Wang, P.Lawley, S.Leinweber, D.Thomas, A.Williams, A.2006-12-032006-12-032005Physical Review C: Nuclear Physics, 2005; 72(4):045801-1-045801-80556-28131089-490Xhttp://hdl.handle.net/2440/17566We investigate the equations of state for pure neutron matter and strange hadronic matter in $\beta$-equilibrium, including $\Lambda$, $\Sigma$ and $\Xi$ hyperons. The masses and radii of pure neutron stars and strange hadronic stars are obtained. For a pure neutron star, the maximum mass is about $1.8 M_{\mathrm{sun}}$, while for a strange hadronic star, the maximum mass is around $1.45 M_{\mathrm{sun}}$. The typical radii of pure neutron stars and strange hadronic stars are about 11.0-12.3 km and 10.7-11.7 km, respectively.en©2005 American Physical Society.Journal article002005119510.1103/PhysRevC.72.0458010002329354000612-s2.0-2884450782554507Leinweber, D. [0000-0002-4745-6027]Thomas, A. [0000-0003-0026-499X]Williams, A. [0000-0002-1472-1592]