High Energy Physics

粒子物理学的标准模型（SM）是对由强、电磁力和弱力控制的相互作用的一种优雅的理论描述。这个基本而重要的模型在基础上仍然是稳固的，它成功地将500范围内的所有物理观测值归因于数值。随着技术的进步，人们提出并进行了新的实验。这些实验验证了SM的预测，并提出了超越标准模型（BSM）物理学的必要性。在所有的BSM问题中，最重要的是新中微子质量、暗物质和物质-反物质不对称。人们提出了许多模型，试图同时解决这些问题。需要新的现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最重要的工具之一。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。一个更具体的研究项目将在第一年确定。

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.