English

Chiral superfluid helium-3 in the quasi-two-dimensional limit

Superconductivity 2025-04-02 v2 Mesoscale and Nanoscale Physics Quantum Gases

Abstract

Anisotropic pair breaking close to surfaces favors the chiral A phase of the superfluid 3^3He over the time-reversal invariant B phase. Confining the superfluid 3^3He into a cavity of height DD of the order of the Cooper pair size characterized by the coherence length ξ0\xi_0 - ranging between 16 nm (34 bar) and 77 nm (0 bar) - extends the surface effects over the whole sample volume, thus allowing stabilization of the A phase at pressures PP and temperatures TT where otherwise the B phase would be stable. In this Letter, the surfaces of such a confined sample are covered with a superfluid 4^4He film to create specular quasiparticle scattering boundary conditions, preventing the suppression of the superfluid order parameter. We show that the chiral A phase is the stable superfluid phase under strong confinement over the full PP-TT phase diagram down to a quasi-two-dimensional limit D/ξ0=1D / \xi_0 = 1 , where D=80D = 80 nm. The planar phase, which is degenerate with the chiral A phase in the weak-coupling limit, is not observed. The gap inferred from measurements over the wide pressure range from 0.2 to 21.0 bar leads to an empirical ansatz for temperature-dependent strong-coupling effects. We discuss how these results pave the way for the realization of the fully gapped two-dimensional px+ipyp_x + ip_y superfluid under more extreme confinement.

Keywords

Cite

@article{arxiv.2409.12901,
  title  = {Chiral superfluid helium-3 in the quasi-two-dimensional limit},
  author = {Petri J. Heikkinen and Lev V. Levitin and Xavier Rojas and Angadjit Singh and Nathan Eng and Andrew Casey and John Saunders and Anton Vorontsov and Nikolay Zhelev and Abhilash Thanniyil Sebastian and Jeevak M. Parpia},
  journal= {arXiv preprint arXiv:2409.12901},
  year   = {2025}
}

Comments

8 pages, 4 figures. This is a copy of the version of record of this article, first published in Physical Review Letters, available online at Publisher's website: https://doi.org/10.1103/PhysRevLett.134.136001 The Supplemental Material is available at http://link.aps.org/supplemental/10.1103/PhysRevLett.134.136001