NSR Query Results
Output year order : Descending NSR database version of April 29, 2024. Search: Author = C.D.Hoyle Found 5 matches. 1983AD03 Phys.Rev. C27, 2833 (1983) E.G.Adelberger, M.M.Hindi, C.D.Hoyle, H.E.Swanson, R.D.Von Lintig, W.C.Haxton Beta Decays of 18Ne and 19Ne and Their Relation to Parity Mixing in 18F and 19F NUCLEAR STRUCTURE 18,19F, 19,21Ne, 21Na; calculated B(λ). 18,19Ne, 21Na; calculated Gamow-Teller transition strengths. Shell model. RADIOACTIVITY 18Ne(β+) [from O(3He, xn), E=12 MeV]; 19Ne(β+) [from 19F(p, n), E=6.4 MeV]; measured Eγ, Iγ; deduced ft. 18,19F levels deduced β-branching ratios, relative Iγ, parity mixing effects. Shell model. Natural O2, SF6 gas targets.
doi: 10.1103/PhysRevC.27.2833
1983HO05 Phys.Rev. C27, 1244 (1983) C.D.Hoyle, E.G.Adelberger, J.S.Blair, K.A.Snover, H.E.Swanson, R.D.Von Lintig Isospin Mixing in 24Mg RADIOACTIVITY 24Al(β+) [from 24Mg(p, n)]; measured βγ CP asymmetry, Eγ, Iγ; deduced isospin forbidden transition matrix element. 24Mg levels deduced isospin mixing.
doi: 10.1103/PhysRevC.27.1244
1982RA05 Nucl.Phys. A378, 29 (1982) A.Ray, C.D.Hoyle, E.C.Adelberger Beta Decay of 24Al and 24mAl RADIOACTIVITY 24,24mAl [from 24Mg(p, n)]; measured Eγ, Iγ; deduced log ft, Gamow-Teller matrix elements. Shell model calculations.
doi: 10.1016/0375-9474(82)90381-5
1981AD01 Phys.Rev.Lett. 46, 695 (1981) E.G.Adelberger, C.D.Hoyle, H.E.Swanson, R.D.Von Lintig O+ → O- β+ Decay of 18Ne and the Determination of F(π) RADIOACTIVITY 18Ne [from O(3He, xn), E=12 MeV]; measured β-delayed Eγ, Iγ; 18F levels deduced β-branching, strength of parity-nonconserving effects. Pion exchange, parity-mixing operator in nucleon-nucleon interaction.
doi: 10.1103/PhysRevLett.46.695
1981AD05 Phys.Rev. C24, 313 (1981) E.G.Adelberger, M.M.Hindi, C.D.Hoyle, H.E.Swanson, R.D.Von Lintig (1/2)+ → (1/2)- Beta Decay of 19Ne and the Parity Nonconserving NN Force RADIOACTIVITY 19Ne [from 19F(p, n), E=6.4 MeV]; measured γγγ-coin; deduced Iβ, log ft. 19F deduced parity mixing effect smaller than shell model predictions.
doi: 10.1103/PhysRevC.24.313
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