Nuclear Astrophysics at TRIUMF-ISAC: Stellar Burning Reaction Studies with DRAGON and TUDA

TRUMF-ISAC 的核天体物理学：使用 DRAGON 和 TUDA 研究恒星燃烧反应

• 批准号: SAPPJ-2016-00029
• 负责人: Ruiz, Chris
• 金额: $ 12.75万
• 依托单位: TRIUMF
• 依托单位国家: 加拿大
• 项目类别: Subatomic Physics Envelope - Project
• 财政年份: 2017
• 资助国家: 加拿大
• 起止时间: 2017-01-01 至 2018-12-31
• 项目状态: 已结题
• 来源: https://www.nserc-crsng.gc.ca/ase-oro/Details-Detailles_eng.asp?id=617798
• 关键词: Nuclear; Astrophysics; TRIUMF; ISAC; Stellar

It is presently accepted that most of the chemical elements heavier than boron were produced in stars through nuclear reactions involving stable and radioactive nuclei and radioactive decays. Astrophysical models of the various stages of stellar evolution (e.g. quiescent burning, or explosive processes as seen in novae and supernovae) that contribute to this nucleosynthesis have recently become more advanced, enabling good predictions of astronomical observables. Examples of these are isotopic abundances frozen into dust grains that make up our solar system, gamma-ray fluxes from synthesized long-lived radionuclides, optical or x-ray luminosity etc. These quantities can be compared with astronomical observations, including those from orbiting gamma ray observatories or laboratory measurements on meteoric grains. This comparison is a powerful tool in the field of astrophysics and cosmology, giving us the most direct imaging technique of the nuclear processes inside stars and their explosions. In order to improve the models, and therefore advance our understanding of these powerful and mysterious stellar events, a precise knowledge of the nuclear reactions involved in energy generation and nucleosynthesis is required.

目前公认的是，大多数比硼重的化学元素都是在恒星中通过涉及稳定和放射性核以及放射性衰变的核反应产生的。恒星演化各个阶段的天体物理模型（例如，在新星和超新星中看到的静态燃烧或爆炸过程）有助于这种核合成，最近变得更加先进，能够很好地预测天文观测。例如，构成我们太阳系的尘埃颗粒中的同位素丰度，合成的长寿命放射性核素的伽马射线通量，光学或X射线光度等，这些量可以与天文观测进行比较，包括轨道伽马射线观测站或实验室对流星颗粒的测量。这种比较是天体物理学和宇宙学领域的一个强大工具，为我们提供了恒星内部核过程及其爆炸的最直接成像技术。为了改进模型，从而推进我们对这些强大而神秘的恒星事件的理解，需要精确了解能量产生和核合成中涉及的核反应。