QMC and the nature of dense matter: written in the stars?

Carroll, J.

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Publication date

January 2010

DOI

10.1063/1.3479349

Publisher

AIP Publishing

Journal

issn:1551-7616

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.J. D. Carrol

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QMC and the nature of dense matter: written in the stars?

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QMC and the nature of dense matter: written in the stars?

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