References quoted in the XUNDL dataset: 34P 18O(18O,PNG):XUNDL-5
3 references found.
Clicking on a keynumber will list datasets that reference the given article.
Phys.Rev. C 80, 014302 (2009)
P.C.Bender, C.R.Hoffman, M.Wiedeking, J.M.Allmond, L.A.Bernstein, J.T.Burke, D.L.Bleuel, R.M.Clark, P.Fallon, B.L.Goldblum, T.A.Hinners, H.B.Jeppesen, S.Lee, I.-Y.Lee, S.R.Lesher, A.O.Macchiavelli, M.A.McMahan, D.Morris, M.Perry, L.Phair, N.D.Scielzo, S.L.Tabor, V.Tripathi, A.Volya
Approaching the "island of inversion": 34P
NUCLEAR REACTIONS 18O(18O, np), E=20, 24, 25, 30, 44 MeV; measured Eγ, Iγ, γγ-, pγ-coin, γ(θ), DSA and half-lives. 34P; deduced levels, J, π, multipolarities, transition strengths and configurations. Island of inversion. Comparison with shell-model calculations using a modified WBP interaction.
NUCLEAR STRUCTURE 32,34,36P; calculated levels, J, π and subshell occupancies using WBP interaction shell-model formalism.
doi: 10.1103/PhysRevC.80.014302
Priv.Comm. (2011)
P.C.Bender, S.L.Tabor, L.Hamilton, C.R.Hoffman, V.Tripathi, R.M.Clark, P.Fallon, A.O.Macchiavelli, S.Paschalis, M.Petri, C.Chiara, R.V.F.Janssens, T.Lauritsen, E.McCutchan, S.Zhu, X.Chen, W.Reviol, D.G.Sarantites, Y.Toh
Notes on 34P
NUCLEAR REACTIONS 18O(18O, np), E=25 MeV; measured Eγ, Iγ, γ(θ), γγ-, (proton)γ-coin, DSA using Gammasphere array and Microball. 34P; deduced levels, J, π, branching ratios, half-lives, multipolarity, mixing ratio, B(M1), B(E1), B(E2) and B(M2) strengths.
Phys.Rev. C 85, 044305 (2012)
P.C.Bender, S.L.Tabor, V.Tripathi, C.R.Hoffman, L.Hamilton, A.Volya, R.M.Clark, P.Fallon, A.O.Macchiavelli, S.Paschalis, M.Petri, M.P.Carpenter, R.V .F.Janssens, T.Lauritsen, E.A.McCutchan, D.Seweryniak, S.Zhu, C.J.Chiara, X.Chen, W.Reviol, D.G.Sarantites, Y.Toh
Multi-intruder structures in 34P
NUCLEAR REACTIONS 18O(18O, np), E=24 MeV; measured Eγ, Iγ, γ(θ), γγ-, (proton)γ-coin, half-lives by DSA using Gammasphere array and Microball. 34P; deduced levels, J, π, branching ratios, multipolarity, mixing ratio, B(M1), B(E1), B(E2), B(M2), B(E3) strengths. Comparisons with shell-model calculations.
doi: 10.1103/PhysRevC.85.044305