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Statistical Analysis of Neutron Star Cooling: Implications for the Nuclear Equation of State and Nucleon Pairing
We perform a statistical analysis of the thermal evolution of isolated neutron stars by confronting theoretical cooling curves with luminosity-age measurements for 24 sources. For each object, we explore five purely nucleonic equations of state (APR4, FSU2R, DD2, IST, and NL3$ωρ$) combined with repr
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