{"title":"Study of the isomeric yield ratio in the photoneutron reaction of natural holmium induced by laser-accelerated electron beams","authors":"Jingli Zhang, Wei Qi, Wenru Fan, Zongwei Cao, Kaijun Luo, Changxiang Tan, Xiaohui Zhang, Zhigang Deng, Zhimeng Zhang, Xinxiang Li, Yun Yuan, Wen Luo, Weimin Zhou","doi":"10.3389/fspas.2023.1265919","DOIUrl":null,"url":null,"abstract":"Introduction: An accurate knowledge of the isomeric yield ratio (IR) induced by the photonuclear reaction is crucial to study the nuclear structure and reaction mechanisms. 165 Ho is a good candidate for the investigation of the IR since the Ho target has a natural abundance of 100% and the residual nuclide has a good decay property. Methods: In this study, the photoneutron production of 164m, g Ho induced by laser-accelerated electron beams is investigated experimentally. The γ-ray spectra of activated Ho foils are off-line detected. Since the direct transitions from the 164m Ho are not successfully observed, we propose to extract the IRs of the 164m, g Ho using only the photopeak counts from the ground-state decay. Results: The production yields of 164m, g Ho are extracted to be (0.45 ± 0.10) × 10 6 and (1.48 ± 0.14) × 10 6 per laser shot, respectively. The resulting IR is obtained to be 0.30 ± 0.08 at the effective γ-ray energy of 12.65 MeV. Discussion: The present data, available experimental data, and TALYS calculations are then compared to examine the role of the excitation energy. It is found that besides the giant dipole resonance, the excitation energy effect also plays a key role in the determination of the IRs.","PeriodicalId":46793,"journal":{"name":"Frontiers in Astronomy and Space Sciences","volume":null,"pages":null},"PeriodicalIF":2.6000,"publicationDate":"2023-11-08","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Frontiers in Astronomy and Space Sciences","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.3389/fspas.2023.1265919","RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
Introduction: An accurate knowledge of the isomeric yield ratio (IR) induced by the photonuclear reaction is crucial to study the nuclear structure and reaction mechanisms. 165 Ho is a good candidate for the investigation of the IR since the Ho target has a natural abundance of 100% and the residual nuclide has a good decay property. Methods: In this study, the photoneutron production of 164m, g Ho induced by laser-accelerated electron beams is investigated experimentally. The γ-ray spectra of activated Ho foils are off-line detected. Since the direct transitions from the 164m Ho are not successfully observed, we propose to extract the IRs of the 164m, g Ho using only the photopeak counts from the ground-state decay. Results: The production yields of 164m, g Ho are extracted to be (0.45 ± 0.10) × 10 6 and (1.48 ± 0.14) × 10 6 per laser shot, respectively. The resulting IR is obtained to be 0.30 ± 0.08 at the effective γ-ray energy of 12.65 MeV. Discussion: The present data, available experimental data, and TALYS calculations are then compared to examine the role of the excitation energy. It is found that besides the giant dipole resonance, the excitation energy effect also plays a key role in the determination of the IRs.
准确地了解光核反应引起的异构体产率(IR)对于研究核结构和反应机理至关重要。由于Ho靶的自然丰度为100%,并且其残余核素具有良好的衰变特性,因此Ho是红外研究的一个很好的候选者。方法:实验研究了激光加速电子束诱导164m, g Ho的光子中子产生。离线检测了活化Ho箔的γ射线能谱。由于164m Ho的直接跃迁没有被成功地观测到,我们建议仅使用基态衰变的光峰计数来提取164m, g Ho的IRs。结果:提取164m, g Ho的产率分别为(0.45±0.10)× 10.6和(1.48±0.14)× 10.6 /次激光。所得IR为0.30±0.08,有效γ射线能量为12.65 MeV。讨论:然后将现有数据、可用实验数据和TALYS计算结果进行比较,以检验激发能的作用。研究发现,除了巨偶极子共振外,激发能效应对红外光谱的测定也起着关键作用。