[c]STELLA: Multi-group Radiation Hydrodynamics Code[/c][/b]
Abstract: STELLA is a one-dimensional multi-group radiation hydrodynamics code. STELLA incorporates implicit hydrodynamics coupled to a multi-group non-equilibrium radiative transfer for modeling SN II-L light curves. The non-equilibrium description of radiation is crucial for this problem since the presupernova envelope may be of low mass and very dilute. STELLA implicitly treats time dependent equations of the angular moments of intensity averaged over a frequency bin. Local thermodynamic equilibrium is assumed to determine the ionization levels of materials.
Credit: Blinnikov, Sergei I.; Bartunov, Oleg S.
Site: https://dau.itep.ru/sn/code/stella
http://adsabs.harvard.edu/abs/1993A%26A...273..106B
Bibcode: 2011ascl.soft08013B
ID: ascl:1108.013
STELLA: Multi-group Radiation Hydrodynamics Code
STELLA: Multi-group Radiation Hydrodynamics Code
Last edited by Ada Coda on Sun Mar 17, 2019 6:53 pm, edited 1 time in total.
Reason: Updated code entry.
Reason: Updated code entry.
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