Probing the Isospin Dependence of In-Medium Nuclear Effective Interactions at the Rare Isotope Accelerator

探讨稀有同位素加速器中介质核有效相互作用的同位旋依赖性

• 批准号: 0652548
• 负责人: Bao-An Li
• 金额: --
• 依托单位: Texas A&M University-Commerce
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 2006
• 资助国家: 美国
• 起止时间: 2006-09-01 至 2009-10-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=0652548&HistoricalAwards=false
• 关键词: Probing; Isospin; Dependence; Medium; Nuclear

Isospin asymmetry is a measure of the imbalance between the numbers of neutrons and protons in finite nuclei and/or infinite nuclear matter. How do neutrons and protons interact among themselves in extremely isospin asymmetric systems, such as, neutron stars? How does the equation of state, i.e., a relationship among energy, density and temperature, change as a function of isospin asymmetry in neutron-rich nuclear matter? Answers to these questions have significant astrophysical ramifications for the structure of neutron stars and the dynamics of supernova explosions. However, astrophysical observations are too limited to answer these questions. Fortunately and interestingly, these questions can be studied experimentally by using nuclear reactions induced by short-lived isotope beams at the planned Rare Isotope Accelerator (RIA) in the USA and other competing facilities abroad. The physics associated with these experiments is currently one of the major thrusts and at the foremost front of nuclear sciences. In particular, with high energy neutron-rich beams at RIA, a transient state of nuclear matter with appreciable isospin asymmetry and compression of more than twice the saturation density of normal nuclear matter can be created. RIA will thus provide a unique opportunity to explore the nature of nucleonic matter under extreme conditions of isospin asymmetry and density. To facilitate the success of the experimental research on the isospin dependence of the in-medium nuclear effective interactions and the nuclear equation of state, I shall carry out theoretical studies on several issues important for planning experiments and interpreting data by investigating novel properties of neutron-rich matter and their manifestations in nuclear reactions induced by rare isotope beams. The major foci of my work will be on developing new models for nuclear reactions induced by radioactive beams; identifying the role of isospin degree of freedom in the reaction dynamics; determining experimental observables that can be used to extract critical information about the isospin dependence of the in-medium nuclear effective interactions; and constraining the equation of state of isospin asymmetric nuclear matter.

同位旋不对称是有限核和/或无限核物质中中子和质子数量不平衡的量度。中子和质子是如何在极端同位旋不对称系统中相互作用的，比如中子星？在富含中子的核物质中，状态方程（即能量、密度和温度之间的关系）如何作为同位旋不对称性的函数而变化？这些问题的答案对于中子星的结构和超新星爆炸的动力学具有重要的天体物理学意义。然而，天体物理观测太有限，无法回答这些问题。幸运和有趣的是，这些问题可以通过在美国计划中的稀有同位素加速器（RIA）和国外其他竞争设施中使用短寿命同位素束诱导的核反应进行实验研究。与这些实验相关的物理学目前是核科学的主要推动力之一，处于最前沿。特别是，在RIA中使用高能富中子束，可以产生具有明显同位旋不对称性和压缩密度超过正常核物质饱和密度两倍的核物质的瞬态。因此，RIA将提供一个独特的机会来探索核物质在同位旋不对称和密度的极端条件下的本质。为了使介质内核有效相互作用的同位旋依赖性和核状态方程的实验研究取得成功，我将通过研究富中子物质的新性质及其在稀有同位素束诱导的核反应中的表现，对规划实验和解释数据的几个重要问题进行理论研究。我的主要工作重点将是发展放射性光束引起的核反应的新模型；确定同位旋自由度在反应动力学中的作用；确定可用于提取有关介质内核有效相互作用的同位旋依赖性的关键信息的实验观测值；约束了同位旋不对称核物质的状态方程。