论文标题

$^{249,251} $ MD的梁内伽马射线和电子光谱

In-beam gamma-ray and electron spectroscopy of $^{249,251}$Md

论文作者

Briselet, R., Theisen, Ch., Sulignano, B., Airiau, M., Auranen, K., Cox, D. M., Déchery, F., Drouart, A., Favier, Z., Gall, B., Goigoux, T., Grahn, T., Greenlees, P. T., Hauschild, K., Herzan, A., Herzberg, R. -D., Jakobsson, U., Julin, R., Juutinen, S., Konki, J., Leino, M., Lopez-Martens, A., Mistry, A., Nieminen, P., Pakarinen, J., Papadakis, P., Peura, P., Rahkila, P., Rey-Herme, E., Rubert, J., Ruotsalainen, P., Sandzelius, M., Sarén, J., Scholey, C., Sorri, J., Stolze, S., Uusitalo, J., Vandebrouck, M., Ward, A., Zielińska, M., Bally, B., Bender, M., Ryssens, W.

论文摘要

使用$γ$ -Ray和转换电子光谱学研究了奇数 - $ z $ $^{251} $ md核。除了基于$ [521] 1/2^ - $配置的先前观察到的旋转频段外,还使用$γ$ - $γ$ cocidences确定了另一种旋转结构。电子光谱的使用允许在较大的旋转频率范围内观察旋转带。使用依赖于陀螺因子的过渡强度,已经推断出了$ [514] 7/2^ - $单颗粒构型,即该频段,即地面范围。通过模拟一组未解决的激发频带,可以很好地再现以$ \ simeq $ 60%的强度为$ \ simeq $ 60%的物理背景。此外,对角动量的强度曲线的详细分析提供了一种推导轨道旋转磁因子的方法,即$ g_k = 0.69^{+0.19} _ { - 0.16} $,用于基地状态频段。使用$γ$ -Ray -Ray射击光谱研究了奇数 - $ z $ $^{249} $ MD。在$^{249,251} $ MD中都发现了$Δl=Δj= 3 $ [521] 3/2^ - $和$ [633] 7/2^+$ [633] 7/2^+$ [633] $ [633] $ [633] $ [633] $ [633] $ [633] $ [633] $ [633] $ [633] $ [249,251} $ MD的证据。已经讨论了$^{251} $ MD地面带过渡能量与$^{255} $ lr的兴奋带的相似性。进行了Skyrme-Hartree-fock-Bogoliubov计算,以研究这些频段之间相似性的起源。

The odd-$Z$ $^{251}$Md nucleus was studied using combined $γ$-ray and conversion-electron in-beam spectroscopy. Besides the previously observed rotational band based on the $[521]1/2^-$ configuration, another rotational structure has been identified using $γ$-$γ$ coincidences. The use of electron spectroscopy allowed the rotational bands to be observed over a larger rotational frequency range. Using the transition intensities that depend on the gyromagnetic factor, a $[514]7/2^-$ single-particle configuration has been inferred for this band, i.e., the ground-state band. A physical background that dominates the electron spectrum with an intensity of $\simeq$ 60% was well reproduced by simulating a set of unresolved excited bands. Moreover, a detailed analysis of the intensity profile as a function of the angular momentum provided a method for deriving the orbital gyromagnetic factor, namely $g_K = 0.69^{+0.19}_{-0.16}$ for the ground-state band. The odd-$Z$ $^{249}$Md was studied using $γ$-ray in-beam spectroscopy. Evidence for octupole correlations resulting from the mixing of the $Δl = Δj = 3$ $[521]3/2^-$ and $[633]7/2^+$ Nilsson orbitals were found in both $^{249,251}$Md. A surprising similarity of the $^{251}$Md ground-state band transition energies with those of the excited band of $^{255}$Lr has been discussed in terms of identical bands. Skyrme-Hartree-Fock-Bogoliubov calculations were performed to investigate the origin of the similarities between these bands.

扫码加入交流群

加入微信交流群

微信交流群二维码

扫码加入学术交流群,获取更多资源