On non-Riemannian geometry of superfluids

Details On non-Riemannian geometry of superfluids On non-Riemannian geometry of superfluids

2003-01-05

arxiv.org/abs/gr-qc/0301013v1

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

Latex file

Scientific paper

The 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.

Affiliated with

Also associated with

No associations

Rating

On non-Riemannian geometry of superfluids does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with On non-Riemannian geometry of superfluids, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On non-Riemannian geometry of superfluids will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-386018