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A&A 420, 411-422 (2004)
DOI: 10.1051/0004-6361:20035721
The cellular burning regime in type Ia supernova explosions
I. Flame propagation into quiescent fuel
F. K. Röpke1, W. Hillebrandt1 and J. C. Niemeyer21 Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 85741 Garching, Germany
e-mail: fritz@mpa-garching.mpg.de; wfh@mpa-garching.mpg.de
2 Universität Würzburg, Am Hubland, 97074 Würzburg, Germany
e-mail: niemeyer@astro.uni-wuerzburg.de
(Received 21 November 2003 / Accepted 4 March 2004 )
Abstract
We present a numerical investigation of the cellular burning
regime in Type Ia supernova explosions. This regime holds at small
scales (i.e. below the Gibson scale), which are unresolved in
large-scale Type Ia supernova simulations. The fundamental effects that
dominate the flame evolution here are the Landau-Darrieus instability
and its nonlinear stabilization, leading to a stabilization of the
flame in a cellular shape. The flame propagation into quiescent fuel
is investigated addressing the dependence of the simulation
results on the specific parameters of the numerical
setup. Furthermore, we investigate the flame stability at a range of fuel
densities. This is directly connected to the questions of active
turbulent combustion (a mechanism of flame destabilization and
subsequent self-turbulization) and a deflagration-to-detonation transition of
the flame. In our simulations we find no substantial destabilization
of the flame when propagating into quiescent fuels of densities down
to
, corroborating fundamental
assumptions of large-scale SN Ia explosion models. For these models,
however, we suggest an increased lower cutoff for the flame
propagation velocity to take the cellular burning regime into
account.
Key words: stars: supernovae: general -- hydrodynamics -- instabilities
Offprint request: F. K. Röpke, fritz@mpa-garching.mpg.de
© ESO 2004
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