Pauli degeneracy dominates pressure in dense matter, interactions set EOS stiffness, and pairing correlations add subleading corrections especially in quark matter, informing neutron star models.
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hep-ph 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
A van der Waals description with temperature-dependent degeneracy g(T) and effective chemical potential μ(T) reproduces the trace anomaly and its peak near the QCD crossover.
citing papers explorer
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Equation of State of Dense Matter: Pauli Degeneracy, Pairing Correlations, and Implications for Neutron Stars
Pauli degeneracy dominates pressure in dense matter, interactions set EOS stiffness, and pairing correlations add subleading corrections especially in quark matter, informing neutron star models.
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Trace anomaly, effective degrees of freedom, and chemical potential effects near the QCD crossover
A van der Waals description with temperature-dependent degeneracy g(T) and effective chemical potential μ(T) reproduces the trace anomaly and its peak near the QCD crossover.