Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/97423
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dc.contributor.authorWhittenbury, D.en
dc.contributor.authorCarroll, J.en
dc.contributor.authorThomas, A.en
dc.contributor.authorTsushima, K.en
dc.contributor.authorStone, J.en
dc.date.issued2014en
dc.identifier.citationPhysical Review C, 2014; 89(6):065801-1-065801-18en
dc.identifier.issn0556-2813en
dc.identifier.issn1089-490Xen
dc.identifier.urihttp://hdl.handle.net/2440/97423-
dc.descriptionPublished 3 June 2014en
dc.description.abstractWe explore the equation of state for nuclear matter in the quark-meson coupling model, including full Fock terms. The comparison with phenomenological constraints can be used to restrict the few additional parameters appearing in the Fock terms which are not present at the Hartree level. Because the model is based upon the in-medium modification of the quark structure of the bound hadrons, it can be readily extended to include hyperons and to calculate the equation of state of dense matter in β equilibrium. This leads naturally to a study of the properties of neutron stars, including their maximum mass, radii, and density profiles.en
dc.description.statementofresponsibilityD. L. Whittenbury, J. D. Carroll, A. W. Thomas, K. Tsushima, J. R. Stoneen
dc.language.isoenen
dc.publisherAmerican Physical Societyen
dc.rights©2014 American Physical Societyen
dc.titleQuark-meson coupling model, nuclear matter constraints, and neutron star propertiesen
dc.typeJournal articleen
dc.identifier.doi10.1103/PhysRevC.89.065801en
dc.relation.granthttp://purl.org/au-research/grants/arc/FL0992247en
pubs.publication-statusPublisheden
dc.identifier.orcidThomas, A. [0000-0003-0026-499X]en
Appears in Collections:Chemistry and Physics publications

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