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A&A 429, L29-L32 (2005)
DOI: 10.1051/0004-6361:200400100
Letter
The distributed burning regime in type Ia supernova models
F. K. Röpke and W. HillebrandtMax-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 85741 Garching, Germany
e-mail: [fritz;wfh]@mpa-garching.mpg.de
(Received 4 October 2004 / Accepted 5 November 2004 )
Abstract
The deflagration mode of flame propagation in type Ia supernova (SN Ia) models requires a correct description of the interaction
of the flame with turbulent motions. It is well-known that
turbulent combustion proceeds in different regimes. For most parts of the
deflagration in SNe Ia the flamelet regime applies. This has been modeled in previous multi-dimensional simulations. However,
at late stages of the explosion, the
flame will propagate in the so-called distributed regime. We
investigate the effects of this regime on SN Ia models in a first
and simplified approach and show that the trend of effects seems
capable of curing some problems of current pure deflagration
models.
Key words: stars: supernovae: general -- hydrodynamics -- methods: numerical
© ESO 2004
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