Gravitational orbits in the expanding universe revisited
Vaclav Vavrycuk

TL;DR
This paper revisits gravitational orbits in an expanding universe using a conformal FLRW metric, revealing that local systems like galaxies expand with the universe and can explain various astrophysical phenomena without dark matter.
Contribution
It introduces modified Newtonian equations based on the conformal FLRW metric, showing local systems expand with the universe and can account for galactic and solar system observations without dark matter.
Findings
Local systems expand with the Hubble flow under the conformal metric.
Galactic sizes grow consistently with observations and reproduce spiral patterns.
Flat rotation curves and solar system anomalies are explained without dark matter or new physics.
Abstract
Modified Newtonian equations for gravitational orbits in the expanding universe indicate that local gravitationally bounded systems like galaxies and planetary systems are unaffected by the expansion of the Universe. This result is derived under the assumption of the space expansion described by the standard FLRW metric. In this paper, an alternative metric is applied and the modified Newtonian equations are derived for the space expansion described by the conformal FLRW metric. As shown by Vavry\v{c}uk (Frontiers in Physics, 2022), this metric is advantageous, because it properly predicts the cosmic time dilation and fits the SNe Ia luminosity observations with no need to introduce dark energy. Surprisingly, the Newtonian equations based on the conformal FLRW metric behave quite differently than those based on the standard FLRW metric. In contrast to the common opinion that local…
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Taxonomy
TopicsCosmology and Gravitation Theories · Geophysics and Gravity Measurements · Solar and Space Plasma Dynamics
