Decay Spectroscopy of Exotic Nuclei at FAIR

FAIR 中奇异核的衰变光谱

• 批准号: EP/E001734/1
• 负责人: Philip J Woods
• 金额: $ 99.5万
• 依托单位: University of Edinburgh
• 依托单位国家: 英国
• 项目类别: Research Grant
• 财政年份: 2006
• 资助国家: 英国
• 起止时间: 2006 至 无数据
• 项目状态: 已结题
• 来源: https://gtr.ukri.org/projects?ref=EP%2FE001734%2F1
• 关键词: Decay; Spectroscopy; Exotic; Nuclei; FAIR

It is an astonishing fact that most of the chemical elements we observe today were created from the ashes of ancient stellar explosions. The most spectacular events of this type are supernovae. With very high sensitivity modern telescopes we can study the chemical abundances of material ejected from distant supernovae and compare these abundances with those found in our own solar system. Understanding these abundances turns out to crucially depend on nuclear reaction processes. Stars can be thought of as naturally occurring nuclear reactors held together by gravity. Fortunately for us the sun is not currently in an explosive phase of development. However, most of the elements now present in the solar system were in fact produced in earlier generations of exploding stars. In this sense, we can think of ourselves as cosmic debris. The reaction processes in exploding stars are very different to those found in the sun, and involve nuclear species never seen before on our planet. Rather like chemicals that behave very differently according to their electronic shell structure - sodium is highly reactive with water but neon with one less electron is an inert gas - nuclear species can either be very stable or very reactive according to their precise composition of protons and neutrons. Reactions involving these previously unobserved nuclear species are responsible for the chemical abundances we observe today, but until now we have had no chance to study them. The new FAIR accelerator being built in Germany is the only one in the world that can produce intense, high energy beams of the heaviest naturally occurring element, Uranium. This element itself will have been produced during ancient supernova explosions in a chain of nuclear reactions scientists call the r-process in which many neutrons are rapidly absorbed by a seed nucleus! Our experiments will reverse this process, and use advanced separation and detector equipment to observe new exotic nuclear species produced

令人惊讶的是，我们今天观察到的大多数化学元素都是从古代恒星爆炸的灰烬中产生的。这类事件中最壮观的是超新星。借助灵敏度非常高的现代望远镜，我们可以研究从遥远的超新星喷出的物质的化学丰度，并将这些丰度与我们太阳系中发现的丰度进行比较。了解这些丰度的关键取决于核反应过程。恒星可以被认为是自然发生的核反应堆，通过引力结合在一起。对我们来说幸运的是，太阳目前还没有处于爆炸性的发展阶段。然而，现在太阳系中存在的大多数元素实际上是在早期爆炸的恒星中产生的。从这个意义上说，我们可以把自己想象成宇宙碎片。爆炸恒星中的反应过程与太阳中的反应过程非常不同，并且涉及我们星球上从未见过的核物质。就像化学物质根据它们的电子壳层结构表现出非常不同的行为一样-钠与水高度反应，但少一个电子的氖是惰性气体-核物种可以根据质子和中子的精确组成非常稳定或非常活跃。涉及这些以前未观察到的核物种的反应是我们今天观察到的化学丰度的原因，但直到现在我们还没有机会研究它们。正在德国建造的新的FAIR加速器是世界上唯一一个可以产生最重的天然元素铀的强烈高能束的加速器。这种元素本身可能是在古代超新星爆炸的一系列核反应中产生的，科学家们称之为r过程，在这一过程中，许多中子被种子核迅速吸收！我们的实验将逆转这一过程，并使用先进的分离和检测设备来观察新的外来核物种产生

项目成果

The Advanced Implantation Detector Array (AIDA)

• DOI: 10.1016/j.nima.2023.168166
• 发表时间: 2023-02
• 期刊: Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
• 作者: O. Hall;T. Davinson;C. Griffin;P. Woods;C. Appleton;C. Bruno;A. Estrade;D. Kahl;L. Sexton;I. Burrows;P. Coleman-Smith;M. Cordwell;A. Grant;M. Kogimtzis;M. Labiche;J. Lawson;I. Lazarus;P. Morall;V. Pucknell;J. Simpson;C. Unsworth;D. Braga;M. Prydderch;S. Thomas;L. Harkness-Brennan;P. Nolan;R. Page;D. Seddon