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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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.