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Diffusion in superfluid Fermi mixtures: General formalism

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arxiv 2309.03313 v2 pith:EMFJNNJO submitted 2023-09-06 astro-ph.HE cond-mat.quant-gasnucl-th

classification astro-ph.HEcond-mat.quant-gasnucl-th
keywords fermidiffusionsuperfluidcoefficientsmixturescurrentsdevelopeddifferent
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With neutron star applications in mind, we developed a theory of diffusion in mixtures of superfluid, strongly interacting Fermi liquids. By employing the Landau theory of Fermi liquids, we determined matrices that relate the currents of different particle species, their momentum densities, and the partial entropy currents to each other. Using these results, and applying the quasiclassical kinetic equation for the Bogoliubov excitations, we derived general expressions for the diffusion coefficients, which properly incorporate all the Fermi liquid effects and depend on the momentum transfer rates between different particle species. The developed framework can be used as a starting point for systematic calculations of the diffusion coefficients (as well as other kinetic coefficients) in superfluid Fermi mixtures, particularly, in superfluid neutron stars.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Neutron contribution to the force on a proton vortex in superconducting neutron-star matter

    astro-ph.HE 2026-07 conditional novelty 7.0 of 10

    Normal neutrons scatter off proton vortices via the spatially varying condensate momentum, producing a purely longitudinal force proportional to relative neutron-vortex velocity that vanishes without neutron-proton Fe...

  2. Non-purely transverse Magnus force in superconducting neutron stars

    astro-ph.HE 2025-05 conditional novelty 6.0 of 10

    In the idealized extreme type-II limit, the force on a proton vortex core is exactly the Magnus force evaluated with a corrected local proton current, yielding a longitudinal force component usually omitted.

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