Constraining gravity with cosmology

用宇宙学约束引力

• 批准号: ST/S004572/3
• 负责人: Johannes Noller
• 金额: $ 19.12万
• 依托单位: University College London
• 依托单位国家: 英国
• 项目类别: Fellowship
• 财政年份: 2023
• 资助国家: 英国
• 起止时间: 2023 至 无数据
• 项目状态: 未结题
• 来源: https://gtr.ukri.org/projects?ref=ST%2FS004572%2F3
• 关键词: Constraining; gravity; cosmology

The recent past has witnessed phenomenal successes in cosmology, constraining the structure, content and evolution of the Universe with tremendous accuracy. Consequently, a current focus of cosmology is to gain an understanding of the agents behind this evolution, identifying the fundamental physics behind the accelerated expansion of the Universe at early and late times and the nature of dark energy and dark matter. Key to this enterprise is thoroughly understanding gravity itself - the least well-understood of the known forces in nature. Specifically, this involves testing, constraining (and potentially detecting deviations from) our current best working theory: General Relativity. With the emergence of new observational windows (e.g. the first detections of gravitational waves) in addition to other well-established probes of gravity (e.g. observations of the cosmic microwave background), we presently have a remarkable and continuously growing amount of data allowing us to precisely measure gravitational phenomena. Simultaneously, recent theoretical advances in understanding what features a consistent theory of gravity must possess, enable us to impose additional strong restrictions on how gravity can behave and and how it interacts with matter in the universe. Altogether this means we currently have at our disposal an unprecedented amount of powerful instruments to precisely identify and constrain the nature of gravity. Given the different areas of physics they originate from, these instruments have not been used jointly so far, yet the qualitatively different ways in which they operate means they in fact ideally complement one another, testing and probing gravity in a variety of different ways. This research program therefore aims to take full advantage of this complementarity, integrating methods ranging from the development of data-driven numerical codes to the implementation of theoretical bounds from high-energy particle physics in order to obtain the most systematic and tight bounds on gravity yet. In this way, we will be able to thoroughly probe the nature of gravity, testing several of its fundamental properties in the process.

最近的过去见证了宇宙学的巨大成功，以极大的准确性限制了宇宙的结构，内容和演化。因此，宇宙学目前的重点是了解这种演变背后的因素，确定宇宙早期和晚期加速膨胀背后的基本物理学以及暗能量和暗物质的性质。这项事业的关键是彻底理解重力本身-自然界中已知的力量中最不为人所知的力量。具体来说，这涉及到测试，约束（并可能检测偏离）我们目前最好的工作理论：广义相对论。随着新的观测窗口（例如引力波的首次探测）以及其他成熟的引力探测（例如宇宙微波背景辐射的观测）的出现，我们目前拥有显着且不断增长的数据量，使我们能够精确测量引力现象。与此同时，最近在理解一个相容的引力理论必须具备的特征方面的理论进展，使我们能够对引力如何表现以及它如何与宇宙中的物质相互作用施加额外的强有力的限制。总而言之，这意味着我们目前拥有前所未有的强大工具来精确识别和限制重力的性质。鉴于它们来自不同的物理学领域，这些仪器到目前为止还没有联合使用，但它们的操作方式在性质上不同，这意味着它们实际上是理想的互补，以各种不同的方式测试和探测引力。因此，该研究计划旨在充分利用这种互补性，整合从开发数据驱动的数值代码到实施高能粒子物理学理论边界的方法，以获得最系统和最紧密的引力边界。通过这种方式，我们将能够彻底探索引力的本质，在这个过程中测试它的几个基本性质。