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Illustrating the liquid gas transition of nuclear matter in QCD

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arxiv 2504.00539 v1 pith:G6MFYGBY submitted 2025-04-01 nucl-th hep-phhep-thnucl-ex

classification nucl-thhep-phhep-thnucl-ex
keywords nucleonbindingenergynucleartransitiondensitydifferenceequation
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

We demonstrate that the liquid-gas transition of nuclear matter can be rigorously described with the quantum chromodynamics by combining the quark gap equation and the Faddeev equation of nucleon. Our investigation focuses on this transition at zero temperature and finite chemical potential, revealing a finite difference between the gas and liquid solution of the quark propagator. This difference emerges from the shift of the nucleon pole mass in medium, which is generated in the nucleon channel of the quark gap equation. We prove that such a difference is precisely the contour contribution from the shift of the nucleon pole. The resulting discontinuity manifests as a first-order phase transition and fundamentally determines both the nuclear binding energy and the saturation density. We then derive an analytical relation between the binding energy and the sigma term of the nucleon, yielding a binding energy of $E/A=15.9\,\textrm{MeV}$. Furthermore, by establishing the relation between the nuclear saturation density and the vector charge of nucleon in association with the binding energy, we determine the saturation density to be $n_{\textrm{B}}^{0}=0.15\,\textrm{fm}^{-3}$.

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  1. The equation of state and surface tension of QCD in the first order phase transition region

    hep-ph 2025-07 conditional novelty 5.0 of 10

    A parametrized order-parameter model yields the equation of state, spinodal boundaries, and surface tension for the first-order QCD phase transition.

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