References quoted in the XUNDL dataset: 140I 140I B-:%B-N:XUNDL-3

4 references found.

Clicking on a keynumber will list datasets that reference the given article.

Return to 140I B-:%B-N:XUNDL-3

1977SH01

Nucl.Phys. A275, 76 (1977)

S.Shalev, G.Rudstam

Energy Spectra of Delayed Neutrons from Separated Fission Products (III). The Precursors ⁸⁸Br, ⁹⁰Br, ¹³⁸I, ¹⁴⁰I, ¹⁴²(Xe+Cs) and ¹⁴⁴Cs

RADIOACTIVITY ^88,90Br, ^138,140I, ^142,144Cs, ¹⁴²Xe; measured delayed neutrons; deduced average level spacing, neutron envelopes, neutron emission probability, possible Qβ discrepancies. ⁸⁸Br deduced J, π.

doi: 10.1016/0375-9474(77)90276-7

2002PF04

Prog.Nucl.Energy 41, 39 (2002)

B.Pfeiffer, K.Kratz, P.Moller

Status of delayed-Neutron Precursor Data: Half-Lives and Neutron Emission Probabilities

COMPILATION Z=27-63; compiled, analyzed β-decay T_1/2, neutron emission probabilities, model predictions.

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

2020WA04

Phys.Rev. C 101, 025806 (2020)

B.S.Wang, S.A.Caldwell, N.D.Scielzo, A.Czeszumska, J.A.Clark, G.Savard, A.Aprahamian, M.T.Burkey, C.J.Chiara, J.Harker, A.F.Levand, S.T.Marley, G.E.Morgan, J.M.Munson, E.B.Norman, A.Nystrom, R.Orford, S.W.Padgett, A.Perez Galvan, K.S.Sharma, K.Siegl, S.Y.Strauss

β-delayed-neutron studies of ^135,136Sb and ¹⁴⁰I performed with trapped ions

RADIOACTIVITY ^135,136Sb, ¹⁴⁰I(β^-), (β^-n) [from ²⁵²Cf(SF) CARIBU facility and mass scans of radioactive beams with the Canadian Penning Trap (CPT) mass spectrometer at Argonne National Laboratory]; measured recoil ions, Eβ, Eγ, (recoil ions)β- and βγ-coin using Beta-decay Paul Trap with two plastic-scintillator ΔE-E telescopes, two MCP detectors, and two HPGe detectors; deduced beta-delayed neutron spectra, beta-delayed neutron-emission probabilities (%β^-n or P_n). Comparison with earlier experimental results.

doi: 10.1103/PhysRevC.101.025806