Alpha capture on 14C and its astrophysical implications

Details Alpha capture on 14C and its astrophysical implications Alpha capture on 14C and its astrophysical implications

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992nupha.548..414g&link_type=abstract

Nuclear Physics A, Volume 548, Issue 3, p. 414-426.

Physics

Nuclear Physics

21

Nuclear Reactions

Scientific paper

The reaction 14C(α, γ)18O has been measured in the alpha energy range of Eα = 1.14-2.33 MeV. The resonance strengths of the 4+ resonance at Eα = 1.14 MeV and of the 1- resonance at Eα = 1.79 MeV have been measured relative to the 14C(p, γ)15N resonance at Ep=0.528 MeV. Additionally, two nonresonant γ-transitions to the ground state and to the first excited state of 18O were found. The energy dependence of their cross sections can be described by the direct capture process and its interference with the two 1- resonances at Eα = 1.79 and 2.33 MeV.
Present address: EGG-Astrophysics Research Corp., Long Beach, CA, USA.

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