Derivation of Klein-Gordon-Fock equation from General relativity in a time-space symmetrical model
Vo Van Thuan

TL;DR
This paper demonstrates that Einstein's gravitational equations in a symmetrical time-space model can lead to the Klein-Gordon-Fock equations, bridging quantum mechanics and general relativity through a bi-cylindrical geometrical framework.
Contribution
It introduces a bi-cylindrical geometrical model where Einstein's equations produce Klein-Gordon-Fock equations, suggesting a new approach to unify quantum mechanics with general relativity.
Findings
Einstein equations lead to bi-geodesic descriptions in symmetrical time-space.
Geodesic solutions are mathematically equivalent to Klein-Gordon-Fock equations.
The model provides a potential pathway for quantum-gravity unification.
Abstract
Following a bi-cylindrical model of geometrical dynamics, in the present study we show that Einstein gravitational equation leads to bi-geodesic description in an extended symmetrical time-space which fit Hubble expansion in a "microscopic" cosmological model. As a duality, the geodesic solution is mathematically equivalent to the basic Klein-Gordon-Fock equations of free massive elementary particles, in particular, as the squared Dirac equations of leptons and as a sub-solution with pseudo-axion. This result would serve an explicit approach to consistency between quantum mechanics and general relativity.
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Taxonomy
TopicsQuantum Mechanics and Non-Hermitian Physics · Quantum Mechanics and Applications · Algebraic and Geometric Analysis
