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Thermodynamic signatures do not uniquely identify deconfinement in neutron stars
The smallness of polytropic index $Γ_\varepsilon \lesssim 1.75$ and near conformality of sound velocity $c_s^2 \approx 1/3$ in neutron star matter are usually referred to as signals of the emergence of quark matter. We construct a density-resolved nucleonic reference domain in the \((P/P_{\rm free},
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