As we go from the center toward the surface of a neutron star, the state of baryonic matter changes from the deconfined quark-gluon to a mixed phase of quark and hadronic matter and a thin crust of hadronic matter. For the quark matter, within the MIT bag model, the total energy density of the system is the kinetic energy for noninteracting quarks plus a bag constant. In this article we consider a density-dependent bag constant obtained using the recent experimental results of CERN SPS on the formation of a quarkgluon plasma. For calculations of the hadron phase, we use the lowest-order constrained variational method. The equation of state of the mixed phase is determined using Gibbs conditions. Finally, we calculated the structure of a hot neutron star with quark core employing the TOV equation. Our results show that a density-dependent bag constant leads to a higher mass and lower radius for the hot neutron star with respect to the case where we use a fixed bag constant.
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Published in Astrofizika, Vol. 56, No. 1, pp. 134–141 (February 2013).
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Yazdizadeh, T., Bordbar, G.H. The Effect of a Density-Dependent Bag Constant on the Structure of a Hot Neutron Star with a Quark Core. Astrophysics 56, 121–129 (2013). https://doi.org/10.1007/s10511-013-9272-y
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DOI: https://doi.org/10.1007/s10511-013-9272-y