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arXiv 2405.08511nucl-ex
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利用JYFLTRAP双潘宁阱对富中子稀土同位素进行精密质谱测量以探究N=104中子壳层中部区域对r过程的贡献

Probing the N=104 midshell region for the r process via precision mass spectrometry of neutron-rich rare-earth isotopes with the JYFLTRAP double Penning trap

A. Jaries, S. Nikas, A. Kankainen, T. Eronen, O. Beliuskina, T. Dickel, M. Flayol, Z. Ge, M. Hukkanen, M. Mougeot, I. Pohjalainen, A. Raggio, M. Reponen, J. Ruo… 展开作者

A. Jaries, S. Nikas, A. Kankainen, T. Eronen, O. Beliuskina, T. Dickel, M. Flayol, Z. Ge, M. Hukkanen, M. Mougeot, I. Pohjalainen, A. Raggio, M. Reponen, J. Ruotsalainen, M. Stryjczyk, V. Virtanen

AI总结:

本文利用JYFLTRAP双潘宁阱对富中子稀土同位素进行高精度质量测量,首次测定多个核素质量并扩展N=104区域双中子分离能系统学,为r过程提供更精确的质量约束,显著改善A=170附近丰度计算。

摘要:

我们利用JYFLTRAP双潘宁阱中的相位成像离子回旋共振技术,对富中子稀土元素铽(Tb)、镝(Dy)和钬(Ho)同位素进行了高精度质量测量。我们报告了首次实验测定的169Tb、170Dy和171Dy的质量值,以及首次对169Dy和169-171Ho进行的高精度质量测量。对于170Ho,我们分辨了两个长寿命的基态和同核异能态并测量了它们的质量,得到同核异能激发能Eexc=150.8(54) keV。此外,我们还对之前潘宁阱获得的167,168Tb和167,168Dy的质量值进行了独立交叉检验。我们将双中子分离能的系统学扩展到了所有研究同位素链中N=104的中子壳层中部区域。我们更新和新增的质量测量结果为与天体物理快中子俘获(r)过程相关的中子俘获反应速率提供了更好的质量相关约束。利用新质量值计算的r过程丰度似乎在A=170处产生一个更陡的极小值,并且与使用原子质量评估2020值计算的丰度相差约15-30%。

英文摘要:

We have performed high-precision mass measurements of neutron-rich rare-earth Tb, Dy and Ho isotopes using the Phase-Imaging Ion-Cyclotron-Resonance technique at the JYFLTRAP double Penning trap. We report on the first experimentally determined mass values for $^{169}$Tb, $^{170}$Dy and $^{171}$Dy, as well as the first high-precision mass measurements of $^{169}$Dy and $^{169\text{-}171}$Ho. For $^{170}$Ho, the two long-lived ground and isomeric states were resolved and their mass measured, yielding an isomer excitation energy of $E_\text{exc}=150.8(54)$~keV. In addition, we have performed independent crosschecks of previous Penning-trap values obtained for $^{167\text{,} 168}$Tb and $^{167\text{,} 168}$Dy. We have extended the systematics of two-neutron separation energies to the neutron midshell at $N=104$ in all of the studied isotopic chains. Our updated and new mass measurements provide better mass-related constraints for the neutron-capture reaction rates relevant to the astrophysical rapid neutron capture (r) process. The r-process abundances calculated with the new mass values seem to produce a steeper minimum at A=170 and differ by around 15-30\% from the abundances computed with the Atomic Mass Evaluation 2020 values.

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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