Sharing symmetries in non-linear systems: Generalized Heisenberg-Weyl algebra on the de Sitter space-time out of the sphere S 3
In this paper, we exploit the formal equivalence of the Solution Manifold of two distinct physical systems to create enough symmetries so as to characterize them by Noether Invariants, thus favoring their future quantization. In so doing, we somehow generalize the Arnold Transformation for non-neces...
| Autores: | , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión aceptada para publicación |
| Fecha de publicación: | 2021 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/256633 |
| Acceso en línea: | http://hdl.handle.net/10261/256633 |
| Access Level: | acceso abierto |
| Palabra clave: | Symmetry Non-linear systems Non-point symmetries Cartan formalism Hamilton–Jacobi Inverse Noether theorem S3 sigma model Generalized position and momentum in de Sitter space-time |
| Sumario: | In this paper, we exploit the formal equivalence of the Solution Manifold of two distinct physical systems to create enough symmetries so as to characterize them by Noether Invariants, thus favoring their future quantization. In so doing, we somehow generalize the Arnold Transformation for non-necessarily linear systems. Very particularly, this algorithm applies to the case of the motion on the de Sitter space-time providing a finite-dimensional algebra generalizing the Heisenberg-Weyl algebra globally. In this case, the basic (contact) symmetry is imported from the motion of a (non-relativistic) particle on the sphere S3. © 2021 World Scientific Publishing Company. |
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