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Classical and Quantum Gravity

Article . 1991 . Peer-reviewed

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Classical and Quantum Gravity

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Properties of quark stars

descriptionPublicationkeyboard_double_arrow_right Article 01 Feb 1991Publisher:IOP PublishingJournal:Classical and Quantum Gravity, volume 8, pages L49-L56 (issn: 0264-9381, eissn: 1361-6382,

Authors: E Ostgaard; T Overgard;

doi: 10.1088/0264-9381/8/2/004

Properties of quark stars

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Abstract

The authors calculate the mass, radius, moment of inertia and surface gravitational red shift of quark stars described by three models: the noninteracting Fermi gas model of Itoh (1970), the asymptotic MIT bag model, and the perturbative QCD model of Chapline and Nauenberg (1977). They report the results of phase transition calculations, and comment on possible observable differences between neutron stars and quark stars.

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