A. Simon, J. Koros, O. Olivas-Gomez, R. Kelmar, E. Churchman, A. M. Clark, C. Harris, S. L. Henderson, S. E. Kelly, P. Millican, A. Palmisano-Kyle, C. S. Reingold, D. Robertson, E. Stech, A. Spyrou, W. P. Tan
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Abstract
The \(^{90}\)Zr(p,\(\gamma \))\(^{91}\)Nb reaction is one of the important reactions in the \(A\approx 90\) mass region and part of the nucleosynthesis path responsible for production of \(^{92}\)Mo during the \(\gamma \)-process. Discrepant data in the literature provide a cross section that varies up to 30% within the Gamow window for the \(^{90}\)Zr(p,\(\gamma \))\(^{91}\)Nb reaction. Thus, the cross section measurements of \(^{90}\)Zr(p,\(\gamma \))\(^{91}\)Nb reaction were revisited using the \(\gamma \)-summing technique. The results are consistent with the lower-value cross sections found in the literature. Based on the new data an updated reaction rate for \(^{90}\)Zr(p,\(\gamma \))\(^{91}\)Nb is provided that is up to 20% higher than that obtained from the non-smoker code.
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