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IRIS : Charged particle reaction spectroscopy at ISAC

IRIS：ISAC 的带电粒子反应光谱

基本信息

批准号：
SAPPJ-2018-00024
负责人：
Kanungo, Rituparna
金额：
$ 17.48万
依托单位：
Saint Mary's University
依托单位国家：
加拿大
项目类别：
Subatomic Physics Envelope - Project
财政年份：
2020
资助国家：
加拿大
起止时间：
2020-01-01 至 2021-12-31
项目状态：
已结题

来源：
https://www.nserc-crsng.gc.ca/ase-oro/Details-Detailles_eng.asp?id=718937
关键词：
IRIS Charged particle reaction spectroscopy

项目摘要

A large part of our universe is powered by nuclear reactions, that are the secret behind the glow of the sun and the shine of the stars. In our laboratories nuclear reactions and scattering are the ways to uncover the secrets that lie in the heart of visible matter in our universe. This project focuses on exploring the rare isotopes with a large excess of neutrons over protons or vice versa, that are created in certain environments of our universe such as supernovae, neutron stars etc. New discoveries about their unknown properties become possible using the facility IRIS at Canada's National Laboratory for subatomic physics, TRIUMF in Vancouver, BC. The IRIS facility has pioneered in the use of an thin frozen sheet of solid hydrogen as reaction target. The hydrogen isotope of the target interacts with accelerated beams of rare isotopes produced at TRIUMF. By observing the particles emitted from this interaction process we get a peek into the properties of rare isotopes. This reveals how nature arranges the building blocks to build these isotopes and hence deduce the properties of nature's strongest force (nuclear force). This also allows us to unravel how nature creates the majority of the heavy elements that we find on earth. The unexpected characteristics of these unstable nuclei make it necessary to seek answers to the fundamental question on how nature organizes the neutrons and protons to form a bound systems with highly asymmetric neutron to proton ratio and how do they behave at the limit when they become unbound.

我们宇宙的很大一部分是由核反应提供动力的，这是太阳和星星发光背后的秘密。在我们的实验室里，核反应和散射是揭开宇宙可见物质核心秘密的方法。这个项目的重点是探索稀有同位素与大量过剩的中子超过质子或反之亦然，这是在我们的宇宙，如超新星，中子星等的某些环境中创建的新发现，其未知的属性成为可能使用设施IRIS在加拿大国家实验室的亚原子物理学，TRIUMF在温哥华，BC。IRIS设施率先使用固体氢的薄冷冻片作为反应目标。靶的氢同位素与TRIUMF产生的稀有同位素加速束相互作用。通过观察从这种相互作用过程中发射出来的粒子，我们可以一窥稀有同位素的性质。这揭示了大自然如何安排构建这些同位素的积木，从而推导出自然界最强力（核力）的性质。这也使我们能够解开大自然如何创造我们在地球上发现的大多数重元素。这些不稳定核的意外特性使得有必要寻求基本问题的答案，即自然界如何组织中子和质子以形成具有高度不对称的中子质子比的束缚系统，以及当它们变得不束缚时它们如何在极限处表现。