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Neutron stars and massive quark matter

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Other literature type 01 Jan 1996Embargo end date: 01 Jan 1995 Italy English Publisher:Elsevier BVJournal:Progress in Particle and Nuclear Physics, volume 36, pages 407-408 (issn: 0146-6410,

Authors: DRAGO, Alessandro; U. Tambini; M. Hjorth Jensen;

doi: 10.1016/0146-6410(96)00045-2 , 10.1016/0370-2693(96)00479-0 , 10.48550/arxiv.nucl-th/9505037

arXiv: http://arxiv.org/abs/nucl-th/9505037

handle: 11392/1685446

Neutron stars and massive quark matter

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Abstract

Using the Color-Dielectric model to describe quark confinement, including strange quarks and accounting for beta--equilibrium, we get masses for a static neutron star in the range $1.3\leq M/M_{\odot}\leq 1.54 $ for a radius $R\approx 9$ km. Rapid cooling through the direct URCA mechanism is obtained. The implications for the composition of neutron stars is discussed.

8 pages, Revtex style, 4 uuencoded figures appended

Country

Italy

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Keywords

Nuclear Theory (nucl-th), Equation of state; Massive quark matter; Neutron stars;, Nuclear Theory, FOS: Physical sciences

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