Neutrino transport in core collapse supernovae

DOI10.1016/S0377-0427(99)00162-4zbMath0946.76063OpenAlexW2995130828MaRDI QIDQ1807725

O. E. B. Messer, Anthony Mezzacappa

Publication date: 23 November 1999

Published in: Journal of Computational and Applied Mathematics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1016/s0377-0427(99)00162-4

zbMATH Keywords

spherical symmetryradiation transportcore hydrodynamicsmultigroup flux-limited diffusionneutrino Boltzmann equationsneutrino transportshock-revival mechanism

Mathematics Subject Classification ID

Finite difference methods applied to problems in fluid mechanics (76M20) Rarefied gas flows, Boltzmann equation in fluid mechanics (76P05) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Computational methods for problems pertaining to astronomy and astrophysics (85-08)

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Cites Work

• Asymptotic solutions of numerical transport problems in optically thick, diffusive regimes
• Tensor Artificial Viscosity for Numerical Hydrodynamics
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