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The relativistic entrainment matrix of a superfluid nucleon-hyperon mixture. II. Effect of finite temperatures

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arxiv 0907.0010 v1 pith:CFZCMBEC submitted 2009-06-30 astro-ph.SR astro-ph.HEnucl-th

classification astro-ph.SRastro-ph.HEnucl-th
keywords matrixsuperfluidnucleon-hyperonentrainmentmixturerelativisticandreev-bashkinarbitrary
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We calculate the important quantity of superfluid hydrodynamics, the relativistic entrainment matrix for a nucleon-hyperon mixture at arbitrary temperature. In the nonrelativistic limit this matrix is also termed the Andreev-Bashkin or mass-density matrix. Our results can be useful for modeling the pulsations of massive neutron stars with superfluid nucleon-hyperon cores and for studies of the kinetic properties of superfluid baryon matter.

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