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thornado+FLASH-X: A Hybrid Discontinuous Galerkin–Implicit-explicit and Finite-volume Framework for Neutrino-radiation Hydrodynamics in Core-collapse Supernovae

  • Authors: Eirik Endeve, Vassilios Mewes, J. Austin Harris, M. Paul Laiu, Ran Chu, Steven A. Fromm, Anthony Mezzacappa, O. E. Bronson Messer, W. Raphael Hix, Stephen W. Bruenn, Eric J. Lentz, Klaus Weide, Christian Y. Cardall, Ann S. Almgren, Anshu Dubey, Sean M. Couch, Philipp Mösta, Donald E. Willcox

Eirik Endeve et al 2026 The Astrophysical Journal Supplement Series 284 .

  • Provider: AAS Journals

Caption: Figure 6.

Results for the radiating sphere test at t = 104. Left panels show energy-integrated number densities (top panel) and energy densities (bottom panel) multiplied by r2 vs. radius. In each of these panels we show the comoving- and Eulerian-frame number and energy densities, and results have been scaled to values at the outer radial boundary. In the top left panel, we plot the comoving-frame number density ﹩[{D}_{\nu }(r)/{D}_{\nu }(r=1{0}^{4})]\times {(r/1{0}^{4})}^{2}﹩ (dotted black) and the Eulerian-frame number density ﹩[{N}_{\nu }(r)/{N}_{\nu }(r=1{0}^{4})]\times {(r/1{0}^{4})}^{2}﹩ (dotted blue). In the bottom-left panel, we plot the comoving-frame energy density ﹩[{J}_{\nu }(r)/{J}_{\nu }(r=1{0}^{4})]\times {(r/1{0}^{4})}^{2}﹩ (dotted black) and the Eulerian-frame energy density ﹩[{E}_{\nu }(r)/{E}_{\nu }(r=1{0}^{4})]\times {(r/1{0}^{4})}^{2}﹩ (dotted blue). In both of these panels, the analytical solution, obtained using Equation (149), is plotted for the comoving-frame quantity (solid black). In the right panel, spectral particle distributions are plotted for various radii. Analytic spectra are plotted for r = 101 (solid black) and r = 1.5 × 102 (solid blue). Numerically obtained spectra are plotted for r = 101 (black circles), r = 1.5 × 102 (blue circles), and r = 104 (red crosses).

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