Covariant description for superfluids in gravitational fields
| dc.creator | Casini, H. | |
| dc.creator | Montemayor, R. | |
| dc.date | 1999-11-01 | |
| dc.date.accessioned | 2026-07-07T03:33:40Z | |
| dc.date.available | 2026-07-07T03:33:40Z | |
| dc.description | In this paper we develop a formalism to describe a superfluid in a gravitational background. This formalism is based on a covariant generalization of the field description for a superconductor in terms of a U(1) spontaneous symmetry breaking. We study the stability of the solutions for a vortexless fluid and the force acting on vortices in the fluid, which is a generalization of the well-known flat space-time Magnus force. To clarify the development we include the explicit discussion of two particular cases, one of them of astrophysical interest. | |
| dc.description | 22 pages, no figures | |
| dc.identifier | https://arxiv.org/abs/gr-qc/9910115 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/9910115 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/36664 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Covariant description for superfluids in gravitational fields | |
| dc.type | text |