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NSR database version of April 29, 2024.

Search: Author = A.Chevis

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2021CO11      Phys.Rev. C 104, 024620 (2021)

K.J.Cook, A.Chevis, T.K.Eriksen, E.C.Simpson, T.Kibedi, L.T.Bezzina, A.C.Berriman, J.Buete, I.P.Carter, M.Dasgupta, D.J.Hinde, D.Y.Jeung, P.McGlynn, S.Parker-Steele, B.M.A.Swinton-Bland, T.Tanaka, W.Wojtaczka

High-precision proton angular distribution measurements of ¹²C (p, p') for the decay branching ratio of the Hoyle state

NUCLEAR REACTIONS ¹²C(p, p'), E=10.20-10.70 MeV from 14UD electrostatic accelerator at HIAF-ANU facility; measured E(p), I(p), p(θ), differential σ(θ, E) for the first 2+ and second 0+ (Hoyle) state using the Breakup Array for Light Nuclei (BALiN) array of wedge shaped segmented double-sided silicon detectors (DSSDs), configured as two ΔE-E telescopes; deduced total σ(E) for the population of the first 2+ and second 0+ (Hoyle) state in ¹²C, thick target yields. Discussed radiative width of the Hoyle state, and possible application of measured cross sections for investigating cluster structures in ¹³N. Relevance to rate of carbon production in stars via radiative decay of the Hoyle state.

doi: 10.1103/PhysRevC.104.024620
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD1006.