Exploring Strong-Field Gravity through Gravitational-Wave and Multimessenger Observations

通过引力波和多信使观测探索强场引力

• 批准号: 2207349
• 负责人: Kento Yagi
• 金额: $ 6万
• 依托单位: University of Virginia Main Campus
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2022
• 资助国家: 美国
• 起止时间: 2022-09-01 至 2024-08-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=2207349&HistoricalAwards=false
• 关键词: Exploring; Strong; Field; Gravity; through

The overarching goal of this project is to reveal how well one can ultimately probe the nature of strong, dynamical, and nonlinear gravity through gravitational-wave observations of black holes and multimessenger observations of neutron stars. Currently, one of the biggest challenges in testing General Relativity with gravitational waves from binary black hole coalescences is the lack of complete gravitational waveforms from theories beyond General Relativity that are valid throughout the inspiral, merger, and ringdown of the binary evolution. Moreover, for binary neutron stars, certain tests of General Relativity are limited by uncertainties in nuclear matter properties. The PI will tackle these problems by (I) constructing, for the first time, gravitational waveforms in theories beyond General Relativity that are valid in all of the inspiral-merger-ringdown phases, and (II) performing a comprehensive study of multimessenger tests of General Relativity with neutron star observations by avoiding uncertainties in nuclear physics. The gravitational waveform models to be developed will be ready to use and can be widely adopted by the gravitational wave community and beyond. Multimessenger tests of General Relativity with neutron star observations are extremely timely, and the outcome of both projects will impact various communities in physics and beyond, including gravitational physics, particle physics, nuclear physics, and astrophysics. The long-term educational goal of the project is to connect, globally, potential next-generation scientists and convey the beauty and excitement of physics, in particular General Relativity. For the construction of the complete gravitational waveforms, the PI will work in a specific gravitational theory motivated by string theory, in which some simulations are already available. The PI and collaborators will produce more simulation data for the merger-ringdown and will stitch them against analytic waveforms during the inspiral. These complete waveforms allow one to probe more precisely theories beyond General Relativity with the existing gravitational wave events and will assist in searches for new physics with future observations. For multi-messenger tests, the PI will employ universal relations among certain neutron star observables that do not depend sensitively on the unknown internal structure of neutron stars. The PI will study such relations in a few theories beyond General Relativity that either introduce additional scalar/vector fields or introduce modifications in the high curvature regime. The PI will then study how well one can probe these theories through current and future multimessenger observations. To achieve the educational goal, the PI's team will develop an online game on General Relativity and gravitational waves to reach out to young players across the world. In the game instructions, the PI will provide a brief description of General Relativity, black holes, and gravitational waves, conveying the excitement and key aspects of recent Nobel-prize winning physics. Some students will be involved in the game development, integrating the research and educational activities. The PI will make the source codes publicly available so that anyone can develop their own games.This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.

该项目的总体目标是揭示通过对黑洞的引力波观测和对中子星的多信使观测，最终能够如何很好地探测强、动态和非线性引力的本质。目前，用双星黑洞聚结产生的引力波测试广义相对论的最大挑战之一是，缺乏广义相对论之外的理论中完整的引力波形，这些波形在双星演化的整个吸气、合并和振铃过程中都有效。此外，对于双中子星，广义相对论的某些测试受到核物质性质的不确定性的限制。 PI 将通过以下方式解决这些问题：(I) 首次在超越广义相对论的理论中构建在所有吸气-合并-衰荡阶段都有效的引力波形，以及 (II) 对多信使测试进行全面研究广义相对论通过中子星观测避免了核物理中的不确定性。待开发的引力波形模型将可供使用，并可被引力波界及其他领域广泛采用。广义相对论与中子星观测的多信使测试非常及时，这两个项目的结果将影响物理学界及其他领域的各个领域，包括引力物理学、粒子物理学、核物理学和天体物理学。该项目的长期教育目标是在全球范围内连接潜在的下一代科学家，并传达物理学（特别是广义相对论）的美丽和兴奋。为了构建完整的引力波形，PI 将在由弦理论驱动的特定引力理论中工作，其中一些模拟已经可用。 PI 和合作者将为合并振铃生成更多模拟数据，并将它们与吸气期间的分析波形进行拼接。这些完整的波形使人们能够利用现有的引力波事件更精确地探索广义相对论之外的理论，并将有助于通过未来的观测来寻找新的物理学。对于多信使测试，PI 将采用某些中子星可观测值之间的普遍关系，这些关系不敏感地依赖于中子星的未知内部结构。 PI 将研究广义相对论之外的一些理论中的此类关系，这些理论要么引入额外的标量/矢量场，要么引入高曲率机制的修改。然后，PI 将研究人们如何通过当前和未来的多信使观察来探索这些理论。为了实现教育目标，PI 的团队将开发一款关于广义相对论和引力波的在线游戏，以吸引世界各地的年轻玩家。在游戏说明中，PI 将简要描述广义相对论、黑洞和引力波，传达近期诺贝尔物理学奖的精彩内容和关键方面。一些学生将参与游戏开发，将研究和教育活动结合起来。 PI 将公开源代码，以便任何人都可以开发自己的游戏。该奖项反映了 NSF 的法定使命，并通过使用基金会的智力价值和更广泛的影响审查标准进行评估，被认为值得支持。

项目成果

Breaking bad degeneracies with Love relations: Improving gravitational-wave measurements through universal relations

用爱情关系打破不良简并：通过普遍关系改进引力波测量

• DOI: 10.1103/physrevd.107.043010
• 发表时间: 2023
• 期刊: Physical Review D
• 影响因子: 5
• 作者: Xie, Yiqi;Chatterjee, Deep;Holder, Gilbert;Holz, Daniel E.;Perkins, Scott;Yagi, Kent;Yunes, Nicolás
• 通讯作者: Yunes, Nicolás