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Issue A&A
Volume 429, Number 2, January II 2005
Page(s) L29 - L32
Section Letters
DOI http://dx.doi.org/10.1051/0004-6361:200400100



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. Hillebrandt

Max-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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