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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 10.

Time evolution of far-field neutrino luminosities, ﹩{L}_{{\nu }_{l}}^{\mathrm{Euler}}﹩, observed by an Eulerian observer at a distance of 500 km from a collapsing 20 M star. Dashed lines and solid lines correspond to the results with the advanced set (I) and (II) interactions (i.e., Adv.I and Adv.II), respectively. Dashed–dotted lines, loosely dotted lines, and dotted lines correspond to the results of Adv.II with cutoff density values for ﹩{\nu }_{e}{\bar{\nu }}_{e}﹩ pair annihilation of ρ cut = 1011 g cm−3, ρ cut = 1012.5 g cm−3, and ρ cut = 0 without the conservation treatment in Equation (70), respectively.

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