High Energy Physics

粒子物理学的标准模型（SM）是对由强、电磁和弱力控制的相互作用的优雅理论描述。这个基本而重要的模型仍然是坚实的基础，成功地将数值归因于500范围内的所有物理观测值。随着技术的改进，提出并进行了新的实验。这些实验验证了标准模型的预言，并提出了对超越标准模型（BSM）物理学的需求。在所有的BSM问题中，最重要的是neu-特里诺质量，暗物质和物质-反物质不对称性。为了同时解决这些问题，人们提出了许多模型。需要新的唯象学工具来确认这些BSM问题的解决方案。引力波是探索早期宇宙物理模型的重要工具之一。冰立方中微子望远镜发现的高能中微子也可能有宇宙学的起源。这些可以用来测试物质起源的模型。该研究项目将涉及这些广泛的主题。第一年将确定一个更具体的研究项目。

The Standard Model(SM) of Particle Physics is an elegant theoretical description of the interactions governed by strong, electromagnetic, and weak forces. This basic yet important model is still firm at the foundation, succeeding in attributing numerical values to all the physical observables within the 500 range. With the advent of improved technologies, new experiments were proposed and performed. These experiments verified SM predictions and presented the need for Beyond Standard Model(BSM) Physics. Amongst all the BSM problems, the most important are neu- trino mass, dark matter, and matter-antimatter asymmetry. Many models have been proposed in an attempt to ad-dress these problems simultaneously. New phenomenological tools are required to confirm solutions to these BSM problems. A gravitational wave is one of the most important tools in probing the early universe physics models. The high-energy neutrinos discovered at the IceCube neutrino telescope might as well have a cosmological origin. These can be used to test the models on the origin of matter. The research project will deal with these broad topics. A more specific research project will be defined during the 1st year.