Superintegrability on Three-Dimensional Riemannian and Relativistic Spaces of Constant Curvature

A family of classical superintegrable Hamiltonians, depending on an arbitrary radial function, which are defined on the 3D spherical, Euclidean and hyperbolic spaces as well as on the (2+1)D anti-de Sitter, Minkowskian and de Sitter spacetimes is constructed. Such systems admit three integrals of th...

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Published in:Symmetry, Integrability and Geometry: Methods and Applications
Date:2006
Main Authors: Herranz, F.J., Ballesteros, Á
Format: Article
Language:English
Published: Інститут математики НАН України 2006
Online Access:https://nasplib.isofts.kiev.ua/handle/123456789/146443
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Journal Title:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Cite this:Superintegrability on Three-Dimensional Riemannian and Relativistic Spaces of Constant Curvature / F.J. Herranz, Á. Ballesteros // Symmetry, Integrability and Geometry: Methods and Applications. — 2006. — Т. 2. — Бібліогр.: 43 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
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author Herranz, F.J.
Ballesteros, Á
author_facet Herranz, F.J.
Ballesteros, Á
citation_txt Superintegrability on Three-Dimensional Riemannian and Relativistic Spaces of Constant Curvature / F.J. Herranz, Á. Ballesteros // Symmetry, Integrability and Geometry: Methods and Applications. — 2006. — Т. 2. — Бібліогр.: 43 назв. — англ.
collection DSpace DC
container_title Symmetry, Integrability and Geometry: Methods and Applications
description A family of classical superintegrable Hamiltonians, depending on an arbitrary radial function, which are defined on the 3D spherical, Euclidean and hyperbolic spaces as well as on the (2+1)D anti-de Sitter, Minkowskian and de Sitter spacetimes is constructed. Such systems admit three integrals of the motion (besides the Hamiltonian) which are explicitly given in terms of ambient and geodesic polar coordinates. The resulting expressions cover the six spaces in a unified way as these are parametrized by two contraction parameters that govern the curvature and the signature of the metric on each space. Next two maximally superintegrable Hamiltonians are identified within the initial superintegrable family by finding the remaining constant of the motion. The former potential is the superposition of a (curved) central harmonic oscillator with other three oscillators or centrifugal barriers (depending on each specific space), so that this generalizes the Smorodinsky-Winternitz system. The latter one is a superposition of the Kepler-Coulomb potential with another two oscillators or centrifugal barriers. As a byproduct, the Laplace-Runge-Lenz vector for these spaces is deduced. Furthermore both potentials are analysed in detail for each particular space. Some comments on their generalization to arbitrary dimension are also presented.
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institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
issn 1815-0659
language English
last_indexed 2025-11-27T17:05:54Z
publishDate 2006
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spelling Herranz, F.J.
Ballesteros, Á
2019-02-09T17:13:53Z
2019-02-09T17:13:53Z
2006
Superintegrability on Three-Dimensional Riemannian and Relativistic Spaces of Constant Curvature / F.J. Herranz, Á. Ballesteros // Symmetry, Integrability and Geometry: Methods and Applications. — 2006. — Т. 2. — Бібліогр.: 43 назв. — англ.
1815-0659
2000 Mathematics Subject Classification: 37J35; 22E60; 37J15; 70H06
https://nasplib.isofts.kiev.ua/handle/123456789/146443
A family of classical superintegrable Hamiltonians, depending on an arbitrary radial function, which are defined on the 3D spherical, Euclidean and hyperbolic spaces as well as on the (2+1)D anti-de Sitter, Minkowskian and de Sitter spacetimes is constructed. Such systems admit three integrals of the motion (besides the Hamiltonian) which are explicitly given in terms of ambient and geodesic polar coordinates. The resulting expressions cover the six spaces in a unified way as these are parametrized by two contraction parameters that govern the curvature and the signature of the metric on each space. Next two maximally superintegrable Hamiltonians are identified within the initial superintegrable family by finding the remaining constant of the motion. The former potential is the superposition of a (curved) central harmonic oscillator with other three oscillators or centrifugal barriers (depending on each specific space), so that this generalizes the Smorodinsky-Winternitz system. The latter one is a superposition of the Kepler-Coulomb potential with another two oscillators or centrifugal barriers. As a byproduct, the Laplace-Runge-Lenz vector for these spaces is deduced. Furthermore both potentials are analysed in detail for each particular space. Some comments on their generalization to arbitrary dimension are also presented.
This work was partially supported by the Ministerio de Educaci´on y Ciencia (Spain, Project FIS2004-07913) and by the Junta de Castilla y Le´on (Spain, Projects BU04/03 and VA013C05).
en
Інститут математики НАН України
Symmetry, Integrability and Geometry: Methods and Applications
Superintegrability on Three-Dimensional Riemannian and Relativistic Spaces of Constant Curvature
Article
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spellingShingle Superintegrability on Three-Dimensional Riemannian and Relativistic Spaces of Constant Curvature
Herranz, F.J.
Ballesteros, Á
title Superintegrability on Three-Dimensional Riemannian and Relativistic Spaces of Constant Curvature
title_full Superintegrability on Three-Dimensional Riemannian and Relativistic Spaces of Constant Curvature
title_fullStr Superintegrability on Three-Dimensional Riemannian and Relativistic Spaces of Constant Curvature
title_full_unstemmed Superintegrability on Three-Dimensional Riemannian and Relativistic Spaces of Constant Curvature
title_short Superintegrability on Three-Dimensional Riemannian and Relativistic Spaces of Constant Curvature
title_sort superintegrability on three-dimensional riemannian and relativistic spaces of constant curvature
url https://nasplib.isofts.kiev.ua/handle/123456789/146443
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AT ballesterosa superintegrabilityonthreedimensionalriemannianandrelativisticspacesofconstantcurvature