Extreme Laboratory Astrophysics and high photon energy source development.

极限实验室天体物理学和高光子能源开发。

• 批准号: 2285995
• 金额: --
• 依托单位: University of Oxford
• 依托单位国家: 英国
• 项目类别: Studentship
• 财政年份: 2019
• 资助国家: 英国
• 起止时间: 2019 至 无数据
• 项目状态: 已结题
• 来源: https://gtr.ukri.org/projects?ref=studentship-2285995
• 关键词: Extreme; Laboratory; Astrophysics; photon; energy

With the advent of high power laser facilities such as the Extreme Light Infrastructure (ELI), the focussed laser intensity is becoming large enough to be able to excite astrophysical processes that are relevant to the early Universe. These include magnetized supersonic turbulence, generation of (pseudo)scalar fields, and high energy x-ray and gamma-ray sources. In this project, the student will be involved in developing the underlying theory and designing experiments that can access these regimes. The core of the experimental work will focus on high energy electron beam colliding with optical laser pulses in order to produce both gamma-ray pulses (by inverse Compton scattering) and (pseudo)scalar particles. The application of this work is both towards the understanding of extreme astrophysical processes as well as for the generation of intense x-ray and gamma-ray pulses. The latter will be important for material studies in inertial fusion energy and is of direct interest to AWE.

随着诸如极光基础设施（ELI）等高功率激光设施的出现，聚焦的激光强度变得足够大，能够激发与早期宇宙相关的天体物理过程。这些包括磁化超音速湍流，（伪）标量场的产生，以及高能X射线和伽马射线源。在这个项目中，学生将参与开发基础理论和设计实验，可以访问这些制度。实验工作的核心将集中在高能电子束与光学激光脉冲碰撞，以产生伽马射线脉冲（通过逆康普顿散射）和（伪）标量粒子。这项工作的应用是对极端天体物理过程的理解，以及产生强烈的X射线和伽马射线脉冲。后者对于惯性聚变能的材料研究将是重要的，并与AWE直接相关。