Observations of massive ( M \approx 2.0 ~ { } { M } _ { \odot } ) neutron stars ( NSs ) , PSRs J1614-2230 and J0348+0432 , rule out most of the models of nucleon-hyperon matter employed in NS simulations .
Here we construct three possible models of nucleon-hyperon matter consistent with the existence of 2 ~ { } { M } _ { \odot } pulsars as well as with semi-empirical nuclear matter parameters at saturation , and semi-empirical hypernuclear data .
Our aim is to calculate for these models all the parameters necessary for modelling dynamics of hyperon stars ( such as equation of state , adiabatic indices , thermodynamic derivatives , relativistic entrainment matrix , etc .
) , making them available for a potential user .
To this aim a general non-linear hadronic Lagrangian involving \sigma \omega \rho \phi \sigma ^ { \ast } meson fields , as well as quartic terms in vector-meson fields , is considered .
A universal scheme for calculation of the \ell = 0 , 1 Landau Fermi-liquid parameters and relativistic entrainment matrix is formulated in the mean-field approximation .
Use of this scheme allow us to obtain numerical tables with the equation of state , Landau quasiparticle effective masses , adiabatic indices , the \ell = 0 , 1 Landau Fermi-liquid parameters , and the relativistic entrainment matrix for the selected models of nucleon-hyperon matter .
These data are available on-line and suitable for numerical implementation in computer codes modelling various dynamical processes in NSs , in particular , oscillations of superfluid NSs and their cooling .