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Bibliographic Details
Main Author: Rumler, David
Format: Preprint
Published: 2025
Subjects:
Online Access:https://arxiv.org/abs/2508.01732
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author Rumler, David
author_facet Rumler, David
contents Stability of circular orbits of the dust particles within a charged rotating disc of dust with respect to perturbations in the equatorial plane is analyzed. Within Einstein-Maxwell theory, the charged rotating disc of dust is an axisymmetric, stationary solution given in terms of a post-Newtonian expansion. The disc solution is characterized by a rigid rotation around the axis of symmetry and a constant specific charge $ε$. It is found that for $ε<1$ all realized dust particle orbits are stable and for $ε=1$ all dust particles are in marginally stable states.
format Preprint
id arxiv_https___arxiv_org_abs_2508_01732
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Equatorial stability analysis of dust particle orbits within a charged rotating disc of dust
Rumler, David
General Relativity and Quantum Cosmology
Stability of circular orbits of the dust particles within a charged rotating disc of dust with respect to perturbations in the equatorial plane is analyzed. Within Einstein-Maxwell theory, the charged rotating disc of dust is an axisymmetric, stationary solution given in terms of a post-Newtonian expansion. The disc solution is characterized by a rigid rotation around the axis of symmetry and a constant specific charge $ε$. It is found that for $ε<1$ all realized dust particle orbits are stable and for $ε=1$ all dust particles are in marginally stable states.
title Equatorial stability analysis of dust particle orbits within a charged rotating disc of dust
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2508.01732