Anisotropic geometrodynamics in cosmological problems
Sergey Siparov

TL;DR
This paper proposes a modified gravitation theory based on geometric principles, addressing classical issues like galaxy rotation curves and the Tully-Fisher law, and offering insights into cosmic acceleration.
Contribution
It introduces a generalized geodesic framework that extends classical GRT, providing a geometric origin for dark matter effects and cosmic acceleration.
Findings
Explains flat galaxy rotation curves without dark matter
Derives the Tully-Fisher law from geometric principles
Reveals a fundamental geometric origin of cosmic acceleration
Abstract
The gravitation theory is modified on the base of geometric identity and equivalence principle. This makes it possible to generalize the geodesics and solve several problems of classical GRT such as flat rotation curves of the spiral galaxies, Tully-Fisher law and some others and reveal the fundamental (geometrical) origin of the cH acceleration value. The developed approach contains all the results of the classical GRT and has promising cosmological consequences.
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Taxonomy
TopicsGeophysics and Gravity Measurements · Relativity and Gravitational Theory
