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Nuclear structure studies on halo nuclei by direct reactions with radioactive beams

机译:与放射性束直接反应对晕核的核结构研究

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摘要

The investigation of direct reactions with exotic beams in inverse kinematics gives access to a wide field of nuclear structure studies in the region far off stability. The basic concept and the methods involved are briefly discussed. The present contribution will focus on the investigation of light neutron-rich halo nuclei. Such nuclei reveal a new type of nuclear structure, namely an extended neutron distribution surrounding a nuclear core. An overview on this phenomenon, and on the various methods which gave first evidence and qualitative confirmation of our present picture of halo nuclei, is given. To obtain more quantitative information on the radial shape of halo nuclei, elastic proton scattering on neutron-rich light nuclei at intermediate energies was recently investigated for the first time. This method is demonstrated to be an effective means for studying the nuclear matter distributions of such nuclei. The results on the nuclear matter radii of 6He and 8He, the deduced nuclear matter density distributions, and the significance of the data on the halo structure is discussed. The present data allow also a sensitive test of theoretical model calculations on the structure of neutron-rich helium isotopes. A few examples are presented. The investigation of few-nucleon transfer reactions in inverse kinematics may provide new and complementary information on nuclear structure, as well as astrophysical questions. The physics motivation and the experimental concept for such experiments, to be performed due to momentum matching reasons at low incident energies around 5 - 20
机译:对逆运动学中奇异束直接反应的研究为进入远离稳定区域的核结构研究提供了广阔的空间。简要讨论了基本概念和涉及的方法。目前的贡献将集中于研究轻中子富集的晕核。这样的核揭示了一种新型的核结构,即围绕核芯的扩展中子分布。本文概述了这种现象,并提供了各种方法,这些方法为我们目前的晕核研究提供了初步的证据和定性的证明。为了获得有关晕原子核的径向形状的更多定量信息,最近首次研究了在中等能量下富于中子的光核上的弹性质子散射。实践证明,该方法是研究此类核的核物质分布的有效手段。讨论了6He和8He核物质半径的结果,推导的核物质密度分布以及有关晕结构的数据的意义。目前的数据还允许对富含中子的氦同位素的结构进行理论模型计算的敏感测试。给出了一些例子。在逆运动学中对少数核子转移反应的研究可能会提供有关核结构以及天体物理问题的新的补充信息。由于动量匹配的原因,在5-20左右的低入射能量下,将进行此类实验的物理动力和实验概念

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