arXiv:0907.0010·v1·Solar and Stellar Astrophysics
The relativistic entrainment matrix of a superfluid nucleon-hyperon mixture. II. Effect of finite temperatures
M.E. Gusakov (1) · E.M. Kantor (1) · P. Haensel (2) ((1) Ioffe Institute · (2) CAMK)
Abstract
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.
Comments: 10 pages, 1 figure, accepted for publication in Phys. Rev. C