Classical and quantum mechanics of the nonrelativistic Snyder model
Creators
- 1. Dipartimento di Matematica, Universita di Cagliari, viale Merello 92, 09123 Cagliari (Italy) and INFN, Sezione di Cagliari (Italy)
Description
The Snyder model is an example of noncommutative spacetime admitting a fundamental length scale β and invariant under Lorentz transformations, that can be interpreted as a realization of the doubly special relativity axioms. Here, we consider its nonrelativistic counterpart, i.e. the Snyder model restricted to three-dimensional Euclidean space. We discuss the classical and the quantum mechanics of a free particle in this framework, and show that they strongly depend on the sign of a coupling constant λ, appearing in the fundamental commutators and proportional to β2. For example, if λ is negative, momenta are bounded. On the contrary, for positive λ, positions and areas are quantized. We also give the exact solution of the harmonic oscillator equations both in the classical and the quantum case, and show that its frequency is energy dependent.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.84.025021;
- arXiv
- arXiv:1104.0490v2;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 84
- Journal Issue
- 2
- Journal Page Range
- p. 025021-025021.11
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 43079562
- Subject category
- S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- COMMUTATION RELATIONS; COUPLING CONSTANTS; ENERGY DEPENDENCE; EUCLIDEAN SPACE; EXACT SOLUTIONS; HARMONIC OSCILLATORS; LORENTZ TRANSFORMATIONS; PARTICLES; QUANTUM MECHANICS; RELATIVITY THEORY; SIMULATION; SPACE-TIME; THREE-DIMENSIONAL CALCULATIONS
- Descriptors DEC
- MATHEMATICAL SOLUTIONS; MATHEMATICAL SPACE; MECHANICS; RIEMANN SPACE; SPACE; TRANSFORMATIONS
Optional Information
- Notes
- (c) 2011 American Institute of Physics