References quoted in the XUNDL dataset: 118SN COULOMB EXCITATION:XUNDL-9
4 references found.
Clicking on a keynumber will list datasets that reference the given article.
Phys.Lett. B 695, 110 (2011)
A.Jungclaus, J.Walker, J.Leske, K.-H.Speidel, A.E.Stuchbery, M.East, P.Boutachkov, J.Cederkall, P.Doornenbal, J.L.Egido, A.Ekstrom, J.Gerl, R.Gernhauser, N.Goel, M.Gorska, I.Kojouharov, P.Maier-Komor, V.Modamio, F.Naqvi, N.Pietralla, S.Pietri, W.Prokopowicz, H.Schaffner, R.Schwengner, H.-J.Wollersheim
Evidence for reduced collectivity around the neutron mid-shell in the stable even-mass Sn isotopes from new lifetime measurements
NUCLEAR REACTIONS C, Gd, Cu(112Sn, 112Sn'), (114Sn, 114Sn'), (116Sn, 116Sn'), (118Sn, 118Sn'), (120Sn, 120Sn'), (122Sn, 122Sn'), (124Sn, 124Sn'), E=4 MeV/nucleon; measured Eγ, Iγ, particle-γ coin. 112,114,116,118,120,122,124Sn; deduced energy levels, lifetimes, B(E2). Comparison with shell model calculations.
doi: 10.1016/j.physletb.2010.11.012
Phys.Rev. C 92, 041303 (2015)
J.M.Allmond, A.E.Stuchbery, A.Galindo-Uribarri, E.Padilla-Rodal, D.C.Radford, J.C.Batchelder, C.R.Bingham, M.E.Howard, J.F.Liang, B.Manning, S.D.Pain, N.J.Stone, R.L.Varner, C.-H.Yu
Investigation into the semimagic nature of the tin isotopes through electromagnetic moments
NUCLEAR REACTIONS C, Ti(112Sn, 112Sn'), (114Sn, 114Sn'), (116Sn, 116Sn'), (118Sn, 118Sn'), (120Sn, 120Sn'), (122Sn, 122Sn'), (124Sn, 124Sn'), E=2.9 MeV/nucleon; measured Eγ, Iγ, (particle)γ-coin, (particle)γ(θ), absolute cross sections using CLARION Ge array, BareBall CsI array, and a Bragg curve detector at HRIBF-ORNL. 112,114,116,118,120,122,124Sn; deduced E2 matrix elements, B(E2), quadrupole moments, g-factors for the first 2+ states. Coulomb excitation and GOSIA analysis. Comparison with shell model calculations, and several previous experimental measurements. Systematic differences found between results from the present experiment and a recent experiment using DSAM technique.
doi: 10.1103/PhysRevC.92.041303
At.Data Nucl.Data Tables 107, 1 (2016), Erratum At.Data Nucl.Data Tables 114, 371 (2017)
B.Pritychenko, M.Birch, B.Singh, M.Horoi
Tables of E2 transition probabilities from the first 2+ states in even-even nuclei
COMPILATION 4,6,8,10He, 6,8,10,12,14Be, 10,12,14,16,18,20C, 12,14,16,18,20,22,24,26O, 16,18,20,22,24,26,28,30,32Ne, 20,22,24,26,28,30,32,34,36,38Mg, 24,26,28,30,32,34,36,38,40,42Si, 28,30,32,34,36,38,40,42,44,46S, 32,34,36,38,40,42,44,46,48Ar, 36,38,40,42,44,46,48,50,52,54Ca, 42,44,46,48,50,52,54,56,58Ti, 46,48,50,52,54,56,58,60,62,64Cr, 48,50,52,54,56,58,60,62,64,66,68Fe, 52,54,56,58,60,62,64,66,68,70,72,74,76Ni, 60,62,64,66,68,70,72,74,76,78,80Zn, 62,64,66,68,70,72,74,76,78,80,82,84,86Ge, 66,68,70,72,74,76,78,80,82,84,86Se, 72,74,76,78,80,82,84,86,88,90,92,94,96Kr, 76,78,80,82,84,86,88,90,92,94,96,98,100,102Sr, 80,82,84,86,88,90,92,94,96,98,100,102,104,106,108Zr, 84,86,88,90,92,94,96,98,100,102,104,106,108,110Mo, 88,90,92,94,96,98,100,102,104,106,108,110,112,114,116,118Ru, 92,94,96,98,100,102,104,106,108,110,112,114,116,118,120,122,124,126,128Pd, 98,100,102,104,106,108,110,112,114,116,118,120,122,124,126,128,130Cd, 102,104,106,108,110,112,114,116,118,120,122,124,126,128,130,132,134Sn, 106,108,110,112,114,116,118,120,122,124,126,128,130,132,134,136,138Te, 110,112,114,116,118,120,122,124,126,128,130,132,134,136,138,140,142,144Xe, 118,120,122,124,126,128,130,132,134,136,138,140,142,144,146,148Ba, 122,124,126,128,130,132,134,136,138,140,142,144,146,148,150,152Ce, 128,130,132,134,136,138,140,142,144,146,148,150,152,154,156Nd, 130,132,134,136,138,140,142,144,146,148,150,152,154,156,158,160Sm, 138,140,142,144,146,148,150,152,154,156,158,160,162,164Gd, 140,142,144,146,148,150,152,154,156,158,160,162,164,166,168,170Dy, 144Er, 148,150,152,154,156,158,160,162,164,166,168,170,172,174Er, 152,154,156,158,160,162,164,166,168,170,172,174,176,178Yb, 160,162,164,166,168,170,172,174,176,178,180,182,184,186,188,190,192W, 162,164,166,168,170,172,174,176,178,180,182,184,186,188,190,192,194,196,198Os, 168,170,172,174,176,178,180,182,184,186,188,190,192,194,196,198,200,202,204Pt, 172,174,176,178,180,182,184,186,188,190,192,194,196,198,200,202,204,206,208,210Hg, 180,182,184,186,188,190,192,194,196,198,200,202,204,206,208,210,212,214Pb, 192,194,196,198,200,202,204,206,208,210,212,214,216,218Po, 198,200,202,204,206,208,210,212,214,216,218,220,222Rn, 206,208,210,212,214,216,218,220,222,224,226,228,230,232Ra, 214,216,218,220,222,224,226,228,230,232,234,236Th, 226,228,230,232,234,236,238,240,242U, 236,238,240,242,244,246Pu, 238,240,242,244,246,248,250Cm, 244,246,248,250,252Cf, 246,248Fm, 252,254,256Fm, 252,254No, 256Rf; compiled evaluated B(E2) values, T1/2, deformation parameters, first 2+ state energies in even-even nuclei.
NUCLEAR STRUCTURE 6He, 10,12Be, 10,12,14,16,18,20C, 16,18,20,22O, 18,20,22,24,26,28,30Ne, 20,22,24,26,28,30,32,34Mg, 24,26,28,30,32,34,36,38,40Si, 30,32,34,36,38,40,42,44S, 32,34,36,38,40,42,44,46Ar, 38,40,42Ca, 46,48,50Ca, 42,44,46,48,50,52,54,56Ti, 46,48,50,52,54,56,58,60,62Cr, 50,52,54,56,58,60,62,64,66Fe, 54,56,58,60,62,64,66,68,70,72,74,76Ni, 62,64,66,68,70,72,74,76,78Zn, 104,106Sn; calculated transition energies, B(E2). Nuclear shell model.
doi: 10.1016/j.adt.2015.10.001
Phys.Rev. C 96, 054318 (2017)
R.Kumar, M.Saxena, P.Doornenbal, A.Jhingan, A.Banerjee, R.K.Bhowmik, S.Dutt, R.Garg, C.Joshi, V.Mishra, P.J.Napiorkowski, S.Prajapati, P.-A.Soderstrom, N.Kumar, H.-J.Wollersheim
No evidence of reduced collectivity in Coulomb-excited Sn isotopes
NUCLEAR REACTIONS 112,116,118,120,122,124Sn(58Ni, 58Ni'), E=175 MeV; measured scattered projectiles and recoils from Coulomb excitation using annular gas-filled parallel-plate avalanche counter (PPAC), Eγ and Iγ, (particle)γ-coin using four Clover Ge detectors for γ detection at the IUAC-New Delhi tandem accelerator facility. 112,116,118,120,122,124Sn; deduced first 2+ levels, γ-ray yields, Coulomb excitation cross sections, and B(E2) for the first 2+ states using Winther and de Boer COULEX code. 114Sn; re-evaluated B(E2) for the first 2+ state. Comparison with recent experimental results for B(E2) from Coulomb excitation and DSAM techniques.
doi: 10.1103/PhysRevC.96.054318