Uncovering the dynamics of black holes and neutron stars for gravitational wave and multimessenger astronomy

揭示黑洞和中子星的动力学，用于引力波和多信使天文学

• 批准号: RGPIN-2019-04226
• 负责人: East, William
• 金额: $ 2.4万
• 依托单位: University of Waterloo
• 依托单位国家: 加拿大
• 项目类别: Discovery Grants Program - Individual
• 财政年份: 2021
• 资助国家: 加拿大
• 起止时间: 2021-01-01 至 2022-12-31
• 项目状态: 已结题
• 来源: https://www.nserc-crsng.gc.ca/ase-oro/Details-Detailles_eng.asp?id=737493
• 关键词: Uncovering; dynamics; black; holes; neutron

With the stunning observations of gravitational waves from merging black holes and neutron stars made recently by LIGO/Virgo, we have entered a new age of multimessenger astronomy. There is every indication that as the number and sensitivity of gravitational wave detectors increase in the coming years, that there will be a flood of observations, revealing new aspects of the universe visible only in gravitational waves. However, maximizing the return of these observations, and utilizing them as a new probe of fundamental physics will require advances in our theoretical understanding of gravity in this regime. A central part of this proposal is to study neutron star mergers--the violent collision of the densest stars in the Universe--with the ultimate goal of understanding the gravitational wave signal, and accompanying electromagnetic transients, in order to aid in targeting and interpreting current and future observations. As part of achieving this long-term goal, my team and I will study several aspects of these systems that remain poorly understood, including the effects of neutron star spin and orbital eccentricity, and the dynamics of the post-merger remnant and accretion disk, and determine how they can shed light on the behavior of nuclear matter at the highest densities, the origin of the heaviest elements in the universe, and other questions. My team and I will study the underlying mechanisms of relativistic black hole jets that govern accreting black hole systems of all sizes, from those arising from neutron star mergers, to those residing at the centers of galaxies. We will elucidate the role of a spinning black hole's geometry, and large reservoir of rotational energy, in powering jets, both in stationary and dynamical scenarios. This will involve bridging the divide between different descriptions of the plasma dynamics to include the effects of both the black hole spacetime, as well as particle effects like acceleration and heating. My team and I will also explore how this new window into extreme gravity can be used to look for new fundamental physics, such as the origin of dark matter. We will determine how gravitational wave observations can be used to probe the existence of new particles through superradiance, a process which causes black holes to form clouds of ultralight bosons at the expense of their rotational energy. We will also study how neutron stars could be converted into black holes in some models of dark matter, and understanding the observational signatures. This research will provide students with the chance to participate in a rapidly growing field, gaining fluency in a number of topics including astrophysics, gravity, particle physics, and computational physics. They will develop skills in advanced mathematics, software development, and high-performance computing that are increasingly in demand both in academia and areas of technology like data science.

随着LIGO/Virgo最近对黑洞和中子星合并产生的引力波的惊人观测，我们已经进入了多信使天文学的新时代。种种迹象表明，随着引力波探测器的数量和灵敏度在未来几年的增加，将会有大量的观测结果，揭示出只有在引力波中才能看到的宇宙的新方面。然而，最大限度地提高这些观测的回报，并利用它们作为基础物理学的新探索，将需要我们在这一领域对引力的理论理解取得进展。 该提案的核心部分是研究中子星星合并-宇宙中致密恒星的剧烈碰撞-最终目标是了解引力波信号和伴随的电磁瞬变，以帮助定位和解释当前和未来的观测。作为实现这一长期目标的一部分，我和我的团队将研究这些系统中仍然知之甚少的几个方面，包括中子星星自旋和轨道偏心率的影响，以及合并后残余物和吸积盘的动力学，并确定它们如何揭示最高密度下核物质的行为，宇宙中最重元素的起源以及其他问题。我和我的团队将研究相对论性黑洞喷流的基本机制，这些喷流控制着各种大小的吸积黑洞系统，从中子星星合并产生的黑洞到星系中心的黑洞。我们将阐明一个旋转黑洞的几何形状的作用，和旋转能量的大水库，在供电喷流，无论是在静态和动态的情况。这将涉及弥合等离子体动力学的不同描述之间的鸿沟，以包括黑洞时空的影响以及加速和加热等粒子效应。我和我的团队还将探索如何利用这扇通往极端引力的新窗口来寻找新的基础物理学，比如暗物质的起源。我们将确定引力波观测如何通过超辐射来探测新粒子的存在，超辐射是一个导致黑洞以牺牲旋转能量为代价形成超轻玻色子云的过程。我们还将研究中子星如何在某些暗物质模型中转化为黑洞，并了解观测特征。 这项研究将为学生提供参与一个快速发展的领域的机会，在包括天体物理学，重力，粒子物理学和计算物理学在内的许多主题中获得流畅性。他们将培养高等数学，软件开发和高性能计算方面的技能，这些技能在学术界和数据科学等技术领域的需求越来越大。