Holographic Approaches to Black Holes, Cosmology and Entanglement

黑洞、宇宙学和纠缠的全息方法

• 批准号: SAPIN-2015-00032
• 负责人: Maloney, Alexander
• 金额: $ 5.83万
• 依托单位: McGill University
• 依托单位国家: 加拿大
• 项目类别: Subatomic Physics Envelope - Individual
• 财政年份: 2018
• 资助国家: 加拿大
• 起止时间: 2018-01-01 至 2019-12-31
• 项目状态: 已结题
• 来源: https://www.nserc-crsng.gc.ca/ase-oro/Details-Detailles_eng.asp?id=658603
• 关键词: Holographic; Approaches; Black; Holes; Cosmology

I propose to investigate foundational questions at the interface of particle physics, string theory and cosmology. I will focus on basic conceptual puzzles in quantum gravity, and in particular on problems related to the physics of black holes and cosmology. To address these questions I will use the holographic principle, perhaps our most powerful tool in the study of quantum gravity. In particular, I will utilize emerging holographic techniques at the interface of particle physics and quantum information theory. This will allow us to address some of the most fundamental and long-standing problems in theoretical physics - those concerning the basic structure of space-time and the origin of our observable universe from a big bang singularity.***Many of the deepest questions in theoretical physics involve black holes. What is the nature of a black hole event horizon? Do black holes destroy information? Previous attempts to address these questions have focused only on special classes of black holes, which differ qualitatively from those relevant for astrophysics. This shortcoming must be addressed if we wish to understand the dynamics of realistic black holes, such as the one at the center of our galaxy.***A second set of questions is motivated by recent astronomical observations indicating that the universe began with a big bang singularity, followed by a period of exponential expansion known as inflation. Neither of these two features - the cosmological singularity and the inflating phase - have been successfully described in a fully consistent quantum theory of gravity. These problems, which must be solved if we are to successfully describe the observable universe, offer the exciting prospect of contact with experimental data.***To address these problems we need new tools and techniques to enable us to make sense of quantum gravity in regimes where general relativity breaks down. The most useful such tool is the holographic correspondence (or holography), which states that quantum gravity in a region of space is equivalent to a theory on the boundary of that region. In its most precise form, known as the Anti-de Sitter/Conformal Field Theory (AdS/CFT) correspondence, holography has allowed us to address these previously unsolvable problems in an exact manner.***Recently, these techniques have revealed a fascinating relationship between quantum gravity and quantum information theory. In particular, quantum entanglement - perhaps the most basic and mysterious feature of quantum mechanics - appears to be intimately related to black hole physics, and plays an important role in the emergence of classical space-time from more fundamental quantum degrees of freedom. This has yielded qualitatively new insights into black hole physics, and may have applications to cosmology as well. This remarkable cross-fertilization of ideas between different fields is one of the long-term goals of this proposal.**

我建议研究粒子物理学、弦理论和宇宙学的基础问题，我将重点关注量子引力的基本概念难题，特别是与黑洞物理学和宇宙学相关的问题。使用全息原理，这可能是我们研究量子引力最强大的工具，特别是，我将在粒子物理学和量子信息理论的交叉领域利用新兴的全息技术，这将使我们能够解决一些最基本和最长期的问题。 - 长期存在的问题理论物理学——涉及时空基本结构和我们可观测的宇宙从大爆炸奇点的起源。***理论物理学中的许多最深刻的问题都涉及黑洞事件视界的本质是什么。黑洞会破坏信息吗？以前解决这些问题的尝试只集中于特殊类型的黑洞，它们与天体物理学相关的黑洞有质的不同，如果我们希望了解现实黑洞的动力学，例如黑洞。作为我们的中心人物星系。***第二组问题是由最近的天文学观测引发的，这些观测表明宇宙始于大爆炸奇点，随后是一段称为暴胀的指数膨胀期，这两个特征——宇宙学奇点和膨胀——都不是。相位 - 已在完全一致的量子引力理论中成功描述。如果我们要成功描述可观测的宇宙，就必须解决这些问题，并提供了与实验联系的令人兴奋的前景数据。***为了解决这些问题，我们需要新的工具和技术，使我们能够在广义相对论失效的情况下理解量子引力。最有用的此类工具是全息对应（或全息术），它指出量子引力。空间区域中的重力相当于该区域边界的理论，其最精确的形式称为反德西特/共形场论（AdS/CFT）对应，全息术使我们能够解决这些问题。中无法解决的问题最近，这些技术揭示了量子引力和量子信息理论之间令人着迷的关系，特别是量子纠缠——也许是量子力学最基本和神秘的特征——似乎与黑洞物理学密切相关。 ，并在更基本的量子自由度的经典时空的出现中发挥了重要作用，这为黑洞物理学带来了质的新见解，并且也可能应用于宇宙学。不同的领域是该提案的长期目标之一。**