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Color-flavor locked strange matter

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arxiv hep-ph/0211070 v1 pith:WCJY2SNN submitted 2002-11-05 hep-ph

Color-flavor locked strange matter

classification hep-ph
keywords matterstatestrangedeltaequationpairingabsolutelyaccurate
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We analyze how the CFL states in dense matter work in the direction of enhancing the parameter space for absolutely stable phases (strange matter). We find that the "CFL strange matter" phase can be the true ground state of hadronic matter for a much wider range of the parameters of the model (the gap of the QCD Cooper pairs $\Delta$, the strange quark mass $m_s$ and the Bag Constant $B$) than the state without any pairing, and derive a full equation of state and an accurate analytic approximation to the lowest order in $\Delta$ and $m_{s}$ which may be directly used for applications. The effects of pairing on the equation of state are found to be small (as previously expected) but not negligible and may be relevant for astrophysics.

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Cited by 3 Pith papers

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    Fisher-matrix forecasts show Cosmic Explorer and Einstein Telescope can probe sub-solar PBHs to z~3 and distinguish PBHs from neutron stars up to z~0.2 via lack of tidal deformability.

  2. Anisotropic strange quark stars with a non-linear equation-of-state

    gr-qc 2019-07 unverdicted novelty 4.0

    Exact analytical solution for anisotropic CFL strange quark stars with non-linear EOS, satisfying energy conditions, yielding mass-radius profiles and compactness values.

  3. Radial oscillations of quark stars in light of current astrophysical constraints: A comparative study

    gr-qc 2026-06 unverdicted novelty 3.0

    Comparative numerical study of radial modes in strange quark stars using CFL, interacting, and linear causal EOS shows all satisfy current mass-radius bounds and produce 4-7 kHz fundamental frequencies.