Neutron Stars as a Probe for Dense Matte
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V.A. Dexheimer; S. Schramm
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Article
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2009
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Elsevier Science
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English
β 194 KB
We study different stages of the neutron star cooling by computing neutron star properties at various temperatures and entropies using an effective chiral model including hadronic and quark degrees of freedom. Macroscopic properties of the star such as mass and radius are calculated and compared wit