References quoted in the XUNDL dataset: 140SB 9BE(238U,F):T1/2:XUNDL-3

3 references found.

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2017MO12

Phys.Rev. C 95, 044322 (2017)

B.Moon, C.-B.Moon, P.-A.Soderstrom, A.Odahara, R.Lozeva, B.Hong, F.Browne, H.S.Jung, P.Lee, C.S.Lee, A.Yagi, C.Yuan, S.Nishimura, P.Doornenbal, G.Lorusso, T.Sumikama, H.Watanabe, I.Kojouharov, T.Isobe, H.Baba, H.Sakurai, R.Daido, Y.Fang, H.Nishibata, Z.Patel, S.Rice, L.Sinclair, J.Wu, Z.Y.Xu, R.Yokoyama, T.Kubo, N.Inabe, H.Suzuki, N.Fukuda, D.Kameda, H.Takeda, D.S.Ahn, Y.Shimizu, D.Murai, F.L.Bello Garrote, J.M.Daugas, F.Didierjean, E.Ideguchi, T.Ishigaki, S.Morimoto, M.Niikura, I.Nishizuka, T.Komatsubara, Y.K.Kwon, K.Tshoo

Nuclear structure and β-decay schemes for Te nuclides beyond N=82

RADIOACTIVITY ¹⁴⁰Sb(β^-), (β^-n), (β^-2n)[From ⁹Be(²³⁸U, F), E=345 MeV/nucleon]; measured Eγ, Iγ, half-life of ¹⁴⁰Sb decay, βγ-, γγ-coin at RIBF-RIKEN facility. ^138,139,140Te; deduced levels, J, π, β feedings, delayed one- and two-neutron decay probabilities (P_n and P_2n), logft. Systematics of E(4+)/E(2+) values for nuclei with Z=50-70 with N=76-88. Discussed reduction of neutron-pairing energy.

doi: 10.1103/PhysRevC.95.044322

2020LI32

Nucl.Data Sheets 168, 1 (2020)

J.Liang, B.Singh, E.A.McCutchan, I.Dillmann, M.Birch, A.A.Sonzogni, X.Huang, M.Kang, J.Wang, G.Mukherjee, K.Banerjee, D.Abriola, A.Algora, A.A.Chen, T.D.Johnson, K.Miernik

Compilation and Evaluation of Beta-Delayed Neutron Emission Probabilities and Half-Lives for Z > 28 Precursors

RADIOACTIVITY ^{73,74,75,76,77,78,79,80,81,82,83}Cu, ^{78,79,80,81,82,83,84,85}Zn, ^{79,80,81,82,83,84,85,86,87}Ga, ^{83,84,85,86,87,88,89,90}Ge, ^{84,85,86,87,88,89,90,91,92}As, ^{86,87,88,89,90,91,92,93,94,95}Se, ^{87,88,89,90,91,92,93,94,95,96,97,98}Br, ^{91,92,93,94,95,96,97,98,99,100,101}Kr, ^{91,92,93,94,95,96,97,98,99,100,101,102,103,104}Rb, ^{96,97,98,99,100,101,102,103,104,105,106,107}Sr, ^{97,98,99,100,101,102,103,104,105,106,107,108,109}Y, ^{103,104,105,106,107,108,109,110,111,112,113}Zr, ^{103,104,105,106,107,108,109,110,111,112,113,114,115,116}Nb, ^{109,110,111,112,113,114,115,116,117,118,119}Mo, ^{109,110,111,112,113,114,115,116,117,118,119,120,121,122}Tc, ^{114,115,116,117,118,119,120,121,122,123,124,125}Ru, ^{115,116,117,118,119,120,121,122,123,124,125,126,127,128}Rh, ^{119,120,121,122,123,124,125,126,127,128,129,130,131}Pd, ^{120,121,122,123,124,125,126,127,128,129,130,131,132}Ag, ^{126,127,128,129,130,131,132,133,134}Cd, ^{127,128,129,130,131,132,133,134,135,136,137}In, ^{133,134,135,136,137,138,139,140}Sn, ^{134,135,136,137,138,139,140,141,142}Sb, ^{136,137,138,139,140,141,142,143,144,145}Te, ^{137,138,139,140,141,142,143,144,145,146,147}I, ^{141,142,143,144,145,146,147,148,149,150}Xe, ^{141,142,143,144,145,146,147,148,149,150,151,152}Cs, ^{147,148,149,150,151,152,153,154}Ba, ^{147,148,149,150,151,152,153,154,155,156,157}La, ^{153,154,155,156,157,158}Ce, ^{153,154,155,156,157,158,159,160,161}Pr, ^{158,159,160,161,162,163}Nd, ^{159,160,161,162,163,164,165}Pm, ^{163,164,165,166,167}Sm, ^{165,166,167,168,169}Eu, ^169,170,171Gd, ^{169,170,171,172,173,174}Tb, ^174,175,176Dy, ^{174,175,176,177,178}Ho, ¹⁸⁰Er, ^179,180,181Tm, ¹⁸⁵Yb, ^186,187,188Lu, ^{191,192,193,194}Ta, ^198,199Re, ²⁰³Os, ^203,204,205Ir, ^206,207,208Pt, ^{206,207,208,209,210}Au, ^{209,210,211,212,213,214,215,216}Hg, ^{210,211,212,213,214,215,216,217}Tl, ^{219,220,221,222,223,224}Bi, ^{225,226,227,228,229}At, ²²³Fr(β^-); analyzed available data; deduced β-delayed neutron emission probabilities (Pn) and T_1/2 for known or potential β-delayed neutron precursors. Comparison with systematics using three different approaches.

doi: 10.1016/j.nds.2020.09.001

2020WU04

Phys.Rev. C 101, 042801 (2020)

J.Wu, S.Nishimura, P.Moller, M.R.Mumpower, R.Lozeva, C.B.Moon, A.Odahara, H.Baba, F.Browne, R.Daido, P.Doornenbal, Y.F.Fang, M.Haroon, T.Isobe, H.S.Jung, G.Lorusso, B.Moon, Z.Patel, S.Rice, H.Sakurai, Y.Shimizu, L.Sinclair, P.-A.Soderstrom, T.Sumikama, H.Watanabe, Z.Y.Xu, A.Yagi, R.Yokoyama, D.S.Ahn, F.L.Bello Garrote, J.M.Daugas, F.Didierjean, N.Fukuda, N.Inabe, T.Ishigaki, D.Kameda, I.Kojouharov, T.Komatsubara, T.Kubo, N.Kurz, K.Y.Kwon, S.Morimoto, D.Murai, H.Nishibata, H.Schaffner, T.M.Sprouse, H.Suzuki, H.Takeda, M.Tanaka, K.Tshoo, Y.Wakabayashi

β-decay half-lives of 55 neutron-rich isotopes beyond the N = 82 shell gap

RADIOACTIVITY ^{134,135,136,137,138,139}Sn, ^{134,135,136,137,138,139,140,141,142}Sb, ^{137,138,139,140,141,142,143,144}Te, ^{140,141,142,143,144,145,146}I, ^{142,143,144,145,146,147,148}Xe, ^{145,146,147,148,149,150,151}Cs, ^{148,149,150,151,152,153}Ba, ^{151,152,153,154,155}La(β^-)[from ⁹Be(²³⁸U, F), E=345 MeV/nucleon, followed by separation of fragments using BigRIPS separator at RIBF-RIKEN]; measured β and γ radiations, half-lives by (implant)β and (implant)βγ correlations using the Wide range Active Silicon-Strip Stop per Array for Beta and ion (WAS3ABi) detection system and Euroball RIKEN Cluster Array (EURICA) of 84 Ge cluster detectors. Comparison with previously available experimental half-lives, and with theoretical calculations using FRDM+QRPA, KTUY+GT2, RHB+pn-RQRPA, and DF+CQRPA models. ¹⁴¹Te(β^-); calculated half-life and Gamow-Teller strengths using FRDM+QRPA(2019) model, and compared with experimental data. Discussed and calculated effects of new half-life data on r-process abundance.

doi: 10.1103/PhysRevC.101.042801