Abstract
The 90Zr(p,γ)91Nb reaction is one of the important reactions in the A≈90 mass region and part of the nucleosynthesis path responsible for production of 92Mo during the γ-process. Discrepant data in the literature provide a cross section that varies up to 30% within the Gamow window for the 90Zr(p,γ)91Nb reaction. Thus, the cross section measurements of 90Zr(p,γ)91Nb reaction were revisited using the γ-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 90Zr(p,γ)91Nb is provided that is up to 20% higher than that obtained from the non-smoker code.
Original language | English |
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Article number | 57 |
Journal | European Physical Journal A |
Volume | 61 |
Issue number | 3 |
DOIs | |
State | Published - 1 Mar 2025 |
Externally published | Yes |
ASJC Scopus subject areas
- Nuclear and High Energy Physics