Newtonian Fractional-Dimension Gravity and Galaxies without Dark Matter
Gabriele U. Varieschi

TL;DR
This paper applies Newtonian Fractional-Dimension Gravity (NFDG) to galaxies with little or no dark matter, successfully explaining their dynamics through variable fractional dimensions without invoking dark matter.
Contribution
The study demonstrates that NFDG can accurately model galaxy rotation curves and velocity dispersions, providing an alternative to dark matter explanations with variable fractional dimensions.
Findings
NFDG reproduces the rotation curve of galaxy AGC 114905 without dark matter.
NFDG explains velocity dispersions in NGC 1052-DF2 with a fractional dimension D≈2.9.
NFDG accounts for the Bullet Cluster merger velocity without dark matter.
Abstract
We apply Newtonian Fractional-Dimension Gravity (NFDG), an alternative gravitational model, to some notable cases of galaxies with little or no dark matter. In the case of the ultra-diffuse galaxy AGC 114905, we show that NFDG methods can effectively reproduce the observed rotation curve, by using a variable fractional dimension as was done for other galaxies in previous studies. For AGC 114905, we obtain a variable dimension in the range , but our fixed curve can still fit all the experimental data within their error bars. This confirms other studies indicating that the dynamics of this galaxy can be described almost entirely by the baryonic mass distribution alone. However, our NFDG model explains the residual discrepancies without using any dark matter component. In the case of NGC 1052-DF2, we use an argument based on the NFDG…
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Taxonomy
TopicsCosmology and Gravitation Theories · Relativity and Gravitational Theory · Black Holes and Theoretical Physics
