Equation of state for strange quark matter: Linking the Nambu--Jona-Lasinio model to perturbative QCD
Marcus Benghi Pinto

TL;DR
This paper proposes a density-dependent NJL model with a decreasing repulsive coupling to produce an equation of state for strange quark matter that smoothly transitions from stiff at intermediate densities to soft at high densities, aligning with neutron star constraints and pQCD results.
Contribution
It introduces a novel density-dependent repulsive coupling in the NJL model that interpolates between non-perturbative and perturbative QCD regimes for the EoS.
Findings
The EoS exhibits a slope change at around 0.7 GeV/fm^3.
The speed of sound peaks at 3.23 times nuclear saturation density.
The trace anomaly remains positive across all densities.
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-. Here, I suggest that the three flavor NJL model with a density dependent repulsive coupling, , can generate an EoS which interpolates between these two regimes. Such an interpolation requires repulsion to start decreasing with the chemical potential just after chiral transition takes place. The conjecture behind this mechanism is that repulsion should be necessary only as long as the quark condensates, which dress the effective masses, have non-vanishing values. This assumption guarantees that an initially hard EoS suffers a conspicuous change of slope at converging to the pQCD results at higher energy densities. Then, the speed of sound naturally reaches a…
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Taxonomy
TopicsHigh-Energy Particle Collisions Research · Pulsars and Gravitational Waves Research · High-pressure geophysics and materials
