NSR Query Results
Output year order : Descending NSR database version of April 11, 2024. Search: Author = R.F.Hausman Found 6 matches. 1983GR12 Phys.Rev. C27, 2893 (1983) S.M.Grimes, S.D.Bloom, H.K.Vonach, R.F.Hausman, Jr. Spectral Distribution Calculations of the Level Density and Spin-Cutoff Parameters of 28Si NUCLEAR STRUCTURE 28Si; calculated level density, spin cutoff parameter. Spectral distribution method.
doi: 10.1103/PhysRevC.27.2893
1983MA45 Phys.Rev. C28, 1367 (1983) G.J.Mathews, S.D.Bloom, R.F.Hausman, Jr. Gamow-Teller Strength Function for 90Zr: Effects of spin and isospin exchange forces, and ground-state correlations RADIOACTIVITY 90Zr(β-); calculated Gamow-Teller strength function; deduced spin, isospin exchange force, ground state correlation effects. Shell model.
doi: 10.1103/PhysRevC.28.1367
1981BL17 Phys.Lett. 107B, 336 (1981) S.D.Bloom, C.D.Goodman, S.M.Grimes, R.F.Hausman, Jr. Gamow-Teller Strength Function for 26Mg → 26Al NUCLEAR REACTIONS 26Mg(p, n), E=120 MeV; calculated Gamow-Teller strength function distribution. Shell model.
doi: 10.1016/0370-2693(81)90336-1
1980BL06 Phys.Lett. 93B, 227 (1980) S.D.Bloom, S.M.Grimes, R.F.Hausman, Jr. A Monte Carlo Method for Calculating Strength Functions in Many-Fermion Systems NUCLEAR STRUCTURE 21Ne, 28Si; calculated Hamiltonian moments, strength functions. Monte-Carlo method, random vectors, many-fermion system.
doi: 10.1016/0370-2693(80)90500-6
1979GR07 Phys.Rev. C19, 2378 (1979) S.M.Grimes, S.D.Bloom, R.F.Hausman, Jr., B.J.Dalton Method for Calculating Operator Traces NUCLEAR STRUCTURE 21Ne; calculated level density, operator moments. Spectral distribution expansion.
doi: 10.1103/PhysRevC.19.2378
1978WO14 Phys.Rev. C18, 2052 (1978) C.Wong, S.D.Bloom, S.M.Grimes, R.F.Hausman, Jr., V.A.Madsen Population of the 1+ Levels in 58Co via the 58Fe(p, n) Reaction NUCLEAR REACTIONS 58Fe(p, n), E=16, 19.1, 20.2 MeV; measured σ(θ). 58Co deduced 1+ strength distribution, fractional M1 strengths. Compared with reaction data, shell model calculations.
doi: 10.1103/PhysRevC.18.2052
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