We review quark matter properties using of isospin asymmetric in confined-dependent-mass (CIDDM) model. This model is well enough for describing large mass pulsar by a quark stars. But after comparing its equation of state with the result from perturbative QCD calculation then we find that CIDDM model cannot precisely predicts equation of state of quark matter at high baryon density and low temperature. Here we give several plots and comparison to the pQCD calculation.
|Publication status||Published - 2014|