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斉藤 照之; 松尾 正之*
no journal, ,
近年の連星中性子星合体の観測に伴い、理論方面からも-processに関与するより正確な核データなどの評価が求められている。そこで我々は直接中性子捕獲について、従来はポテンシャルモデルを用いるところをRPAによって評価する手法を開発してきた。最近になって対相関を取り入れた計算が可能になり、これによって(n,g)生成核が偶々核の場合にも同理論が広く適用できるようになった。今回は我々の最新の(n,g)断面積の計算結果について報告する。
斉藤 照之; 松尾 正之*
no journal, ,
The radiative neutron capture reactions in r-process evaluation are described mainly in terms of two mechanisms, the compound nuclear (CN) process and the direct capture (DC) process. Several studies suggest that the existence of resonances near the one neutron separation energy, such as the pygmy dipole resonance and the scissors mode, may influence r-process nucleosynthesis and its final abundance pattern. However, these discussions are based on the CN process. On the other hand, it is expected that the DC contributions may be dominanted in neutron-rich nuclei. Therefore we ask the question whether the resonances may also affect the r process not through the CN process. From this point of view, we have developed new neutron capture model based on Density Functional Theory and continuum QRPA. This model can take into account pair correlation, collectivity (e.g. surface vibrational modes) and resonances as intermediate states of (n,g) reactions. We will present our numerical calculations, Zn(n,g)
Zn and
Ge(n,g)
Ge as examples, and discuss the effects of pair correlation, collectivity and resonances for the neutron capture reactions. In addition, we will show our recent attempts to apply to the case of (n,g) final states are odd-odd nuclei by using proton-neutron continuum QRPA.