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
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.