Geodesic motion in Euclidean Schwarzschild geometry
General Relativity and Quantum Cosmology
2022-12-01 v3 High Energy Physics - Theory
Abstract
This paper performs a systematic investigation of geodesic motion in Euclidean Schwarzschild geometry, which is studied in the equatorial plane. The explicit form of geodesic motion is obtained in terms of incomplete elliptic integrals of first, second and third kind. No elliptic-like orbits exist in Euclidean Schwarzschild geometry, unlike the corresponding Lorentzian pattern. Among unbounded orbits, only unbounded first-kind orbits are allowed, unlike general relativity where unbounded second-kind orbits are always allowed.
Keywords
Cite
@article{arxiv.2202.03763,
title = {Geodesic motion in Euclidean Schwarzschild geometry},
author = {Emmanuele Battista and Giampiero Esposito},
journal= {arXiv preprint arXiv:2202.03763},
year = {2022}
}
Comments
v3: version accepted for publication in EPJ C