Measurement of the branching ratio for β\beta-delayed α\alpha decay of 16^{16}N

Jun 30, 2015
6 pages
Published in:
  • Phys.Lett.B 752 (2016) 296-301
  • Published: Jan 10, 2016
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Abstract: (Elsevier)
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 16 N 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 16 N 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.
  • 23.40.-s
  • 26.20.Fj
  • 27.20.+n
  • β decay
  • Stellar helium burning
  • Properties of specific nuclei 6≤A≤19
  • Properties of specific nuclei [formula omitted]