\begin{table}%t1
\caption{\label{tab:EOSs-had}Equations of state of the neutron star core.}
\small%\centerline
 {
\begin{tabular}{ccccc}
\hline \hline
&&&& \\[-8pt]
\raisebox{-1.5ex}{EOS} & \raisebox{-1.5ex}{Model} &
\raisebox{-1.5ex}{Ref.}
& $M_{\rm max}^{\rm stat}$& $R_{1.4}$\\ 
&&&[$M_\odot$]&[km]\\
\hline 
\raisebox{-1.5ex}{FPS} & N, energy& \raisebox{-1.5ex}a&
\raisebox{-1.5ex}{1.800}&\raisebox{-1.5ex}{10.85}\\ 
&density functional&&&\\
\hline 
\raisebox{-1.5ex}{GN3}& N, relativistic& \raisebox{-1.5ex}b&
\raisebox{-1.5ex}{2.134}&\raisebox{-1.5ex}{14.22}\\ 
&mean field&&&\\
\hline
 \raisebox{-1.5ex}{DH}& N, energy & \raisebox{-1.5ex}c&
\raisebox{-1.5ex}{2.048}&\raisebox{-1.5ex}{11.69}\\ 
&density functional&&&\\
\hline 
\raisebox{-1.5ex}{APR}& N, variational&
\raisebox{-1.5ex}{${\rm d}$}&
\raisebox{-1.5ex}{2.212}&  \raisebox{-1.5ex}{11.42}\\ 
&theory&&&\\
\hline \raisebox{-1.5ex}{BGN1H1} & NH, energy&
\raisebox{-1.5ex}e&
\raisebox{-1.5ex}{1.630}&  \raisebox{-1.5ex}{12.90} \\
&density functional&&&\\
\hline 
\raisebox{-.5ex}{BBB} &
\raisebox{-.5ex}{N, Brueckner theory}&\raisebox{-.5ex}f&
\raisebox{-.5ex}{1.920}&\raisebox{-.5ex}{11.13}\\
\hline
\raisebox{-1.5ex}{GNH3} & NH,  relativistic &  \raisebox{-1.5ex}g&
\raisebox{-1.5ex}{1.964}&  \raisebox{-1.5ex}{14.20}\\ 
&mean field &&&\\
\hline 
\raisebox{-1.5ex}{GMGS-Km} & N + mixed &
\raisebox{-1.5ex}h&
\raisebox{-1.5ex}{1.454}&  \raisebox{-1.5ex}{13.12}\\ 
&N-kaon condensed&&&\\
\hline 
\raisebox{-1.5ex}{GMGS-Kp} & N + pure &
\raisebox{-1.5ex}i &
\raisebox{-1.5ex}{1.450}&\raisebox{-1.5ex}{13.20}\\ 
& N-kaon condensed&&&\\
 \hline
\end{tabular}}
\medskip
N -- nucleons and leptons. NH -- nucleons, hyperons, and leptons. Exotic states of hadronic matter are indicated explicitly. Maximum allowable mass for  non-rotating stars, $M_{\rm max}^{\rm stat}$,
and the circumferential radius of non-rotating stars of $1.4~M_\odot$, $R_{1.4}$, are given in last two columns, respectively. References for the EOSs: a~--  \cite{ FPS1989}; b~--  \cite{Glend1985}; c~-- \cite{DH2001};  d~--  A18  Argonne NN potential with relativistic corrections and Urbana  modified UIX$^*$ NNN~potential model, from  \cite{APR1998}; e~--   \cite{BG1997}; f~-- Paris two-body NN potential and Urbana UIX three body NNN potential, from \cite{BBB1997}; g~-- \cite{Glend1985}; h, i~-- kaon condensate models with $U_K^{\rm lin}=-125~$MeV, \cite{PonsKcond2000}.
\end{table}