Abstract
Precise knowledge of the branching ratio in the α decay of is important for accurate measurement of the cross section, the reaction involved in the termination of the astrophysical process. The branching ratio was determined from independent measurements of α and γ spectra of bismuth samples simultaneously irradiated by neutrons near the core of the Soreq research reactor (IRR1). The branching ratio was found to be , consistent with the results of several measurements performed six decades ago. As a by-product value the thermal cross section was measured to be mb.
- Received 26 October 2017
DOI:https://doi.org/10.1103/PhysRevC.97.034303
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