The -process nucleosynthesis in the carbon deflagration model for type Ia supernovae

Kusakabe, Motohiko*; Iwamoto, Nobuyuki ; Nomoto, Kenichi*

We calculate nucleosynthesis of proton-rich isotopes in the Carbon deflagration model for Type Ia supernova. We investigate the influence of variations int he C/O ratios and $^{22}$ Ne abundances left in accreting CO white dwarf on the -process nucleosynthesis. We compare the yields of $^{56}$ Fe and -nuclei in Type Ia and Type II supernovae, and obtain a result that C-deflagration supernovae can contribute to the galactic evolution (and the solar system) of the -nuclei.

Language	:	English
Journal	:	Nuclear Physics A
Volume	:	758
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Pages	:	p.459c - 462c
Publication Year/Month	:	2005/07
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Registration No. : AA20060183
JAEA Abstracts No. : 34000801
Paper Submission No. : 919

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