Hidden symmetry group for particle orbits (timelike geodesics) in Schwarzschild spacetime

Fuente: arXiv
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Autores principales: Anco, Stephen C., Moghadam, Mahdieh Gol Bashmani
Formato: Preprint
Publicado: 2026
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author Anco, Stephen C.
Moghadam, Mahdieh Gol Bashmani
author_facet Anco, Stephen C.
Moghadam, Mahdieh Gol Bashmani
contents For the timelike geodesic equations in Schwarzschild spacetime, three hidden conserved quantities were found recently, which are analogues of dynamical quantities related to the well-known Laplace-Runge-Lenz (LRL) vector in Newtonian gravity. In particular, the geodesic equations possess an LRL angle, an LRL Killing-vector time and an LRL proper-time, each of which is a conserved quantity for all timelike geodesics. The present work provides a natural symmetry interpretation for these three quantities by applying Noether's theorem in reverse to the geodesic Lagrangian. This yields three hidden symmetry transformations. They are shown to commute with the Killing isometries and act on the equatorial geodesics by separate shifts and scaling of the geodesic energy and angular momentum. Together with the Killing symmetries, these transformations comprise the complete Noether symmetry group of the timelike equatorial geodesic equations.
format Preprint
id arxiv_https___arxiv_org_abs_2604_16644
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Hidden symmetry group for particle orbits (timelike geodesics) in Schwarzschild spacetime
Anco, Stephen C.
Moghadam, Mahdieh Gol Bashmani
General Relativity and Quantum Cosmology
Mathematical Physics
For the timelike geodesic equations in Schwarzschild spacetime, three hidden conserved quantities were found recently, which are analogues of dynamical quantities related to the well-known Laplace-Runge-Lenz (LRL) vector in Newtonian gravity. In particular, the geodesic equations possess an LRL angle, an LRL Killing-vector time and an LRL proper-time, each of which is a conserved quantity for all timelike geodesics. The present work provides a natural symmetry interpretation for these three quantities by applying Noether's theorem in reverse to the geodesic Lagrangian. This yields three hidden symmetry transformations. They are shown to commute with the Killing isometries and act on the equatorial geodesics by separate shifts and scaling of the geodesic energy and angular momentum. Together with the Killing symmetries, these transformations comprise the complete Noether symmetry group of the timelike equatorial geodesic equations.
title Hidden symmetry group for particle orbits (timelike geodesics) in Schwarzschild spacetime
topic General Relativity and Quantum Cosmology
Mathematical Physics
url https://arxiv.org/abs/2604.16644