J arXiv:1308.4436v2 [cond-mat.supr-con] 17 Nov 2013
2Ñj, where j(r) is the phase of the B-phase Cooper pairs. The flow field breaks the SO(2) L z+Sz orbital rotation symmetry about the normal axis of confined 3He-B, as well as time reversal (T) and particle-hole (C) symmetry. However, the Bogoliubov-Nambu Hamiltonian remains invariant under the combined symmetry, U z(p) T, where U z(p)is a p ... ................
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