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Nuclear level density and γ-ray strength function of Ni67 and the impact on the i process
- Ingeberg, VW;
- Siem, S;
- Wiedeking, M;
- Choplin, A;
- Goriely, S;
- Siess, L;
- Abrahams, KJ;
- Arnswald, K;
- Garrote, F Bello;
- Bleuel, DL;
- Cederkäll, J;
- Christoffersen, TL;
- Cox, DM;
- De Witte, H;
- Gaffney, LP;
- Görgen, A;
- Henrich, C;
- Illana, A;
- Jones, P;
- Kheswa, BV;
- Kröll, T;
- Majola, SNT;
- Malatji, KL;
- Ojala, J;
- Pakarinen, J;
- Rainovski, G;
- Reiter, P;
- von Schmid, M;
- Seidlitz, M;
- Tveten, GM;
- Warr, N;
- Zeiser, F
- et al.
Abstract
Proton-γ coincidences from (d,p) reactions between a Ni66 beam and a deuterated polyethylene target have been analyzed with the inverse-Oslo method to find the nuclear level density (NLD) and γ-ray strength function (γSF) of Ni67. The Ni66(n,γ) capture cross section has been calculated using the Hauser-Feshbach model in TALYS using the measured NLD and γSF as constraints. The results confirm that the Ni66(n,γ) reaction acts as a bottleneck when relying on one-zone nucleosynthesis calculations. However, the impact of this reaction is strongly dampened in multizone models of low-metallicity AGB stars experiencing i-process nucleosynthesis.
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