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The Thermal Index of Neutron-star Matter in the Virial Approximation

  • Authors: Giuseppe Rivieccio, Adriana Nadal-Matosas, Arnau Rios, Milton Ruiz

Giuseppe Rivieccio et al 2025 The Astrophysical Journal 987 .

  • Provider: AAS Journals

Caption: Figure 6.

Nuclear thermal index Equation (29) as a function of baryon number density for the HS(IUF) EOS taken from CompOSE database fixing Yp = 0.2. The dashed lines have been adjusted accounting for the binding energy while the solid lines have not. The line color changes with temperature from 5 to 45 MeV.

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