Orbital Angular Momentum and Spectral Flow in Two Dimensional Chiral Superfluids
arXiv:1409.7459 · doi:10.1103/PhysRevLett.114.195301
Abstract
We study the orbital angular momentum (OAM) in two dimensional chiral -wave superfluids (SF) of fermions on a disc at zero temperature, in terms of spectral asymmetry and spectral flow. It is shown that for any integer , in the BEC regime. In contrast, in the BCS limit, while the OAM is for the -wave SF, for chiral SF with , the OAM is remarkably suppressed as , where is the gap amplitude and is the Fermi energy. We demonstrate that the difference between the -wave SF and the other chiral SFs in the BCS regimes originates from the nature of edge modes and related depairing effects.
arXiv comment5 pages + 4 pages supplemental material
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