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alpha-Capture and alpha-elastic scattering on P-nuclei to probe the Hauser-Feshbach framework.

机译:在P核上进行alpha捕获和alpha弹性散射以探测Hauser-Feshbach框架。

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摘要

The thirty five neutron deficient stable nuclei known as the p-nuclei are synthesized in a series of photodisintegration reactions of the (gamma,n), (gamma,p) and (gamma,alpha) type in a hot gamma-flux environment.;Abundance calculations involve an extended network of about 20,000 nuclear reactions of almost 2000 nuclei. The bulk of these rates are calculated theoretically with the statistical Hauser Feshbach Model (HF Model). Of particular importance in the p-process modeling are the (gamma,alpha) branchings.;Even though in the astrophysical environment it is photodisintegration reactions that synthesize the p-nuclei, in the laboratory it is the inverse process that is generally measured. By detailed balance, it is possible to arrive at the relevant reactions. The experimental data for alpha-capture reactions is scarce since at the p-process temperatures (2-3 GK), the alpha-particle energies are typically of a few MeV and the corresponding cross sections very small. In addition, the results show a significant deviation compared to the model predictions.;The HF cross sections are governed by transmission coefficients. These are extracted from an appropriate optical model potential (OMP). The alpha-nucleus potential in particular is poorly known at low energies mainly due to the lack of relevant data. The observed inconsistencies between the predicted and measured (alpha,gamma) rates may be due to problems with this alpha-potential parameter.;To explore the applicability of the Hauser Feshbach model, to extend the experimental database of alpha-capture reactions on p-nuclei, to test the global parameterizations that currently exist, and to constrain the alpha-nucleus potential, the alpha-capture cross section of 106Cd(alpha,gamma)110Sn and the local alpha-nucleus potentials of 106Cd, 118Sn, and 120,124,126,128,130 Te have been measured and extracted. The experiments have been carried out at the University of Notre Dame. The results are presented here.
机译:在热的γ-通量环境中,在(γ,n),(γ,p)和(γ,α)型的一系列光分解反应中合成了称为p核的35个中子不足的稳定核。丰度计算涉及约2000个核的约20,000个核反应的扩展网络。理论上,这些速率的大部分是使用统计Hauser Feshbach模型(HF模型)来计算的。在p-过程建模中尤为重要的是(γ,α)支链;即使在天体物理环境中,光致分解反应合成了p-核,但在实验室中通常测量的是逆过程。通过详细的平衡,可以得出相关的反应。由于在p加工温度(2-3 GK)下,α粒子的能量通常只有几个MeV,并且相应的横截面非常小,因此关于α捕获反应的实验数据很少。此外,与模型预测相比,结果显示出明显的偏差。HF横截面由透射系数控制。这些是从适当的光学模型电势(OMP)中提取的。主要由于缺乏相关数据,尤其是在低能量时对α核势的了解很少。观察到的预测和测得的(α,γ)速率之间的不一致可能是由于该α势参数存在问题。为了探索Hauser Feshbach模型的适用性,扩展在p-上的α捕获反应的实验数据库核,以测试当前存在的全局参数化,并约束α-核势,106Cd(α,γ)110Sn的α捕获截面和106Cd,118Sn和120,124,126,128,130 Te的局部α-核势具有被测量和提取。实验是在圣母大学进行的。结果显示在这里。

著录项

  • 作者

    Palumbo, Annalia.;

  • 作者单位

    University of Notre Dame.;

  • 授予单位 University of Notre Dame.;
  • 学科 Physics Astrophysics.;Physics Nuclear.
  • 学位 Ph.D.
  • 年度 2009
  • 页码 232 p.
  • 总页数 232
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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