Non-Riemannian acoustic spacetime and Magnus field in rotating Bose-Einstein condensates
| dc.creator | de Andrade, L. C. Garcia | |
| dc.date | 2005-01-31 | |
| dc.date.accessioned | 2026-07-07T03:03:31Z | |
| dc.date.available | 2026-07-07T03:03:31Z | |
| dc.description | The teleparallel $T_{4}$ version of Riemannian geometry of acoustic spacetime in rotating $2-D$ Bose-Einstein condensates (BEC) is investigated. An experiment is proposed on the basis of phonon ray trajectory around a vortex. The deviation geodesic equation may be expressed in terms of Cartan acoustic torsion. The Riemann curvature is computed in terms of rotation of the fluid. The geodesic deviation equation shows that the acoustic torsion acts locally as a diverging lens and the stream lines on opposite sides of the BEC vortex flow apart from each other. We also show that the Magnus field is cancelled when the acoustic torsion coincides with the rotation of the condensate. This effect is equivalent to the Meissner effect in superconductors. It is interesting to note how the teleparallel acoustic spacetime constrains the physical parameters in the BEC. Here we use the term acoustic torsion since in teleparallelism it is derived from the acoustic metric. | |
| dc.description | Latex file | |
| dc.identifier | https://arxiv.org/abs/cond-mat/0501741 | |
| dc.identifier | http://arxiv.org/abs/cond-mat/0501741 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/25780 | |
| dc.subject | Statistical Mechanics | |
| dc.title | Non-Riemannian acoustic spacetime and Magnus field in rotating Bose-Einstein condensates | |
| dc.type | text |