2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/36664In 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.22 pages, no figuresGeneral Relativity and Quantum CosmologyCovariant description for superfluids in gravitational fieldstext