dorsal/arxiv
View SchemaNeutron Stars and Massive Quark Matter
| Authors | A. Drago, U. Tambini, M. Hjorth-Jensen |
|---|---|
| Categories | |
| ArXiv ID | nucl-th/9505037 |
| URL | https://arxiv.org/abs/nucl-th/9505037 |
| DOI | 10.1016/0370-2693(96)00479-0 |
| Journal | Phys. Lett. B380 (1996) 13 |
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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"abstract": "Using the Color-Dielectric model to describe quark confinement, including\nstrange quarks and accounting for beta--equilibrium, we get masses for a static\nneutron star in the range $1.3\\leq M/M_{\\odot}\\leq 1.54 $ for a radius\n$R\\approx 9$ km. Rapid cooling through the direct URCA mechanism is obtained.\nThe implications for the composition of neutron stars is discussed.",
"arxiv_id": "nucl-th/9505037",
"authors": [
"A. Drago",
"U. Tambini",
"M. Hjorth-Jensen"
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"doi": "10.1016/0370-2693(96)00479-0",
"journal_ref": "Phys. Lett. B380 (1996) 13",
"title": "Neutron Stars and Massive Quark Matter",
"url": "https://arxiv.org/abs/nucl-th/9505037"
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