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Pressure and speed of sound in two-flavor color-superconducting quark matter at next-to-leading order

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arxiv 2403.18010 v2 pith:XITLP5LR submitted 2024-03-26 hep-ph nucl-th

Pressure and speed of sound in two-flavor color-superconducting quark matter at next-to-leading order

classification hep-ph nucl-th
keywords quarkmatterdensitieshighordersoundspeedcolor-superconducting
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Deconfined quark matter at asymptotically high densities is weakly coupled, due to the asymptotic freedom of Quantum Chromodynamics. In this weak-coupling regime, bulk thermodynamic properties of quark matter, assuming a trivial ground state, are currently known to partial next-to-next-to-next-to-leading order. However, the ground state at high densities is expected to be a color superconductor, in which the excitation spectrum of (at least some) quarks exhibit a gap with a non-perturbative dependence on the strong coupling. In this work, we calculate the thermodynamic properties of color-superconducting quark matter at high densities and zero temperature at next-to-leading order (NLO) in the coupling in the presence of a finite gap. We work in the limit of two massless quark flavors, which corresponds to deconfined symmetric nuclear matter, and further assume that the gap is small compared to the quark chemical potential. In these limits, we find that the NLO corrections to the pressure and speed of sound are comparable in size to the leading-order effects of the gap, and further increase both quantities above their values for non-superconducting quark matter. We also provide a parameterization of the NLO speed of sound to guide phenomenology in the high-density region, and we furthermore comment on whether our findings should be expected to extend to the case of three-flavor quark matter of relevance to neutron stars.

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Cited by 2 Pith papers

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  1. Neutrino absorption in two-flavor color-superconducting quark matter

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    In 2SC quark matter, neutrino absorption is dominated by strange-quark capture at low temperature, and a degenerate neutrino gas at electron lepton fraction 0.1 has a mean free path of meters or less.

  2. Updated Astrophysical Equation-of-State Constraints on the Color-Superconducting Gap

    hep-ph 2025-08 accept novelty 5.0

    New NICER data plus a two-GP Bayesian analysis confirm the astrophysical upper bound on the CFL color-superconducting gap for baryon chemical potentials from 2.1 to 3.2 GeV.