The outer gravitational potential of an inhomogeneous torus with an elliptical cross-section
Elena Bannikova, Serhii Skolota, Massimo Capaccioli

TL;DR
This paper presents an approximation method for calculating the outer gravitational potential of inhomogeneous elliptical tori in astrophysics, simplifying complex structures with high accuracy.
Contribution
The authors introduce a novel approximation of the outer potential of inhomogeneous elliptical tori using two thin rings, applicable to various geometries and density distributions.
Findings
Approximation with two rings has less than 1% error for homogeneous tori.
Outer potential weakly depends on density distribution law.
Model accurately predicts external force components.
Abstract
Toroidal structures are a common feature in a wide variety of astrophysical objects, including dusty tori in AGNs, rings in galaxies, protoplanetary disks, and others. The matter distribution in such structures is not homogeneous and can be flattened by self-gravity or become elongated in the vertical direction, as is the case with obscuring tori in AGNs. This led us to consider the more general case of the gravitational potential of an inhomogeneous torus with an elliptical cross-section. We begin by showing that the outer potential of a homogeneous elliptical torus can be effectively approximated with less than 1\% error by the potentials of two infinitely thin rings with a minor correction term. These two rings have masses each equal to half the total mass of the torus. The most notable feature is that each such infinitely thin ring is positioned at precisely the halfway point…
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Taxonomy
TopicsTribology and Lubrication Engineering
