arXiv:nucl-th/0612021 Abstract

arXiv:nucl-th/0612021Abstract References Reviews Resources

Neutron stars and quark matter

Published 2006-12-05Version 1

Recent observations of neutron star masses close to the maximum predicted by nucleonic equations of state begin to challenge our understanding of dense matter in neutron stars, and constrain the possible presence of quark matter in their deep interiors.

Comments: To be published in the proceedings of Quark Confinement and the Hadron Spectrum VII, Sept. 2006, Ponta Delgada, Azores. 7 pages, 3 figures, aiproc

Journal: AIPConf.Proc.892:8-14,2007

DOI: 10.1063/1.2714340

Categories: nucl-th, astro-ph, hep-ph

Subjects: 21.65.+f, 97.60.Jd

Keywords: quark matter, neutron star masses close, deep interiors, nucleonic equations, state begin

Tags: journal article

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