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General-relativistic Radiation Transport Scheme in Gmunu. II. Implementation of Novel Microphysical Library for Neutrino Radiation—Weakhub

  • Authors: Harry Ho-Yin Ng, Patrick Chi-Kit Cheong, 志杰 張, Alan Tsz-Lok Lam, Tjonnie Guang Feng Li

Harry Ho-Yin Ng et al 2024 The Astrophysical Journal Supplement Series 272 .

  • Provider: AAS Journals

Caption: Figure 1.

Spectra of neutrino opacities defined in Equation (71) as a function of neutrino energy ε of the weak interactions included in Weakhub at thermodynamic point (I) in Table 3, which corresponds to the central region of s15s7b2 in Woosley & Weaver (1995). Note that the absorption opacities are computed using the full kinematics approach and all available corrections, and the scattering opacities incorporate all of the corrections as mentioned. Absorption processes, elastic scattering, inelastic scattering, and pair processes are represented by red, green, orange, and blue, respectively. We rescale opacities by multiplying 108 for ν e + inelastic scattering, 1010 for e e + annihilation, 1015 for NN bremsstrahlung, 107 for the plasma process, and 106 for the nuclear de-excitation process, respectively.

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