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arxiv: 1006.3648 · v2 · pith:TMSV6EOAnew · submitted 2010-06-18 · ✦ hep-ph · hep-lat· hep-th· nucl-th

Entanglement between deconfinement transition and chiral symmetry restoration

classification ✦ hep-ph hep-lathep-thnucl-th
keywords chemicalchiralentanglementpotentialrealdeconfinementeffectiveendpoint
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We extend the Polyakov-loop extended Nambu-Jona-Lasinio (PNJL) model by introducing an effective four-quark vertex depending on Polyakov loop. The effective vertex generates entanglement interactions between Polyakov loop and chiral condensate. The new model is consistent with lattice QCD data at imaginary quark-number chemical potential and real and imaginary isospin chemical potentials, particularly on strong correlation between the chiral and deconfinement transitions and also on the quark-mass dependence of the order of the Roberge-Weiss endpoint predicted by lattice QCD very lately. We investigate an influence of the entanglement interactions on a location of the tricritical point at real isospin chemical potential and a location of the critical endpoint at real quark-number chemical potential.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. The Roberge-Weiss transition as a probe for conformality in many-flavor QCD

    hep-lat 2026-04 unverdicted novelty 7.0

    For eight-flavor QCD the Roberge-Weiss transition temperature vanishes in the chiral limit, placing the theory inside the conformal window.

  2. CP-violating multi-field phase transitions and gravitational waves in a hidden NJL sector

    hep-ph 2026-04 unverdicted novelty 5.0

    Multi-field CP-violating phase transitions in a hidden NJL sector produce undetectable stochastic gravitational waves but remain cosmologically viable due to prompt domain wall collapse.

  3. CP-violating multi-field phase transitions and gravitational waves in a hidden NJL sector

    hep-ph 2026-04 unverdicted novelty 5.0

    Multi-field tunneling analysis in a CP-violating NJL model yields a slow transition (β/H ~ 100) whose stochastic gravitational-wave signal is detectable by μAres and insensitive to the CP angle.