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

同位旋不对称性是有限核和/或无限核物质中中子和质子数量之间不平衡的度量。在极端的同位旋不对称系统中，比如中子星，中子和质子是如何相互作用的？ 状态方程，即，能量，密度和温度之间的关系，变化作为丰中子核物质中的同位旋不对称性的函数？这些问题的答案对中子星的结构和超新星爆炸的动力学有着重要的天体物理学意义。 然而，天体物理学观测太有限，无法回答这些问题。 幸运而有趣的是，这些问题可以通过在美国计划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引起的核反应进行实验研究。与这些实验相关的物理学是目前核科学的主要研究方向之一，也是核科学的最前沿。特别是，在RIA的高能富中子束，可以创建一个瞬态的核物质与可观的同位旋不对称性和压缩的两倍以上的正常核物质的饱和密度。 因此，放射免疫分析将提供一个独特的机会，探索核子物质的性质，在极端条件下的同位旋不对称性和密度。为了使介质内核有效相互作用和核状态方程的同位旋依赖性实验研究取得成功，我将通过研究丰中子物质的新性质及其在稀有同位素束引起的核反应中的表现，对计划实验和解释数据的几个重要问题进行理论研究。我工作的主要重点将是开发放射性束诱导核反应的新模型;确定反应动力学中的同位旋自由度的作用;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可观测量;并限制同位旋不对称核物质的状态方程。

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.