Decay ofSn126and of the 19-min and 12.4-day Isomers ofSb126

Abstract
The γ radiations of 105yr Sn126 and of the Sb126 isomers have been studied with NaI(Tl) scintillation spectrometers and Ge(Li) detectors. β-ray spectra were measured with a trans-stilbene scintillation unit, and conversion electrons were examined with Si(Li) detectors. The decay of Sn126 involves a 0.25 ± 0.03-MeV β transition followed by 21.6-, 23.4-, 42.7-, 64.4-, and 87.7-keV γ transitions in Sb126. The 23.4- and 87.7-keV transitions are in prompt coincidence with the β rays; the 64.4-keV and either the 21.6- or 42.7-keV transitions deexcite an intermediate delayed level with t12=0.5±0.1 μsec. Both the 19-min and the 12.4- day isomers of Sb126 have essentially the same 1.90 ± 0.15-MeV maximum β-ray endpoint energy; however, the β spectrum of the latter is more complex (intense inner groups). The 19-min isomer decays by β emission (86%) to excited levels in Te126 and by ≤31-keV isomeric transition (14%) to the 12.4-day ground state. The Te126 excited levels involved in the decay of both Sb126 isomers are at 665(2+), 1359(4+), 1774(6+), 2215, 2395, 2494, 2514, 2702, 2761, 2834, 3086, 3187, and 3413 keV. Spin and parity assignments of 5+ and 8 are proposed for the 19-min and 12.4-day isomers, respectively. The total β-disintegration energy of the Sb126 ground state is 3.67 ± 0.15 MeV.

This publication has 19 references indexed in Scilit: