التفاصيل البيبلوغرافية
| العنوان: |
IMPACT OF NEW GAMOW–TELLER STRENGTHS ON EXPLOSIVE TYPE IA SUPERNOVA NUCLEOSYNTHESIS. |
| المؤلفون: |
Kanji Mori1,2 kanji.mori@nao.ac.jp, Michael A. Famiano1,3 michael.famiano@wmich.edu, Toshitaka Kajino1,2,4 kajino@nao.ac.jp, Toshio Suzuki1,5 suzuki@phys.chs.nihon-u.ac.jp, Jun Hidaka6 jun.hidaka@meisei-u.ac.jp, Michio Honma7 m-honma@u-aizu.ac.jp, Koichi Iwamoto8 iwamoto@phys.cst.nihon-u.ac.jp, Ken'ichi Nomoto9,10 nomoto@astron.s.u-tokyo.ac.jp, Takaharu Otsuka11,12 otsuka@phys.s.u-tokyo.ac.jp |
| المصدر: |
Astrophysical Journal. 12/20/2016, Vol. 833 Issue 2, p1-1. 1p. |
| مصطلحات موضوعية: |
*SUPERNOVAE, *NUCLEAR reactions, *NUCLEOSYNTHESIS, *COSMIC abundances, *BETA decay |
| مستخلص: |
Recent experimental results have confirmed a possible reduction in the Gamow–Teller (GT+) strengths of pf-shell nuclei. These proton-rich nuclei are of relevance in the deflagration and explosive burning phases of SNe Ia. While prior GT strengths result in nucleosynthesis predictions with a lower-than-expected electron fraction, a reduction in the GT+ strength can result in a slightly increased electron fraction compared to previous shell model predictions, though the enhancement is not as large as previous enhancements in going from rates computed by Fuller, Fowler, and Newman based on an independent particle model. A shell model parametrization has been developed that more closely matches experimental GT strengths. The resultant electron-capture rates are used in nucleosynthesis calculations for carbon deflagration and explosion phases of SNe Ia, and the final mass fractions are compared to those obtained using more commonly used rates. [ABSTRACT FROM AUTHOR] |
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