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Published in 2022 at "Physical Review C"
DOI: 10.1103/physrevc.107.045807
Abstract: Neutron star constraints and {\it ab initio} pQCD evaluations require the EoS representing cold quark matter to be stiff at intermediate baryonic densities and soft at high-$n_B$. Here, I suggest that the three flavor NJL…
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Keywords:
quark;
state strange;
model;
equation state ... See more keywords