measurement of the branching ratio for β-delayed α decay of 16n

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ID: 228840
2016
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Abstract
While the C12(α,γ)16O reaction plays a central role in nuclear astrophysics, the cross section at energies relevant to hydrostatic helium burning is too small to be directly measured in the laboratory. The β-delayed α spectrum of 16N can be used to constrain the extrapolation of the E1 component of the S-factor; however, with this approach the resulting S-factor becomes strongly correlated with the assumed βα branching ratio. We have remeasured the βα branching ratio by implanting 16N ions in a segmented Si detector and counting the number of βα decays relative to the number of implantations. Our result, 1.49(5)×10−5, represents a 24% increase compared to the accepted value and implies an increase of ≈10% in the extrapolated S-factor.
Reference Key
refsgaard2016physicsmeasurement Use this key to autocite in the manuscript while using SciMatic Manuscript Manager or Thesis Manager
Authors ;J. Refsgaard;O.S. Kirsebom;E.A. Dijck;H.O.U. Fynbo;M.V. Lund;M.N. Portela;R. Raabe;G. Randisi;F. Renzi;S. Sambi;A. Sytema;L. Willmann;H.W. Wilschut
Journal ACS chemical biology
Year 2016
DOI
10.1016/j.physletb.2015.11.047
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