Energetic particle interactions in the universe: consequences for cosmic ray, gamma ray and neutrino astrophysics

宇宙中的高能粒子相互作用：对宇宙射线、伽马射线和中微子天体物理学的影响

• 批准号: ARC : DP0211292
• 负责人: Dr Raymond Protheroe
• 金额: $ 29.6万
• 依托单位: The University of Adelaide
• 依托单位国家: 澳大利亚
• 项目类别: Discovery Projects
• 财政年份: 2002
• 资助国家: 澳大利亚
• 起止时间: 2002-01-01 至 2005-12-31
• 项目状态: 已结题
• 来源: https://researchdata.edu.au/energetic-particle-interactions-neutrino-astrophysics/64714
• 关键词: Energetic; particle; interactions; universe; consequences

Energetic particle interactions in the universe: consequences for cosmic ray, gamma ray and neutrino astrophysics. The most energetic phenomena in the Universe will be explored with giant cosmic ray, neutrino and gamma ray telescopes. Particles accelerated or produced in astrophysical sources interact in their magnetic, matter and radiation environment, making cosmic rays, gamma rays and neutrinos. Subsequently, interactions in space as they travel to Earth change what we see. With theoretical work proposed in this project we aim to determine where in the Universe the highest energy cosmic rays originate, and the fundamental processes responsible for them. It will also lead to a greater understanding of how active galaxies and other astrophysical objects function.

宇宙中高能粒子的相互作用：宇宙射线、伽马射线和中微子天体物理学的结果。宇宙中最具能量的现象将通过巨型宇宙射线、中微子和伽马射线望远镜进行探索。在天体物理源中加速或产生的粒子在其磁场、物质和辐射环境中相互作用，产生宇宙射线、伽马射线和中微子。随后，当它们到达地球时，在太空中的相互作用改变了我们所看到的。通过在这个项目中提出的理论工作，我们的目标是确定宇宙中能量最高的宇宙射线起源于哪里，以及产生它们的基本过程。它还将使人们更好地了解活跃星系和其他天体的功能。