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Radiation hydrodynamics with neutrinos - Variable Eddington factor method for core-collapse supernova simulations

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Rampp,  M.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

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Janka,  H. Th.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

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Rampp, M., & Janka, H. T. (2002). Radiation hydrodynamics with neutrinos - Variable Eddington factor method for core-collapse supernova simulations. Astronomy & Astrophysics, 396(1), 361-392.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0011-BBE0-D
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