On the Kuzmin model in fractional Newtonian gravity
Andrea Giusti, Roberto Garrappa, Genevi\`eve Vachon

TL;DR
This paper explores the Kuzmin disk within fractional Newtonian gravity, deriving potential representations and analyzing asymptotic behavior to understand its implications as an alternative to dark matter.
Contribution
It introduces a detailed analysis of the Kuzmin disk in fractional Newtonian gravity, including new potential representations and asymptotic analysis.
Findings
Derived integral and series representations of the potential
Verified asymptotic behavior at large scales
Provided visualizations of equipotential surfaces
Abstract
Fractional Newtonian gravity, based on the fractional generalization of Poisson's equation for Newtonian gravity, is a novel approach to Galactic dynamics aimed at providing an alternative to the dark matter paradigm through a non-local modification of Newton's theory. We provide an in-depth discussion of the gravitational potential for the Kuzmin disk within this new approach. Specifically, we derive an integral and a series representation for the potential, we verify its asymptotic behavior at large scales, and we provide illuminating plots of the resulting equipotential surfaces.
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