In a recent paper the so-called Spectrum Generating Algebra (SGA) technique has been applied to the N-dimensional Taub-NUT system, a maximally superintegrable Hamiltonian system which can be interpreted as a one-parameter deformation of the Kepler-Coulomb system. Such a Hamiltonian is associated to a specific Bertrand space of non-constant curvature. The SGA procedure unveils the symmetry algebra underlying the Hamiltonian system and, moreover, enables one to solve the equations of motion. Here we will follow the same path to tackle the Darboux III system, another maximally superintegrable system, which can indeed be viewed as a natural deformation of the isotropic harmonic oscillator where the flat Euclidean space is again replaced by another space of non-constant curvature.
Latini, D., Ragnisco, O., Ballesteros, A., Enciso, A., Herranz, F.J., Riglioni, D. (2016). The classical Darboux III oscillator: factorization, Spectrum Generating Algebra and solution to the equations of motion. In XXIII International Conference on Integrable Systems and Quantum Symmetries (ISQS-23) (pp.012031). Institute of Physics Publishing [10.1088/1742-6596/670/1/012031].
The classical Darboux III oscillator: factorization, Spectrum Generating Algebra and solution to the equations of motion
LATINI, DANILO;RAGNISCO, Orlando;RIGLIONI, DANILO
2016-01-01
Abstract
In a recent paper the so-called Spectrum Generating Algebra (SGA) technique has been applied to the N-dimensional Taub-NUT system, a maximally superintegrable Hamiltonian system which can be interpreted as a one-parameter deformation of the Kepler-Coulomb system. Such a Hamiltonian is associated to a specific Bertrand space of non-constant curvature. The SGA procedure unveils the symmetry algebra underlying the Hamiltonian system and, moreover, enables one to solve the equations of motion. Here we will follow the same path to tackle the Darboux III system, another maximally superintegrable system, which can indeed be viewed as a natural deformation of the isotropic harmonic oscillator where the flat Euclidean space is again replaced by another space of non-constant curvature.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
