Please use this identifier to cite or link to this item: http://hdl.handle.net/2440/97423
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Type: Journal article
Title: Quark-meson coupling model, nuclear matter constraints, and neutron star properties
Author: Whittenbury, D.
Carroll, J.
Thomas, A.
Tsushima, K.
Stone, J.
Citation: Physical Review C, 2014; 89(6):065801-1-065801-18
Publisher: American Physical Society
Issue Date: 2014
ISSN: 0556-2813
1089-490X
Statement of
Responsibility: 
D. L. Whittenbury, J. D. Carroll, A. W. Thomas, K. Tsushima, J. R. Stone
Abstract: We 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.
Description: Published 3 June 2014
Rights: ©2014 American Physical Society
RMID: 0030009182
DOI: 10.1103/PhysRevC.89.065801
Grant ID: http://purl.org/au-research/grants/arc/FL0992247
Appears in Collections:Chemistry and Physics publications

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