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Low-lying level structure of ~(56)Cu and its implications for the rp process

机译:低洼水平结构〜(56)CU及其对RP过程的影响

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The low-lying energy levels of proton-rich ~(56)Cu have been extracted using in-beam γ -ray spectroscopy with the state-of-the-art γ -ray tracking array GRETINA in conjunction with the S800 spectrograph at the National Superconducting Cyclotron Laboratory at Michigan State University. Excited states in ~(56)Cu serve as resonances in the ~(55)Ni(p,γ )~(56)Cu reaction, which is a part of the rp process in type-I x-ray bursts. To resolve existing ambiguities in the reaction Q value, a more localized isobaric multiplet mass equation (IMME) fit is used, resulting in Q = 639 ± 82 keV. We derive the first experimentally constrained thermonuclear reaction rate for ~(55)Ni(p,γ )~(56)Cu.We find that,with this newrate, the rp processmay bypass the ~(56)Niwaiting point via the ~(55)Ni(p,γ ) reaction for typical x-ray burst conditions with a branching of up to ~40%. We also identify additional nuclear physics uncertainties that need to be addressed before drawing final conclusions about the rp-process reaction flow in the ~(56)Ni region.
机译:使用束γ-射线光谱从最先进的γ-射线跟踪阵列Gretina与国家的S800光谱仪一起使用束γ-射线光谱来提取质子富型〜(56)Cu的低位能量水平。密歇根州立大学超导回旋加速器实验室。 〜(56)中的激发态用作〜(55)Ni(P,γ)〜(56)Cu反应中的共振,其是I型X射线突发中RP过程的一部分。为了解决反应Q值中的现有歧义,使用更局部化的等离子多功能量程(Imme)配合,导致Q = 639±82 keV。我们衍生出〜(55)Ni(P,γ)〜(56)Cu.We发现的第一种实验约束的热核反应速率。我们发现,通过〜(55次)绕过〜(56)Niwaiting点的RP处理。(55 )Ni(P,γ)反应对于典型的X射线突发条件,分支高达约40%。我们还确定需要解决的额外核物理不确定因素,需要在绘制关于〜(56)Ni区域的RP-过程反应流动的最终结论之前。

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  • 来源
    《Physical Review C》 |2017年第2017期|055806.1-055806.8|共8页
  • 作者单位

    National Superconducting Cyclotron Laboratory Michigan State University East Lansing Michigan 48824 USA Joint Institute for Nuclear Astrophysics Michigan State University East Lansing Michigan 48824 USA Department of Physics and Astronomy Michigan State University East Lansing Michigan 48824 USA;

    National Superconducting Cyclotron Laboratory Michigan State University East Lansing Michigan 48824 USA Joint Institute for Nuclear Astrophysics Michigan State University East Lansing Michigan 48824 USA;

    National Superconducting Cyclotron Laboratory Michigan State University East Lansing Michigan 48824 USA Joint Institute for Nuclear Astrophysics Michigan State University East Lansing Michigan 48824 USA;

    Department of Physics and Joint Institute for Nuclear Astrophysics University of Notre Dame Notre Dame Indiana 46556 USA;

    Physics Division Oak Ridge National Laboratory Oak Ridge Tennessee 37831 USA;

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