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NSR database version of April 29, 2024.

Search: Author = D.Zetterberg

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2022SI17      Phys.Rev. C 106, 015803 (2022)

A.Sieverding, J.S.Randhawa, D.Zetterberg, R.J.deBoer, T.Ahn, R.Mancino, G.Martinez-Pinedo, W.R.Hix

Role of low-lying resonances for the ¹⁰Be(p, α)⁷Li reaction rate and implications for the formation of the Solar System

NUCLEAR REACTIONS ¹⁰Be(p, α), (α, n), E not given; ¹⁰Be(ν, e^-), E=2.8-10 MeV; analyzed reaction rates, σ; deduced influence on the content of ¹⁰Be in supernovae environment. ¹⁰Be(p, α), E<1.5 MeV; analyzed reaction rate, experimental data on resonance in ¹¹B at 193 keV, ; deduced reaction rate, astrophysical S-factor. Showed that, with the new reaction rate, a low-mass corecollapse supernovae is unlikely to produce enough ¹⁰Be to explain the observed ¹⁰Be/⁹Be ratio in meteorites. Comparison to data from JINA-REACLIB.

doi: 10.1103/PhysRevC.106.015803
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