Massive cold hybrid stars in a modified Polyakov-Nambu-Jona-Lasinio model
This paper proposes a modified Polyakov-Nambu-Jona-Lasinio model with a chemical potential-dependent Polyakov potential to describe cold dense matter, demonstrating that repulsive vector interactions and a stiff hadronic equation of state are essential for forming stable hybrid stars with quarkyonic or deconfined cores that exceed two solar masses.