NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = K.H.Chang Found 4 matches. 1988KR06 Phys.Rev.Lett. 60, 1475 (1988) R.M.Kremer, C.A.Barnes, K.H.Chang, H.C.Evans, B.W.Filippone, K.H.Hahn, L.W.Mitchell Coincidence Measurement of the 12C(α, γ)16O Cross Section at Low Energies NUCLEAR REACTIONS, ICPND 12C(α, γ), E(cm)=1.29-3 MeV; measured γ-spectra, γ(recoil)-coin; deduced γ yields, dipole capture σ(E), S-factor vs E.
doi: 10.1103/PhysRevLett.60.1475
1988WI12 Nucl.Instrum.Methods Phys.Res. A267, 242 (1988) M.Wiescher, J.Gorres, K.L.Kratz, B.Leist, K.H.Chang, B.W.Filippone, L.W.Mitchell, M.J.Savage, R.B.Vogelaar The Fabrication and Properties of a 22Na Target NUCLEAR REACTIONS 23Na(p, γ), E ≈ 310-340 keV; 19F(p, α), E ≈ 600-900 keV; measured thick target yield. 30Si(p, γ), E=620 keV; measured Eγ, Iγ. 24Mg(d, α), E not given; measured Eγ, Iγ; deduced 22Na target feasibility.
doi: 10.1016/0168-9002(88)90471-8
1987BA58 Phys.Lett. 197B, 315 (1987) C.A.Barnes, K.H.Chang, T.R.Donoghue, C.Rolfs, J.Kammeraad The 2H(d, γ)4He Reaction at Low Energy and the D-State Admixture in 4He NUCLEAR REACTIONS, ICPND 2H(d, γ), E(cm)=50-500 keV; measured σ(θ), σ(E); deduced dominant radiative capture amplitude character, astrophysical S-factor vs E. 4He deduced D-State admixture.
doi: 10.1016/0370-2693(87)90391-1
1987HA24 Phys.Rev. C36, 892 (1987) K.H.Hahn, K.H.Chang, T.R.Donoghue, B.W.Filippone Search for Nonresonant Capture in the 16O(α, γ)20Ne Reaction at Low Energies NUCLEAR REACTIONS, ICPND 16O(α, γ), E(cm)=1.7-2.35 MeV; measured σ(E), (20Ne)γ-coin, γ yields. 20Ne deduced resonances, Γ, resonance strength, nonresonant capture astrophysical S-factor.
doi: 10.1103/PhysRevC.36.892
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