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Abstract
By means of the EOS of QCD at zero temperature and finite quark chemical potential we proposed [Phys. Rev. D 78 (2008) 054001] in the framework of rainbow-ladder approximation of Dyson–Schwinger approach, we investigate the structure of quark star and its property. It is found that the mass-radius relation in our model is very different from that of usual quark star models, but similar to neutron star models. The obtained mass of quark star is about 1.75Mʘ ∼ 2.2Mʘ. The obtained radius of quark star is 22∼26 km, which is obviously larger than the results in other models. The reason for this discrepancy is analyzed. -
References
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