论文标题

美元

$^{54}$Fe($d$,$p$)$^{55}$Fe and the evolution of single neutron energies in the $N=29$ isotones

论文作者

Riley, L. A., Hay, I. C. S., Baby, L. T., Conley, A. L., Cottle, P. D., Esparza, J., Hanselman, K., Kelly, B., Kemper, K. W., Macon, K. T., McCann, G. W., Quirin, M. W., Renom, R., Saunders, R. L., Spieker, M., Wiedenhöver, I.

论文摘要

$^{54} $ fe($ d $,$ p $)$^{55} $ fe反应在16 meV进行,使用佛罗里达州立大学超级派式谱图确定单中性能量,以确定$ 2P_ {3/2} $,$ 2P_ {1/2} $ 1/2} $ 1/1/1/1/1/1/1/1/1/5/ $ 1G_ {9/2} $和$ 2D_ {5/2} $ ORBITS。观察到两个状态在以前的(d,p)测量中没有观察到。此外,我们进行了角动量转移,\ textit {l},分配到四个状态,并更改了\ textIt {l}分配的分配($ d $,$ p $)的测量值九个状态。 $ 2P_ {3/2} $和$ 2P_ {1/2} $ ORBITS之间的自旋轨道分裂与其他$ n = 29 $ isotones中的旋转轨道分裂相似,而不接近零,如先前的测量所建议。 $ 1f_ {5/2} $单中性能量在$^{55} $中明显低于$^{51} $ ti中的$^{55} $ fe,这是由协变量密度函数理论计算所预测的,这是$^{55} $比1 mev更高的计算,尽管它比400 00更高,但仅超过1 Mev的计算。 $ 2P_ {1/2} $ ORBIT。我们观察到的$ 1G_ {9/2} $ ORBIT到9.3 MEV的单中性分离能量的求和光谱强度仅为0.3。这是令人惊讶的,因为$ 1G_ {9/2} $ orbit由Togashi \ textit {等}预测,仅位于$ 2P_ {3/2} $ orbit的$ 2P_ {3/2} $上方仅位于5.5 meV。

A measurement of the $^{54}$Fe($d$,$p$)$^{55}$Fe reaction at 16 MeV was performed using the Florida State University Super-Enge Split-Pole Spectrograph to determine single-neutron energies for the $2p_{3/2}$, $2p_{1/2}$, $1f_{5/2}$, $1g_{9/2}$ and $2d_{5/2}$ orbits. Two states were observed that had not been observed in previous (d, p) measurements. In addition, we made angular momentum transfer, \textit{L}, assignments to four states and changed \textit{L} assignments from previous ($d$, $p$) measurements for nine more states. The spin-orbit splitting between the $2p_{3/2}$ and $2p_{1/2}$ orbits is similar to that in the other $N=29$ isotones and not close to zero as a previous measurement suggested. While the $1f_{5/2}$ single neutron energy is significantly lower in $^{55}$Fe than in $^{51}$Ti, as predicted by a covariant density functional theory calculation, the single-neutron energy for this orbit in $^{55}$Fe is more than 1 MeV higher than the calculation suggests, although it is only 400 keV above the $2p_{1/2}$ orbit. The summed spectroscopic strength we observed for the $1g_{9/2}$ orbit up to the single-neutron separation energy of 9.3 MeV is only 0.3. This is surprising because the $1g_{9/2}$ orbit is predicted by Togashi \textit{et al.} to be located only 5.5 MeV above the $2p_{3/2}$ orbit.

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