Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/17566
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 Type: Journal article Title: Neutron stars and strange stars in the chiral SU(3) quark mean field model Author: Wang, P.Lawley, S.Leinweber, D.Thomas, A.Williams, A. Citation: Physical Review C: Nuclear Physics, 2005; 72(4):045801-1-045801-8 Publisher: American Physical Soc Issue Date: 2005 ISSN: 0556-28131089-490X Statement ofResponsibility: P. Wang, S. Lawley, D. B. Leinweber, A. W. Thomas, and A. G. Williams Abstract: We 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. Rights: ©2005 American Physical Society. DOI: 10.1103/PhysRevC.72.045801 Published version: http://dx.doi.org/10.1103/PhysRevC.72.045801 Appears in Collections: Aurora harvest 6Special Research Centre for the Subatomic Structure of Matter publications

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