Development of an RF Fragment Separator at the NSCL

NSCL 开发射频片段分离器

• 批准号: 0520930
• 负责人: Hendrik Schatz
• 金额: $ 25.12万
• 依托单位: Michigan State University
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2005
• 资助国家: 美国
• 起止时间: 2005-09-15 至 2008-08-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=0520930&HistoricalAwards=false
• 关键词: Development; RF; Fragment; Separator; NSCL

Extremely unstable neutron deficient rare isotopes play a key role in explosive astrophysical events such as X-ray bursts and Novae. An understanding of the physics of these exotic nuclei is required to interpret in a quantitative way a range of new X-ray binary observations from space based X-ray observatories. This will pave the way to address the many open questions such as the mechanism behind burst oscillations, the origin of superbursts, and the nature of the underlying neutron star. Very neutron deficient nuclei serve also as unique probes of nuclear structure. They provide tests for the limits of nuclear existence, and they show unique decay modes such as one- and two-proton emission. In addition, neutron deficient nuclei include a special class of nuclei - isotopes with equal numbers of protons and neutrons. As protons and neutrons occupy the same shell model orbitals, many nuclear structure effects appear enhanced in such nuclei. This is particularly true for one of the most neutron deficient, classically doubly magic nuclei in nature, 100Sn. Doubly-magic nuclei, where both, protons and neutrons completely fill a nuclear shell, are of particular importance in nuclear physics and serve as benchmarks and beachheads for nuclear theories. The measurement of the decay properties of 100Sn is by many considered one of the "holy grails" of nuclear physics and would provide unique insights into the beta-decay of heavy nuclei. The National Superconducting Cyclotron Laboratory (NSCL) at Michigan State University has worldwide unique capabilities in producing extremely neutron deficient nuclei. This includes sufficient amounts of 100Sn to measure the properties of its decays,as well as all nuclei participating in the astrophysical rapid proton capture process in X-ray bursts. However, due to the nature of the projectile fragmentation mechanism used to create these nuclei, current experimental setups do not achieve the necessary beam purity.Many of the key experiments can therefore not be performed. We will build an RF Fragment Separator experiment, which will deflect unwanted rare isotope beam contaminants with an RF field, while transmitting the desired species. This device can be combined with existing experimental setups for decay and reaction studies and will allow a large group of graduate students and scientists to take full advantage of the production capabilities for neutron deficient beams at the NSCL to address fundamental questions in nuclear physics and astrophysics.

极不稳定的缺中子稀有同位素在X射线爆发和新星等爆炸性天体物理事件中起着关键作用。 了解这些奇异的核的物理需要以定量的方式解释一系列新的X射线双星观测空间为基础的X射线天文台。这将为解决许多悬而未决的问题铺平道路，如爆发振荡背后的机制，超级爆发的起源，以及潜在的中子星星的性质。 非常缺中子的原子核也是核结构的独特探针。它们为核存在的极限提供了测试，并显示出独特的衰变模式，如单质子和双质子发射。此外，缺中子核还包括一类特殊的核--质子数和中子数相等的同位素。由于质子和中子占据相同的壳模型轨道，许多核结构效应在这样的核中出现增强。 这对于自然界中最缺中子的经典双魔核之一100 Sn来说尤其如此。双魔核，其中质子和中子完全填充核壳层，在核物理学中特别重要，并作为核理论的基准和滩头阵地。测量100 Sn的衰变特性被许多人认为是核物理学的“圣杯”之一，并将为重核的β衰变提供独特的见解。位于密歇根州立大学的国家超导回旋加速器实验室（NSCL）在生产极缺中子核方面具有世界上独一无二的能力。这包括足够数量的100 Sn来测量其衰变的性质，以及参与X射线爆发中天体物理快速质子捕获过程的所有核。 然而，由于用于产生这些核的射弹碎裂机制的性质，当前的实验装置不能达到必要的束流纯度。因此，许多关键实验不能进行。 我们将建立一个RF碎片分离器实验，它将用RF场偏转不需要的稀有同位素束污染物，同时传输所需的物质。该设备可以与现有的衰变和反应研究的实验装置相结合，并将允许一大群研究生和科学家充分利用NSCL的中子缺陷束的生产能力，以解决核物理和天体物理中的基本问题。