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

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

2009-06-30

arxiv.org/abs/0907.0010v1

Phys.Rev.C80:015803,2009

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

10 pages, 1 figure, accepted for publication in Phys. Rev. C

Scientific paper

10.1103/PhysRevC.80.015803

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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