Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/63928
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Type: Conference paper
Title: QMC and the nature of dense matter: written in the stars?
Author: Carroll, J.
Citation: Proceedings of Achievements and New Directions in Subatomic Physics: Festchrift in Honor of Tony Thomas 60th Birthday, held in Adelaide, South Australia, 15-19 February 2010 / W. Melnitchouk (ed.): pp.226-231
Publisher: Springer New York LLC
Publisher Place: United States
Issue Date: 2010
Series/Report no.: AIP Conference Proceedings ; 1261
ISBN: 9780735408111
ISSN: 0094-243X
1551-7616
Conference Name: Achievements and New Directions in Subatomic Physics (2010 : Adelaide, South Australia)
Editor: Melnitchouk, W.
Statement of
Responsibility: 
J. D. Carroll
Abstract: We discuss the recent progress in calculating the properties of 'hybrid stars' (stellar objects similar to neutron stars, classified by the incorporation of non-nucleonic degrees of freedom, including but not limited to hyperons and/or a quark-matter core) using the octet-baryon Quark-Meson Coupling (QMC) model. The version of QMC used is a recent improvement which includes the in-medium modification of the quark-quark hyperfine interaction. © 2010 American Institute of Physics.
Keywords: QMC
EOS
dense matter
neutron stars
hybrid stars
MIT
NJL
Rights: © 2010 American Institute of Physics
DOI: 10.1063/1.3479349
Published version: http://dx.doi.org/10.1063/1.3479349
Appears in Collections:Aurora harvest
Physics publications

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