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Neutron Star Properties in a QCD-Motivated Model

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Abstract

We investigate the composition and structure of neutron-, hybrid-, and quark stars within an effective QCD-motivated model of strong interaction. The hadronic phase is described within a novel chiral SU(3) model and the deconfined quark-gluon plasma phase is formulated within the bag model. The phase transition between these phases is treated as a first order transition having two conserved charges.

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Authors and Affiliations

  1. Institut für Theoretische Physik, J.W. Goethe-Universität, D-60054, Frankfurt am Main, Germany

    Matthias Hanauske & Walter Greiner

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  1. Matthias Hanauske
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  2. Walter Greiner
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Hanauske, M., Greiner, W. Neutron Star Properties in a QCD-Motivated Model. General Relativity and Gravitation 33, 739–755 (2001). https://doi.org/10.1023/A:1010291321139

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