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Neutron Stars and Massive Quark Matter

A. Drago·U. Tambini·M. Hjorth-Jensen
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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.

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A. Drago, U. Tambini, M. Hjorth-Jensen. 1995-05-26. Neutron Stars and Massive Quark Matter. https://doi.org/10.1016/0370-2693(96)00479-0

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