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NSR database version of April 29, 2024.

Search: Author = J.Rohrich

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2021KI07      Phys.Rev. C 104, 024621 (2021)

J.Kiener, J.Bundesmann, I.Deloncle, A.Denker, V.Tatischeff, A.Gostojic, C.Hamadache, J.Rohrich, H.Benhabiles, I.Bourgaoub, A.Coc, F.Hammache, R.Mezhoud, J.Peyre

γ-ray emission in α-particle interactions with C, Mg, Si, and Fe at Eα = 50-90 MeV

NUCLEAR REACTIONS C(α, γ)10B/11B/12B/11C/12C/13C/14N/15N/15O, E=50, 60, 75, 90 MeV; Mg(α, γ)16O/20Ne/21Ne/21Na/22Na/23Na/23Mg/24Mg/25Mg/26Mg/26Al, E=50, 60, 75, 90 MeV; Si(α, γ)20Ne/22Ne/23Na/24Mg/25Mg/26Mg/26Al/27Al/28Si/29Si/30Si/30P/31P, E=50, 60, 75, 90 MeV; Fe(α, γ)52Cr/54Cr/51Mn/53Mn/54Mn/53Fe/54Fe/55Fe/56Fe/56Co/57Co, E=50, 60, 75, 90 MeV; measured Eγ, Iγ using three HPGe detectors and a LaBr3 scintillation detector at the center for proton therapy of the Helmholtz-Zentrum Berlin (HZB) in 2015 and 2016; deduced production σ(E) for γ lines of various isotopes. Comparison with previous experimental data at other Eα incident energies, and with TALYS theoretical calculations.

doi: 10.1103/PhysRevC.104.024621
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO2563.


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