Equipment for Theoretical and Experimental Nuclear Physics

核物理理论与实验设备

• 批准号: ST/N002636/1
• 负责人: Carlo Barbieri
• 金额: $ 4.24万
• 依托单位: University of Surrey
• 依托单位国家: 英国
• 项目类别: Research Grant
• 财政年份: 2015
• 资助国家: 英国
• 起止时间: 2015 至 无数据
• 项目状态: 已结题
• 来源: https://gtr.ukri.org/projects?ref=ST%2FN002636%2F1
• 关键词: Equipment; Theoretical; Experimental; Nuclear; Physics

Nuclear physics research is undergoing a transformation. For a hundred years, atomic nuclei have been probed by collisions between stable beams and stable targets, with just a small number of radioactive isotopes being available. Now, building on steady progress over the past 20 years, it is at last becoming possible to generate intense beams of a wide range of short-lived isotopes, so-called "radioactive beams". This enables us vastly to expand the scope of experimental nuclear research. For example, it is now realistic to plan to study in the laboratory a range of nuclear reactions that take place in exploding stars. Thereby, we will be able to understand how the chemical elements that we find on Earth were formed and distributed through the Universe. At the core of our experimental research is our strong participation at leading international radioactive-beam facilities. While we are now contributing, or planning to contribute, to substantial technical developments at these facilities, the present grant request is focused on the exploitation of the capabilities that are now becoming available. Experimental progress is intimately linked with theory, where novel and practical approaches are a hallmark of the Surrey group. An outstanding feature, which is key to our group's research plans and is unique in the UK, is our powerful blend of theoretical and experimental capability. Our science goals are aligned with current STFC strategy for nuclear physics, as expressed in detail through the Nuclear Physics Advisory Panel. We wish to understand the boundaries of nuclear existence, i.e. the limiting conditions that enable neutrons and protons to bind together to form nuclei. Under such conditions, the nuclear system is in a delicate state and shows unusual phenomena. It is very sensitive to the properties of the nuclear force. For example, weakly bound neutrons can orbit their parent nucleus at remarkably large distances. This is already known, and our group made key contributions to this knowledge. What is unknown is whether, and to what extent, the neutrons and protons can show different collective behaviours. Also unknown, for most elements, is how many neutrons can bind to a given number of protons. It is features such as these that determine how stars explode. To tackle these problems, we need a more sophisticated understanding of the nuclear force, and we need experimental information about nuclei with unusual combinations of neutrons and protons to test our theoretical ideas and models. Therefore, theory and experiment go hand-in-hand as we push forward towards the nuclear limits.An overview of nuclear binding reveals that about one half of predicted nuclei have never been observed, and the vast majority of this unknown territory involves nuclei with an excess of neutrons. Much of our activity addresses this "neutron-rich" territory, exploiting the new capabilities with radioactive beams. Our principal motivation is the basic science, and we contribute strongly to the world sum of knowledge and understanding. Nevertheless, there are more-tangible benefits. For example, our radiation-detector advances can be incorporated in medical diagnosis and treatment. In addition, we provide an excellent training environment for our research students and staff, many of whom go on to work in the nuclear power industry, helping to fill the current skills gap. On a more adventurous note, our special interest in nuclear isomers (energy traps) could lead to novel energy applications. Furthermore, we have a keen interest in sharing our specialist knowledge with a wide audience, and we already have an enviable track record with the media.

核物理研究正在经历一场变革。一百年来，原子核一直是通过稳定的光束和稳定的目标之间的碰撞来探测的，只有少量的放射性同位素可用。现在，在过去20年稳步进展的基础上，终于有可能产生各种短寿命同位素的强束，即所谓的“放射性束”。这使我们能够大大扩大核实验研究的范围。例如，现在计划在实验室中研究爆炸恒星中发生的一系列核反应是现实的。因此，我们将能够理解我们在地球上发现的化学元素是如何形成和分布在宇宙中的。我们实验研究的核心是我们在国际领先的放射性束设施的大力参与。虽然我们现在正在或计划为这些设施的实质性技术发展做出贡献，但目前的拨款请求重点是利用现在可用的能力。实验进展与理论密切相关，新颖和实用的方法是萨里小组的标志。一个突出的特点，这是我们集团的研究计划的关键，是在英国独一无二的，是我们强大的理论和实验能力的结合。我们的科学目标与当前STFC的核物理战略一致，如核物理咨询小组所详细表示的那样。我们希望了解核存在的边界，即使中子和质子结合在一起形成原子核的限制条件。在这种情况下，核系统处于微妙的状态，并显示出异常现象。它对核力的性质非常敏感。例如，弱束缚的中子可以在相当大的距离内绕母核运行。这是众所周知的，我们的团队为这一知识做出了关键贡献。目前尚不清楚的是，中子和质子是否以及在多大程度上可以表现出不同的集体行为。对于大多数元素来说，也不知道有多少中子可以与给定数量的质子结合。正是这些特征决定了恒星如何爆炸。为了解决这些问题，我们需要对核力有更深入的了解，我们需要关于中子和质子不寻常组合的原子核的实验信息来检验我们的理论想法和模型。因此，当我们向核极限迈进时，理论和实验是齐头并进的。核束缚的概述表明，大约一半的预测核从未被观察到，而这个未知领域的绝大多数涉及中子过剩的核。我们的大部分活动都是针对这一“富含中子”的领域，利用放射性束的新能力。我们的主要动机是基础科学，我们为世界知识和理解的总和做出了巨大贡献。然而，还有更切实的好处。例如，我们在辐射探测器方面的进步可以用于医疗诊断和治疗。此外，我们为研究生和员工提供优良的培训环境，其中许多人继续在核电行业工作，帮助填补当前的技能缺口。在一个更冒险的注意，我们对核异构体（能量陷阱）的特殊兴趣可能会导致新的能源应用。此外，我们有兴趣与广大观众分享我们的专业知识，我们已经与媒体有一个令人羡慕的记录。