The Euclidean geometry deformations and capacities of their application to microcosm space-time geometry
Yuri A. Rylov

TL;DR
This paper explores a generalized class of space-time geometries called T-geometries, derived from Euclidean deformations, which can geometrically model microcosm phenomena including quantum effects and particle mass without relying on traditional quantum principles.
Contribution
It introduces T-geometries as a broader framework than Riemannian geometry, enabling geometrical modeling of quantum effects and particle properties in microcosm space-time.
Findings
T-geometries can geometrize particle mass.
Quantum effects are described as geometric phenomena.
Asymmetric world functions expand the capacities of T-geometries.
Abstract
Usually a Riemannian geometry is considered to be the most general geometry, which could be used as a space-time geometry. In fact, any Riemannian geometry is a result of some deformation of the Euclidean geometry. Class of these Riemannian deformations is restricted by a series of unfounded constraints. Eliminating these constraints, one obtains a more wide class of possible space-time geometries (T-geometries). Any T-geometry is described by the world function completely. T-geometry is a powerful tool for the microcosm investigations due to three its characteristic features: (1) Any geometric object is defined in all T-geometries at once, because its definition does not depend on the form of world function. (2) Language of T-geometry does not use external means of description such as coordinates and curves; it uses only primordially geometrical concepts: subspaces and world function.…
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Taxonomy
TopicsBiofield Effects and Biophysics · Relativity and Gravitational Theory · Quantum Mechanics and Applications
