Volume 420, Number 1, June II 2004
|Page(s)||L1 - L4|
|Published online||14 May 2004|
Letter to the Editor
The case against the progenitor's carbon-to-oxygen ratio as a source of peak luminosity variations in type Ia supernovae
Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 85741 Garching, Germany e-mail: fritz;email@example.com
Corresponding author: F. K. Röpke, firstname.lastname@example.org
Accepted: 7 April 2004
One of the major challenges for theoretical modeling of type Ia supernova explosions is to explain the diversity of these events and the empirically established correlation between their peak luminosity and light curve shape. In the framework of the so-called Chandrasekhar mass models, the progenitor's carbon-to-oxygen ratio has been suggested as a principal source of peak luminosity variations due to a variation in the production of radioactive 56Ni during the explosion. We describe a mechanism resulting from an interplay between nucleosynthesis and turbulent flame evolution which counteracts such an effect. Based on three-dimensional simulations we argue that it is nearly balanced and only minor differences in the amount of synthesized 56Ni with varying carbon mass fraction in the progenitor can be expected. Therefore the progenitor's carbon-to-oxygen ratio is unlikely to account for the observed variations in type Ia supernova luminosity. We discuss possible effects on the calibration of cosmological measurements.
Key words: supernovae: general / hydrodynamics / nuclear reactions, nucleosynthesis, abundances
© ESO, 2004
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