Chiral Phases of Superfluid 3He in an Anisotropic Medium
arXiv:1307.7656 · doi:10.1103/PhysRevB.88.214503
Abstract
I report theoretical analysis and predictions for the equilibrium phases of superfluid 3He infused into a low-density, homogeneous uniaxial aerogel. Ginzburg-Landau (GL) theory for a class of equal-spin-pairing (ESP) states in a medium with uniaxial anisotropy is developed and used to analyze recent experiments on uniaxially strained aerogels. For 3He in an axially "stretched" aerogel GL theory predicts a transition from normal liquid into a chiral ABM phase at T_c1 in which the chirality axis, l, is aligned along the strain axis. This orbitally aligned state, is protected from random fluctuations in the anisotropy direction, has a positive NMR frequency shift, a sharp NMR resonance line and is identified with the high-temperature ESP-1 phase of superfluid 3He in axially stretched aerogel. A second transition into a biaxial phase is predicted to onset at a slightly lower temperature, T_c2 < T_c1. This phase is an ESP state, breaks time-reversal symmetry, and is defined by an orbital order parameter that spontaneously breaks axial rotation symmetry. This transition is driven by the coupling of an axially aligned 1D "polar" order parameter to the two time-reversed 2D axial ABM states. The biaxial phase has a continuous degeneracy associated with the projection of its chiral axis in the plane normal to the anisotropy axis. Theoretical predictions for the NMR frequency shifts of the biaxial phase provide an identification of the ESP-2 as the biaxial state, partially disordered by random anisotropy (Larkin-Imry-Ma effect). The "width" of the jump in the NMR frequency shift at T_c2 provides an estimate of the orbital domain size, xi_LIM ~ 5 mu-m at 18 bar.
15 pages, 6 figures
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- The Effect of Magnetic Impurities on Superfluid He in Aerogel
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- Impact of Strong Anisotropy on Phase Diagram of Superfluid He in Aerogels
- Planar and Nematic Aerogels: DLCA and Superfluid 3He
- Superfluid He in Planar Aerogel
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- Anomalous Hall Effects in Chiral Superconductors
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