Abstract:A single momentum-carrying dimension connected by Lorentz transformations to a perpendicular non-local dimension having time but lacking spatial measures is applied to electromagnetic radiation, thermal radiation, the Schrödinger equation, Kepler’s 3:rd law, the rotation curve of spiral galaxies, and the universe as a whole represented by the linear part of its apparent expansion. This is made possible by identifying and making local terms equal to non-local ones as prescribed by the geometry. For example, 1-D… Show more
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