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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 7.

Thermal index Γth as a function of number density for our virial approximation (blue solid line) and several EOSs from CompOSE (dashed lines). The left and right panels display the nuclear thermal index (Equation (29)) and the full thermal index (Equation (24)), respectively, for a proton fraction Yp = 0.2 and at a temperature of T = 15 MeV (top) and at a temperature of T = 50 MeV (bottom). Note the different scales in the y-axis of the left and right panels. Horizontal dotted lines represent the values of Γth in both the relativistic and nonrelativistic limits.

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