Revisiting the first-order QCD phase transition in dense strong interaction matter
Yi Lu, Fei Gao, Yu-xin Liu
TL;DR
The paper investigates the first-order QCD phase transition at low temperature and high density using a continuum Dyson-Schwinger equations framework with a Slavnov-Taylor-consistent truncation. It uncovers a distinct intermediate phase $I$ in addition to the Nambu and Wigner phases, indicating spinodal decomposition as a genuine feature of the transition, and analyzes both microscopic (quark mass function $M_q$) and macroscopic (chiral condensate, Polyakov loop) signatures. By coupling the quark sector to a hadronic liquid-gas sector through an excluded-volume mixing, it shows that LG physics can stiffen the equation of state near nuclear saturation density while spinodal dynamics introduce softening, and it provides a quantitative treatment of interface properties, including the interface tension $\sigma$, entropy density $s_A$, and bubble radius $R=2\sigma/\Delta P$. The study extends to isothermal trajectories and computes stability criteria via a total compressibility that combines bulk and interface contributions, offering insights relevant to heavy-ion experiments and neutron star phenomenology, while noting limitations such as the absence of color superconductivity and explicit moiré-like inhomogeneities.
Abstract
We revisit the phase structure and thermodynamics of QCD in the low temperature and high density region, where a strong, first-order phase transition is expected beyond the critical end point. By solving the quark gap equation in the continuum QCD approach, we reveal the coexistence of the multi-phases both in the microscopic dynamics of chiral symmetry breaking and also in the thermodynamic observables, which manifests the existence of spinodal decomposition during the first-order QCD phase transitions. We also analyse the interface structure of the co-exist Nambu and Wigner phases in the isothermal process during the first-order transition. In particular, the interface tension and interface entropy density are extracted from the isothermal trajectories, which further allows for an analysis on the formation of nuclear bubble, including the bubble radius and its stability at different temperatures. Our predictions may serve as useful inputs for further investigations in heavy-ion physics or astrophysics research.
