an isotropic universe which would be represented by a three-dimensional hypersurface with the Lobachevsky geometry.