On non-Riemannian geometry of superfluids

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dc.creatorde Andrade, L. C. Garcia
dc.date2003-01-05
dc.date.accessioned2026-07-07T03:27:29Z
dc.date.available2026-07-07T03:27:29Z
dc.descriptionThe Gross-Pitaevski (GP) equation describing helium superfluids is extended to non-Riemannian spacetime background where torsion is shown to induce the splitting in the potential energy of the flow. A cylindrically symmetric solution for Minkowski background with constant torsion is obtained which shows that torsion induces a damping on the superfluid flow velocity. The Sagnac phase shift is computed from the superfluid flow velocity obtained from the solution of GP equations.
dc.descriptionLatex file
dc.identifierhttps://arxiv.org/abs/gr-qc/0301013
dc.identifierhttp://arxiv.org/abs/gr-qc/0301013
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/34448
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleOn non-Riemannian geometry of superfluids
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