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arXiv 2001.00976nucl-exnucl-th
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铅下及$\boldsymbol{N=126}$外中子壳层结构初探

First Exploration of Neutron Shell Structure Below Lead and Beyond $\boldsymbol{N=126}$

T. L. Tang, B. P. Kay, C. R. Hoffman, J. P. Schiffer, D. K. Sharp, L. P. Gaffney, S. J. Freeman, M. R. Mumpower, A. Arokiaraj, E. F. Baader, P. A. Butler, W. N.… 展开作者

T. L. Tang, B. P. Kay, C. R. Hoffman, J. P. Schiffer, D. K. Sharp, L. P. Gaffney, S. J. Freeman, M. R. Mumpower, A. Arokiaraj, E. F. Baader, P. A. Butler, W. N. Catford, G. de Angelis, F. Flavigny, M. D. Gott, E. T. Gregor, J. Konki, M. Labiche, I. H. Lazurus, P. T. MacGregor, I. Martel, R. D. Page, Zs. Podolyák, O. Poleshchuk, R. Raabe, F. Recchia, J. F. Smith, S. V. Szwec, J. Yang

摘要:

低于铅但超过126个中子的原子核对于理解产生比$r$重的原子核的天体物理过程至关重要。尽管它们的重要性,这些原子核的结构和性质仍然未经实验测试,因为它们很难在稳定束的核反应中产生。在这个区域的壳结构的第一次探索,中子激发$^{207}$汞已探测使用中子添加($d$,$p$)反应在逆运动学。$^{206}$ Hg的放射性核束以高于库仑势垒的能量输送到新的ISOLDE螺线管光谱仪。光谱学的$^{207}$汞标志着第一步,提高我们的理解相关的结构性质的原子核参与的路径的关键部分的$r$ -过程。

英文摘要:

The nuclei below lead but with more than 126 neutrons are crucial to an understanding of the astrophysical $r$-process in producing nuclei heavier than $A\sim190$. Despite their importance, the structure and properties of these nuclei remain experimentally untested as they are difficult to produce in nuclear reactions with stable beams. In a first exploration of the shell structure of this region, neutron excitations in $^{207}$Hg have been probed using the neutron-adding ($d$,$p$) reaction in inverse kinematics. The radioactive beam of $^{206}$Hg was delivered to the new ISOLDE Solenoidal Spectrometer at an energy above the Coulomb barrier. The spectroscopy of $^{207}$Hg marks a first step in improving our understanding of the relevant structural properties of nuclei involved in a key part of the path of the $r$-process.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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