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Experimental Neutron Capture Rate Constraint Far from Stability

机译:实验性中子捕获率约束远非稳定

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摘要

Nuclear reactions where an exotic nucleus captures a neutron are critical for a wide variety of applications, from energy production and national security, to astrophysical processes, and nucleosynthesis. Neutron capture rates are well constrained near stable isotopes where experimental data are available; however, moving far from the valley of stability, uncertainties grow by orders of magnitude. This is due to the complete lack of experimental constraints, as the direct measurement of a neutron-capture reaction on a short-lived nucleus is extremely challenging. Here, we report on the first experimental extraction of a neutron capture reaction rate on Ni-69, a nucleus that is five neutrons away from the last stable isotope of Ni. The implications of this measurement on nucleosynthesis around mass 70 are discussed, and the impact of similar future measurements on the understanding of the origin of the heavy elements in the cosmos is presented.
机译:从能量生产和国家安全到天体物理过程和核合成等广泛的应用,至关重要的是外来原子核捕获中子的核反应。在有实验数据的情况下,中子的捕获率受到稳定同位素附近的良好约束。但是,远离稳定谷底,不确定性增加了数量级。这是由于完全缺乏实验约束,因为在短寿命原子核上直接测量中子俘获反应非常具有挑战性。在这里,我们报道了对Ni-69的中子俘获反应速率的第一个实验性提取,该原子核距Ni的最后一个稳定同位素5个中子。讨论了这种测量对质量70附近核合成的影响,并提出了类似的未来测量对了解宇宙中重元素起源的影响。

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  • 来源
    《Physical review letters》 |2016年第24期|242502.1-242502.6|共6页
  • 作者单位

    Michigan State Univ, Natl Supercond Cyclotron Lab, E Lansing, MI 48824 USA|Michigan State Univ, Dept Chem, E Lansing, MI 48824 USA;

    Michigan State Univ, Natl Supercond Cyclotron Lab, E Lansing, MI 48824 USA|Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA|Michigan State Univ, Joint Inst Nucl Astrophys, E Lansing, MI 48824 USA;

    Michigan State Univ, Natl Supercond Cyclotron Lab, E Lansing, MI 48824 USA;

    Michigan State Univ, Natl Supercond Cyclotron Lab, E Lansing, MI 48824 USA;

    Univ Oslo, Dept Phys, N-0316 Oslo, Norway;

    Univ Oslo, Dept Phys, N-0316 Oslo, Norway;

    Univ Notre Dame, Dept Phys, Notre Dame, IN 46556 USA|Los Alamos Natl Lab, Div Theoret, Los Alamos, NM 87544 USA;

    Univ Notre Dame, Dept Phys, Notre Dame, IN 46556 USA;

    Michigan State Univ, Natl Supercond Cyclotron Lab, E Lansing, MI 48824 USA|Michigan State Univ, Joint Inst Nucl Astrophys, E Lansing, MI 48824 USA|Cent Michigan Univ, Mt Pleasant, MI 48859 USA;

    Lawrence Livermore Natl Lab, 7000 East Ave, Livermore, CA 94550 USA;

    Los Alamos Natl Lab, POB 1663, Los Alamos, NM 87545 USA;

    Univ Oslo, Dept Phys, N-0316 Oslo, Norway;

    Michigan State Univ, Natl Supercond Cyclotron Lab, E Lansing, MI 48824 USA|Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA|Michigan State Univ, Joint Inst Nucl Astrophys, E Lansing, MI 48824 USA;

    Michigan State Univ, Natl Supercond Cyclotron Lab, E Lansing, MI 48824 USA|Michigan State Univ, Dept Chem, E Lansing, MI 48824 USA;

    Los Alamos Natl Lab, POB 1663, Los Alamos, NM 87545 USA;

    Michigan State Univ, Joint Inst Nucl Astrophys, E Lansing, MI 48824 USA|Cent Michigan Univ, Mt Pleasant, MI 48859 USA;

    Michigan State Univ, Natl Supercond Cyclotron Lab, E Lansing, MI 48824 USA|Michigan State Univ, Dept Chem, E Lansing, MI 48824 USA;

    Univ Oslo, Dept Phys, N-0316 Oslo, Norway;

    Univ Valencia, CSIC, IFIC, Valencia 46071, Spain;

    Univ Oslo, Dept Phys, N-0316 Oslo, Norway;

    Michigan State Univ, Natl Supercond Cyclotron Lab, E Lansing, MI 48824 USA|Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA|Michigan State Univ, Joint Inst Nucl Astrophys, E Lansing, MI 48824 USA;

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