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Nucleosynthesis as a result of multiple delayed detonations in Type Ia Supernovae

Domingo Garcia-Senz·Eduardo Bravo
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Abstract

The explosion of a white dwarf of mass 1.36 M$_\odot$ has been simulated in three dimensions with the aid of a SPH code. The explosion follows the delayed detonation paradigma. In this case the deflagration-detonation transition is induced by the large corrugation of the flame front resulting from Rayleigh-Taylor instability and turbulence. The nucleosynthetic yields have been calculated, showing that some neutronized isotopes such as 54^Fe or 58^Ni are not overproduced with respect to the solar system ratios. The distribution of intermediate-mass elements is also compatible with the spectra of normal SNIa. The excepcion is, however, the abundance of carbon and oxygen, which are overproduced.

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Domingo Garcia-Senz, Eduardo Bravo. 2002-10-16. Nucleosynthesis as a result of multiple delayed detonations in Type Ia Supernovae. https://doi.org/10.1016/s0375-9474(03)00847-9

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