Neutron stars and strange stars in the chiral SU(3) quark mean field model

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dc.contributor.authorWang, P.
dc.contributor.authorLawley, S.
dc.contributor.authorLeinweber, D.
dc.contributor.authorThomas, A.
dc.contributor.authorWilliams, A.
dc.date.issued2005
dc.description.abstractWe 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.
dc.description.statementofresponsibilityP. Wang, S. Lawley, D. B. Leinweber, A. W. Thomas, and A. G. Williams
dc.identifier.citationPhysical Review C: Nuclear Physics, 2005; 72(4):045801-1-045801-8
dc.identifier.doi10.1103/PhysRevC.72.045801
dc.identifier.issn0556-2813
dc.identifier.issn1089-490X
dc.identifier.orcidLeinweber, D. [0000-0002-4745-6027]
dc.identifier.orcidThomas, A. [0000-0003-0026-499X]
dc.identifier.orcidWilliams, A. [0000-0002-1472-1592]
dc.identifier.urihttp://hdl.handle.net/2440/17566
dc.language.isoen
dc.publisherAmerican Physical Soc
dc.rights©2005 American Physical Society.
dc.source.urihttps://doi.org/10.1103/physrevc.72.045801
dc.titleNeutron stars and strange stars in the chiral SU(3) quark mean field model
dc.typeJournal article
pubs.publication-statusPublished

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