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Journal of Low Temperature Physics

Orbital dynamics of the Anderson-Brinkman-Morel phase of superfluid3He

M. C. Cross

Published Jan 1, 1977• 58 citations
Publisher
DOI
10.1007/bf00654566

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With proper care on the boundary conditions, the total orbital angular momentum L z at finite temperatures is microscopically calculated for the Anderson-Brinkman-Morel state in a cylinder with axial symmetry about the z axis, i.e. the textures considered by McClure and Takagi at T =0. The pairing in this geometry occurs between m and 1- m one-particle states, where m denotes the axial quantum number. It is found that L z decreases from its zero temperature value \(\frac{\hbar}{2} {\cal N}\), with N the total particle number, in the same way as the components of the superfluid density tensor. Responsible for this reduction is identified to be the phase shift between m and 1- m quasiparticle states caused by the difference in the centrifugal potentials. This fact implies that the plane-wave representation is not suitable for the problem.

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With proper care on the boundary conditions, the total orbital angular momentum L z at finite temperatures is microscopically calculated for the Anderson-Brinkman-Morel state in a cylinder with axial symmetry about the z axis, i.e. the textures considered by McClure and Takagi at T =0. The pairing in this geometry occurs between m and 1- m one-particle states, where m denotes the axial quantum number. It is found that L z decreases from its zero temperature value ℏ2N\frac{\hbar}{2} {\cal N}2ℏ​N, with N the total particle number, in the same way as the components of the superfluid density tensor. Responsible for this reduction is identified to be the phase shift between m and 1- m quasiparticle states caused by the difference in the centrifugal potentials. This fact implies that the plane-wave representation is not suitable for the problem.