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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 5.

Comparison of the radial profiles of several quantities against the isotropic radial coordinate r between Weakhub (Con) and NuLib at the moment of core bounce of a 15 M star. The dashed lines and solid lines correspond to the results obtained by Gmunu with NuLib and Weakhub (Con) (Weakhub with a conventional set of interactions), respectively. The profiles include rest mass density ρ, radial velocity v r /c, matter temperature T, entropy per baryon s, neutrino rms energy observed in the fluid comoving frame ﹩\sqrt{\langle {\epsilon }_{{\nu }_{l}}^{2}\rangle }﹩, and electron fraction Y e . The results obtained by using Weakhub (Con) quantitatively agree with the results obtained using NuLib.

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