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Main Author: Andreoli, Michele
Format: Preprint
Published: 2025
Subjects:
Online Access:https://arxiv.org/abs/2504.07690
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author Andreoli, Michele
author_facet Andreoli, Michele
contents High order corrections to the perihelion precession are obtained in non-Newtonian central potentials, via complex analysis techniques. The result is an exact series expansion whose terms, for a perturbation of the form $δV=\fracγ{r^{s}}$, are calculated in closed form. To validate the method, the series is applied to the specific case of s=3, and the results are compared with those presented in literature, which are relate to the Schwarzschild metric. As a further test, a numerical simulation was carried out for the case where s=4. The algebraic calculations and numerical simulations were carried out via software with symbolic capabilities.
format Preprint
id arxiv_https___arxiv_org_abs_2504_07690
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Perihelion precession in non-Newtonian central potentials
Andreoli, Michele
Earth and Planetary Astrophysics
General Relativity and Quantum Cosmology
High order corrections to the perihelion precession are obtained in non-Newtonian central potentials, via complex analysis techniques. The result is an exact series expansion whose terms, for a perturbation of the form $δV=\fracγ{r^{s}}$, are calculated in closed form. To validate the method, the series is applied to the specific case of s=3, and the results are compared with those presented in literature, which are relate to the Schwarzschild metric. As a further test, a numerical simulation was carried out for the case where s=4. The algebraic calculations and numerical simulations were carried out via software with symbolic capabilities.
title Perihelion precession in non-Newtonian central potentials
topic Earth and Planetary Astrophysics
General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2504.07690