Nuclear level density and γ -ray strength function of Ni 67 and the impact on the i process

dc.contributor.authorAbrahams, Kenzo J
dc.contributor.authorIngeberg, Vetle Wegner
dc.contributor.authorSiem, Sunniva
dc.date.accessioned2026-01-13T07:27:55Z
dc.date.available2026-01-13T07:27:55Z
dc.date.issued2025
dc.description.abstractProton-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.
dc.identifier.citationIngeberg, V.W., Siem, S., Wiedeking, M., Choplin, A., Goriely, S., Siess, L., Abrahams, K.J., Arnswald, K., Bello Garrote, F., Bleuel, D.L. and Cederkäll, J., 2025. Nuclear level density and γ-ray strength function of Ni 67 and the impact on the i process. Physical Review C, 111(1), p.015803.
dc.identifier.urihttps://doi.org/10.1103/PhysRevC.111.015803
dc.identifier.urihttps://hdl.handle.net/10566/21686
dc.language.isoen
dc.publisherAmerican Physical Society
dc.subjectNuclear
dc.subjectLevel Density
dc.subjectNuclear Reaction Rates
dc.subjectGamma Ray Strength Functions
dc.subjectNuclear Astrophysics
dc.titleNuclear level density and γ -ray strength function of Ni 67 and the impact on the i process
dc.typeArticle

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