Experimental Particle Physics at the University of Edinburgh

爱丁堡实验粒子物理小组目前正在进行三个不同的运行实验，我们还在进行几个未来的项目。大型强子对撞机(LHC)的ATLAS实验：Atlas是能够研究由质子以有史以来最高能量碰撞产生的各种粒子的两个探测器之一，它解决了基本问题。最广为人知的是质量的起源。美丽的对称性是我们理解粒子相互作用的基础，它内在地要求所有粒子都是无质量的。事实并非如此，提出的优雅解决方案现在被称为希格斯机制。希格斯玻色子的发现证实了这一点，现在我们必须非常详细地测量它的性质。ATLAS解决的另一个领域是寻找新的重粒子，如新的重希格斯粒子或超对称粒子，这些粒子是在试图解决标准模型(SM)缺点的模型中预测的，例如为什么会有暗物质。大型强子对撞机上的LHCb实验。在20世纪60年代之前，人们一直认为物质和反物质的行为是一样的。然而，人们发现这种对称性被破坏了，而且该物质的行为方式与反物质不同。这体现在CP破坏现象中，对于理解早期宇宙是必不可少的。大爆炸后不久，就有了等量的物质和反物质。在膨胀和冷却期间，物质和反物质会湮灭成光子，留下一个充满辐射的宇宙，但没有恒星和星系。萨卡洛夫在1967年证明，如果满足包括CP破坏在内的三个条件，那么就有可能产生物质对反物质的微小不平衡，这将足以解释宇宙的存在。LHCb测量至少有一个b夸克或反b夸克的粒子和反粒子的行为差异(CP破坏)，并搜索这些粒子的非常罕见的衰变，这可能会受到重的未观察到的粒子的影响。LUX-ZEPLIN实验，这是世界上搜索暗物质最灵敏的设备。众所周知，宇宙的27%是由暗物质组成的--即某种形式的物质，它不会以产生辐射的方式相互作用，也不会有其他容易观察到的信号。有许多理论上的候选者，而解开这个谜团必须包括直接探测我们自己的银河系暗物质。我们领导着合作工作，以探测特别有动力的可能性，包括轴子和暗声子。我们还在努力设计、开发和建造大约2020年的大型强子对撞机的升级探测器。光束的强度将增加，探测器记录的数据速率将增加数量级。这需要建造新的探测器来精确测量长寿命粒子的轨迹，测量切伦科夫光子以确定它们的速度，以及更快、更强大的模拟，以及处理海量数据速率的新方法。我们现在已经完成了LUX-ZEPLIN项目的建设，预计该项目将在未来十年主导对暗物质的直接搜索。我们致力于10吨液体氙气的模拟、控制系统和分析。我们已经在即将建造的沙丘和Hyper-K实验中增加了我们的中微子物理活动。自然界最有趣的事实之一是，只有三种中微子，直到最近还被认为是无质量的。精确测量中微子之间的“混合”和寻找中微子的CP破坏是很重要的。我们还加入了MicroBooNE和SBND实验，这两个实验将寻找新的、无菌的中微子，这些中微子只通过引力相互作用，而不与SM的任何基本相互作用。

The Edinburgh Experimental Particle Physics group is currently working in three different running experiments and we are also working on several future projects.The ATLAS experiment at the Large Hadron Collider (LHC): ATLAS is one of two detectors able to study a wide variety of particles created from the collision of protons at the highest energies ever created, and it addresses fundamental questions. The most well known is that of the origin of mass. The beautiful symmetry which underlies our understanding of particle interactions inherently demands that all particles are massless. This cannot be the case, and the elegant solution put forward is now known as the Higgs mechanism. The discovery of the Higgs boson has verified this, and now we must measure its properties in great detail. Another area addressed by ATLAS is the search for new heavy particles such as new heavy Higgs like particles or supersymmetric particles, which are predicted in models trying to address shortcomings of the Standard Model (SM), such as why there is dark matter.The LHCb experiment at the LHC. Prior to the 1960s, it had been thought that matter and anti-matter would behave in the same way. However, it was discovered that this symmetry was violated, and that matter does not behave in an identical way to anti-matter. This is embodied in the phenomenon of CP violation and is essential to the understanding of the early universe. Shortly after the big bang there were equal amounts of matter and anti-matter. During expansion and cooling, matter and anti-matter would have annihilated into photons to leave a universe full of radiation, but no stars and galaxies. It was shown in 1967 by Sakarov that if three conditions, including CP violation, were met, then it would be possible for a small imbalance of matter over anti-matter to accrue, which would be sufficient to explain the existence of the universe. LHCb measures differences (CP violation) in behaviour of particles and antiparticle with at least one b or anti-b quark and searches for very rare decays of these particles, which could be affected by heavy unobserved particles. The LUX-ZEPLIN experiment, which is the world's most sensitive apparatus searching for dark matter. It is well known that some 27% of the Universe is comprised of Dark Matter - that is matter of some form which does not interact in a way that produces radiation, or other easy to observe signatures. There are many theoretical candidates and resolution of this mystery must include the direct detection of our own galactic dark matter. We lead the collaboration's efforts to detect particularly well-motivated possibilities including axions and dark phonons.We are also working hard on the design, development and construction of the upgraded detectors at the LHC for around 2020. The intensity of the beams will be increased and the data rates recorded by the detectors will increase by orders of magnitude. This requires building new detectors for precisely measuring trajectories of longlived particles, for measuring Cherenkov photons to determine their speed, and faster and more powerful simulation, and new ways to handle the massive data rates. We have now completed the construction of the LUX-ZEPLIN project, expected to dominate direct searches for dark matter in the next decade. We work on simulations, control systems for the 10 tonnes of liquid xenon, and analysis.We have grown our neutrino physics activities in the DUNE and Hyper-K experiments to be constructed. One of the most interesting facts of nature is that there are only three species of neutrinos, which until recently were thought to be massless. It is important to measure precisely the "mixing" between the species and to search for CP violation in neutrinos. We have also joined the MicroBooNE and SBND experiments, which will search for new, sterile, neutrinos which interact only via gravity but not with any of the fundamental interactions of the SM.