Hybrid neutron star EOS constructed from DDME2 hadronic and two-flavor NJL quark models with quintic interpolation requires early crossover near saturation density to satisfy PSR J0740+6620 mass and NICER radius constraints.
Tidal deformability of neutron stars with realistic equations of state and their gravitational wave signatures in binary inspiral
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Study of Neutron Star Properties under the Two-Flavor Quark NJL Model
Hybrid neutron star EOS constructed from DDME2 hadronic and two-flavor NJL quark models with quintic interpolation requires early crossover near saturation density to satisfy PSR J0740+6620 mass and NICER radius constraints.