References quoted in the XUNDL dataset: 28SI 28SI(A,A'):XUNDL-8
3 references found.
Clicking on a keynumber will list datasets that reference the given article.
Phys.Rev. C 95, 024319 (2017)
P.Adsley, D.G.Jenkins, J.Cseh, S.S.Dimitrova, J.W.Brummer, K.C.W.Li, D.J.Marin-Lambarri, K.Lukyanov, N.Y.Kheswa, R.Neveling, P.Papka, L.Pellegri, V.Pesudo, L.C.Pool, G.Riczu, F.D.Smit, J.J.van Zyl, E.Zemlyanaya
α clustering in 28Si probed through the identification of high-lying 0+ states
NUCLEAR REACTIONS 28Si(α, α'), E=200 MeV; measured scattered particles, σ(θ) using K600 magnetic spectrometer at iThemba LABS, natural Si target. 28Si; deduced levels, L-transfers, J, π, high-lying 0+ states. Comparison with multichannel dynamical symmetry (MUSY) calculations.
doi: 10.1103/PhysRevC.95.024319
Phys.Rev. C 102, 015801 (2020)
P.Adsley, A.M.Laird, Z.Meisel
Status of the 24Mg (α, γ)28Si reaction rate at stellar temperatures
NUCLEAR REACTIONS 28Si(α, α'), E*=6-14 MeV; 28Si(p, p'), E=18, 295 MeV; 28Si(e, e'), E*=10-13 MeV; analyzed experimental and evaluated data for levels, resonances, J, π of 28Si. 24Mg(α, γ), T=0.01-1.25 GK; calculated astrophysical reaction rates using RATESMC Monte Carlo code and updated nuclear data for levels in 28Si; discussed effect on x-ray burst light curve. 28Si; analyzed levels, resonances J, π, resonance strengths.
doi: 10.1103/PhysRevC.102.015801
Phys.Rev. C 103, 044315 (2021)
P.Adsley, V.O.Nesterenko, M.Kimura, L.M.Donaldson, R.Neveling, J.W.Brummer, D.G.Jenkins, N.Y.Kheswa, J.Kvasil, K.C.W.Li, D.J.Marin-Lambarri, Z.Mabika, P.Papka, L.Pellegri, V.Pesudo, B.Rebeiro, P.-G.Reinhard, F.D.Smit, W.Yahia-Cherif
Isoscalar monopole and dipole transitions in 24Mg, 26Mg, and 28Si
NUCLEAR REACTIONS 24,26Mg, 28Si(α, α'), E=200 MeV; measured E(α), I(α), differential σ(θ) using K600 magnetic spectrometer for momentum analysis of α particles, and two multiwire drift chambers and two plastic scintillators at the iThemba LABS accelerator facility. 24,26Mg, 28Si; deduced levels, J, π, deformation parameters, percentage of the energy weighted sum rule (EWSR) for a level, B(E1), strength distributions for isoscalar dipole (IS1) and isoscalar monopole transitions (IS0), configurations. Comparison with Skyrme quasiparticle random-phase approximation (QRPA) and antisymmetrized molecular dynamics+generator coordinate method (AMD+GCM) calculations, and with experimental data in the ENSDF database.
doi: 10.1103/PhysRevC.103.044315