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$^{235}$U(n$_{\mathrm{th}}$,f) 同位素裂变产额在 ILL 的 FIPPS 谱仪上利用瞬发和延迟伽马射线的研究结果

Results on $^{235}$U(n$_{\mathrm{th}}$,f) isotopic fission yields using prompt and delayed gamma rays at the FIPPS spectrometer of the ILL

T. Materna, P. Herran, M. Ballu, Q. Poirier, A. Letourneau, D. Doré, L. Thulliez, C. Michelagnoli, F. Kandzia, Y. H. Kim, U. Köster, O. Litaize, O. Sérot, A. Chebboubi

arXiv 2609.13033首次发表:更新:

发表机构

IRFU, CEA, Université Paris-Saclay; Institut Laue-Langevin; CEA, DES, IRESNE, DER, Cadarache(法国原子能及替代能源委员会萨克雷大学核物理研究所; 朗之万研究所; 法国原子能及替代能源委员会卡达拉舍设施)

机构由 AI 辅助整理,请以论文原文为准。

AI 中文总结

利用ILL的FIPPS谱仪和有源靶,通过瞬发和延迟伽马射线测量235U(n_th,f)的同位素裂变产额,发现132Sn产额较JEFF-3.3低约7倍,归因于其基态产生;90Kr衰变存在约40%过剩,可能源于90Rb基态馈送高估。

AI 中文摘要

我们展示了在 ILL 使用 FIPPS $\gamma$ 射线谱仪,以溶解在液体闪烁体中的 $^{235}$U 制成的有源靶进行的测量活动的初步结果。利用瞬发 $\gamma$ 射线提取了绝对、独立的同位素裂变产额。我们获得了 $^{235}$U(n$_{\mathrm{th}}$,f) 反应中一组选定的产额较好的偶偶核的产额,并将其与 JEFF-3.3 评估数据进行了比较。其中包括双幻核 $^{132}$Sn,我们观察到其相对于 JEFF-3.3 存在显著亏损(约因子 7)。利用 FIFRELIN 裂变碎片退激代码,我们将这一差异解释为 $^{132}$Sn 主要在断裂时或中子蒸发后以其基态产生的证据。同一实验中记录的延迟 $\gamma$ 射线也进行了分析。与核数据库相比,$^{132}$Sn 的 $\beta$ 衰变未发现偏差。然而,在 $^{90}$Kr 的 $\beta$ 衰变中发现了约 40% 的过剩,这可能源于评估数据中 $^{90}$Rb 的基态馈送被高估。

英文摘要

We present preliminary results from a measurement campaign conducted with the FIPPS $γ$-ray spectrometer at the ILL using an active target made of $^{235}$U dissolved in a liquid scintillator. Prompt $γ$ rays were used to extract absolute, independent isotopic fission yields. We obtained yields for a selected set of well-produced even-even nuclei from the $^{235}$U(n$_{\mathrm{th}}$,f) reaction and compared them with JEFF-3.3 evaluated data. This included the doubly magic nucleus $^{132}$Sn, for which we observed a pronounced deficit (about a factor 7) with respect to JEFF-3.3. Using the FIFRELIN fission fragment de-excitation code, we interpreted this discrepancy as evidence that $^{132}$Sn is mainly produced in its ground state at scission or after neutron evaporation. Delayed $γ$ rays recorded in the same experiment were also analysed. No deviation was found in the beta decay of $^{132}$Sn compared to the nuclear database. However, an excess of about a 40% was found in the $β$ decay of $^{90}$Kr, which may originate from an overestimated ground-state feeding of $^{90}$Rb in the evaluated data.

论文原文

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