首页> 外文学位 >Neutron spectroscopic factors of Nickel-56 via Nickel(p,d)-56 Nickel-55 reaction in inverse kinematics.
【24h】

Neutron spectroscopic factors of Nickel-56 via Nickel(p,d)-56 Nickel-55 reaction in inverse kinematics.

机译:通过逆运动学中的Nickel(p,d)-56 Nickel-55反应获得Nickel-56的中子光谱因子。

获取原文
获取原文并翻译 | 示例

摘要

Transfer reactions have been the classic tool for studying the angular distributions, the excitation energies, and the spectroscopic factors of possible single-particles states. With the advent of radioactive beams, there has been a renewed effort to utilize these beams in transfer reactions in inverse kinematics. The exact shell structure of the unstable doubly magic nucleus 56Ni has attracted a lot of interest recently. To test if 56Ni has a closed f7/2 orbital, we have carried out the 56Ni(p,d)55Ni transfer reaction measurement with the radioactive 56Ni beam in inverse kinematics for the first time at the NSCL using the HiRA array and S800 spectrograph. The spectroscopic factor predicted by the independent particle model is 8, shell-model calculations give value of 6.8. We have extracted spectroscopic factors of the 56Ni(p,d)55Ni reaction, for the ground and two excited states of 55Ni. The neutron SF value of 7 for the 56Ni(p,d)55Ni ground state agrees with shell-model calculations supports the view that 56Ni is a closed shell nucleus. This result supports the use of 56Ni as a core in shell-model calculations. Another important goal was to study the structure of 55Ni by determining the spin and parities of excited states. We have assigned an ℓ value of 1 to first excited state of 55Ni for 2.089 MeV state of 55Ni. We have extracted a spectroscopic factor of 0.14 for this state. This serves as a second test of the shell model, and the results agree with the shell model calculations. We have confirmed the tentative ℓ = 0 assumption for 3.185 MeV state. A neutron spectroscopic factor of 1.2 was obtained for this state.
机译:转移反应一直是研究角分布,激发能和可能的单粒子状态的光谱因子的经典工具。随着放射性束的出现,人们进行了新的努力以在逆运动学中的转移反应中利用这些束。不稳定的双魔核56Ni的精确壳结构最近引起了很多兴趣。为了测试56Ni是否具有闭合的f7 / 2轨道,我们首次使用HiRA阵列和S800光谱仪在NSCL上进行了逆运动学中的56Ni(p,d)55Ni放射性反应逆运动学测量。独立粒子模型预测的光谱因子为8,壳模型计算得出的值为6.8。我们提取了55Ni的基态和两个激发态的56Ni(p,d)55Ni反应的光谱因子。对于56Ni(p,d)55Ni基态的中子SF值为7,与壳模型计算相符,这支持了56Ni是闭合壳核的观点。该结果支持在壳模型计算中使用56Ni作为核。另一个重要目标是通过确定激发态的自旋和奇偶性来研究55Ni的结构。我们已经分配了ℓ值1到55Ni的2.089 MeV态的第一激发态55Ni。我们为此状态提取了一个光谱因子0.14。这是对壳模型的第二次测试,其结果与壳模型的计算结果一致。我们已经确认了暂定的ℓ = 3.185 MeV状态的假设为0。在此状态下获得的中子光谱系数为1.2。

著录项

  • 作者

    Sanetullaev, Alisher.;

  • 作者单位

    Michigan State University.;

  • 授予单位 Michigan State University.;
  • 学科 Nuclear physics and radiation.
  • 学位 Ph.D.
  • 年度 2012
  • 页码 186 p.
  • 总页数 186
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号