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$^{165}$Ho和$^{169}$Tm在巨偶极共振区的光中子反应

Photoneutron reactions on $^{165}$Ho and $^{169}$Tm in the giant dipole resonance region

I. Gheorghe, S. Goriely, K. Stopani, S. Belyshev, M. Krzysiek, D. Filipescu, H. Wang, G. Fan, L. Liu, H. Scheit, D. Symochko, T. Aumann, T. Renstrøm, G. M. Tveten, F. Furmyr, A. Görgen, A. C. Larsen, S. Siem, V. Orlin, T. Ari-izumi, S. Miyamoto, H. Utsunomiya

arXiv 2609.25984首次发表:更新:

发表机构

National Institute for Physics and Nuclear Engineering, Horia Hulubei (IFIN-HH); Institut d’Astronomie et d’Astrophysique, Université Libre de Bruxelles; Lomonosov Moscow State University; Institute of Nuclear Physics Polish Academy of Sciences; Shanghai Advanced Research Institute, Chinese Academy of Sciences; Institut für Kernphysik, Technische Universität Darmstadt(霍里亚·胡利贝伊核物理与核工程国家研究所; 布鲁塞尔自由大学天体物理学与天文学研究所; 莫斯科罗蒙诺索夫国立大学; 波兰科学院核物理研究所; 中国科学院上海高等研究院; 达姆施塔特工业大学核物理研究所)

机构由 AI 辅助整理,请以论文原文为准。

AI 中文总结

本研究利用NewSUBARU的准单色γ射线束测量了$^{165}$Ho和$^{169}$Tm的光中子反应截面,提取了GDR参数、四极矩并检验了统计模型,发现20-25 MeV高能结构支持巨四极共振预测。

AI 中文摘要

利用日本NewSUBARU设施提供的准单色激光康普顿散射γ射线束,研究了从中子发射阈值附近到约40 MeV(远高于巨偶极共振(GDR)区)的形变核$^{165}$Ho和$^{169}$Tm的光中子反应。采用高且平坦效率的慢化$^3$He计数器阵列进行中子探测,并采用相关的中子多重性分类方法提取$(\gamma,\\,1nX)$、$(\gamma,\\,2nX)$、$(\gamma,\\,3nX)$和$(\gamma,\\,4nX)$反应截面及平均中子发射能量。将本工作的$^{165}$Ho截面与现有数据进行了比较,揭示了与Saclay多重性分类结果的差异,以及与Livermore结果相比总体10%的强度差异。$^{169}$Tm没有其他数据。通过拟合本工作的$\sigma(\gamma,\\,Sn)$数据,并针对实验未观测到的仅带电粒子反应的缺失贡献进行调整,提取了基于唯象Lorentzian模型的GDR参数。对于两个核,我们观察到20-25 MeV处的高能结构,与巨四极共振KMFR预测相符。基于本工作第一和第二GDR峰的质心能量,流体动力学模型预测$^{165}$Ho和$^{169}$Tm基态的内禀电四极矩分别为+7.00(34)~b和+7.38(28)~b。将本工作的实验激发函数和光中子能量与统计模型计算进行了比较。使用EMPIRE代码,我们对光子强度函数和核能级密度的唯象模型进行了敏感性测试。使用TALYS代码,利用微观核能级密度模型重现了本工作的实验$(\gamma,\\,inX)$截面和平均中子能量。

英文摘要

Photoneutron reactions were investigated for the deformed $^{165}$Ho and $^{169}$Tm nuclei from the vicinity of the neutron emission threshold up to $\sim$40~MeV, well above the giant dipole resonance (GDR) region, using quasimonochromatic laser Compton scattering $γ$-ray beams provided at the NewSUBARU facility, Japan. A high-and-flat efficiency moderated array of $^3$He counters was used for the neutron detection and an associated neutron multiplicity sorting method for extracting the $(γ,\,1nX)$, $(γ,\,2nX)$, $(γ,\,3nX)$ and $(γ,\,4nX)$ reaction cross sections and average neutron emission energies. The present $^{165}$Ho cross sections were compared to existing data, revealing discrepancies with the Saclay multiplicity sorting results and an overall 10$\%$ strength difference with the Livermore ones. There are no other data for $^{169}$Tm. GDR parameters based on phenomenological Lorentzian models were extracted by fitting the present $σ(γ,\,Sn)$ data with adjustments for the missing contribution of charged-particle-only reactions not observed experimentally. For both nuclei we observed high energy structures at 20-25~MeV, matching giant quadrupole resonance KMFR predictions. Based on the present centroid energies of the first and second GDR peaks, hydrodynamic model predictions gave intrinsic electric quadrupole moments of +7.00(34)~b and +7.38(28)~b for the ground states of $^{165}$Ho and $^{169}$Tm, respectively. The present experimental excitation functions and photoneutron energies were compared to statistical model calculations. Using the EMPIRE code, we performed a sensitivity test to phenomenological models of photon strength functions and nuclear level densities. The TALYS code was used to reproduce the present experimental $(γ,\,inX)$ cross sections and average neutron energies using microscopic nuclear level density models.

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