论文标题

搜索自然存在的osmium核素的α衰变,并伴有伽马量子

Search for alpha decay of naturally occurring osmium nuclides accompanied by gamma quanta

论文作者

Belli, P., Bernabei, R., Cappella, F., Caracciolo, V., Cerulli, R., Danevich, F. A., Incicchitti, A., Kasperovych, D. V., Kobychev, V. V., Kovtun, G. P., Kovtun, N. G., Laubenstein, M., Poda, D. V., Polischuk, O. G., Shcherban, A. P., Tessalina, S., Tretyak, V. I.

论文摘要

通过使用超低回光的宽阔的葡萄园$γ$γ$γ$ -DeTector,搜索自然发生的osmium同位素的$α$衰减,达到了最低的女儿核,搜索量为112 cm $^3 $^3 $,超纯净的oSmium样品的体积为118 g,在Gran Sasss sassso实验室(IFFN)(IFFN)(IFFN)(IFFN)(IFFN)(IFFN)(IFFN)(iffn forn)。使用负热电离质谱法测量了oSmium样品的同位素组成。在使用$γ$ -DETECTOR的数据获取15851小时后,未检测到效果,并且$α$衰减的下限设置为$ \ lim t_ {1/2} \ sim 10^{15} {15} -10^{19} $ yr。 $α$衰变的限制为$^{184} $ OS和$^{186} $ os的女儿Nuclei的第一个兴奋级别,$ t_ {1/2}(^{184} $ os $) $ t_ {1/2}(^{186} $ os $)\ geq3.3 \ geq3.3 \ times10^{17} $ yr(在90%c.l.),超过了衰减半衰期的当前理论估计。对于$^{189} $ OS和$^{192} $ OS也会腐烂到子核的基态,因为女儿核素的不稳定相对于$β$衰减。

A search for $α$ decay of naturally occurring osmium isotopes to the lowest excited levels of daughter nuclei has been performed by using an ultra-low-background Broad-Energy Germanium $γ$-detector with a volume of 112 cm$^3$ and an ultra-pure osmium sample with a mass of 118 g at the Gran Sasso National Laboratory of the INFN (Italy). The isotopic composition of the osmium sample has been measured with high precision using Negative Thermal Ionisation Mass Spectrometry. After 15851 h of data taking with the $γ$-detector no effect has been detected, and lower limits on the $α$ decays were set at level of $\lim T_{1/2}\sim 10^{15}-10^{19}$ yr. The limits for the $α$ decays of $^{184}$Os and $^{186}$Os to the first excited levels of daughter nuclei, $T_{1/2}(^{184}$Os$)\geq 6.8\times10^{15}$ yr and $T_{1/2}(^{186}$Os$)\geq3.3\times10^{17}$ yr (at 90% C.L.), exceed the present theoretical estimates of the decays half-lives. For $^{189}$Os and $^{192}$Os also decays to the ground states of the daughter nuclei were searched for due to the instability of the daughter nuclides relative to $β$ decay.

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