WoU-MMA: Research in Black Hole Physics and Relativistic Astrophysics

WoU-MMA：黑洞物理学和相对论天体物理学研究

• 批准号: 2308615
• 负责人: Saul Teukolsky
• 金额: $ 60万
• 依托单位: Cornell University
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2023
• 资助国家: 美国
• 起止时间: 2023-07-01 至 2026-06-30
• 项目状态: 未结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=2308615&HistoricalAwards=false
• 关键词: WoU; MMA; Research; Black; Hole

This award supports research in relativity and relativistic astrophysics, and it addresses the priority areas of NSF's "Windows on the Universe" Big Idea. A large component of the research is aimed at the numerical solution of Einstein's equations by supercomputer simulations. The research will have a broad impact on our understanding of fundamental physics. The first real tests of general relativity in the strong field regime of black holes are just beginning to occur with experiments like LIGO. To confront theory with observation, one must be able to calculate what the theory predicts. Are the black holes that LIGO observes the black holes predicted by Einstein's theory? The research will have an impact on astronomy. Mergers of binary systems containing neutron stars can lead to the emission of electromagnetic and neutrino signals, as well as gravitational waves. As more of these events are seen, better simulations are needed to help determine the properties of the sources. The research will also have an impact on the broader area of computational science. The computational techniques to be developed here can be used to solve problems in many other areas, including fluid dynamics, meteorology, seismology, and astrophysics. Young researchers trained in these techniques are in great demand. Relativity and black holes continue to fascinate the public and allow science to be communicated broadly. Movies of simulations produced by the investigators will continue to provide public outreach.To solve Einstein's equations, the investigators will use high-accuracy computational techniques suited to the mathematical properties of the equations. These methods solve the equations at a much smaller computational cost than other techniques. The investigators will include ever more realistic descriptions of the microphysics in the simulations, such as the equation of state of nuclear matter, neutrino effects, and magnetic fields. The investigators will also develop a new code for computational astrophysics that is designed to take advantage of upcoming exascale machines in a way that current codes cannot. This new code will be based on discontinuous Galerkin methods and task-based parallelism. It will provide transformative capabilities not only for numerical relativity, but for many problems in computational astrophysics.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.

该奖项支持相对论和相对论天体物理学的研究，并解决了NSF“宇宙之窗”大理念的优先领域。这项研究的一个重要组成部分是通过超级计算机模拟爱因斯坦方程的数值解。 这项研究将对我们对基础物理学的理解产生广泛的影响。在黑洞的强场区域中，对广义相对论的第一次真实的检验才刚刚开始，就像LIGO这样的实验。为了使理论与观察相对抗，人们必须能够计算出理论所预测的东西。LIGO观测到的黑洞是爱因斯坦理论预测的黑洞吗？ 这项研究将对天文学产生影响。 包含中子星的双星系统的合并可以导致电磁和中微子信号的发射，以及引力波。 随着这些事件越来越多，需要更好的模拟来帮助确定源的属性。 这项研究也将对更广泛的计算科学领域产生影响。这里发展的计算技术可以用来解决许多其他领域的问题，包括流体动力学、气象学、地震学和天体物理学。对受过这些技术培训的年轻研究人员的需求很大。 相对论和黑洞继续吸引着公众，并使科学得到广泛传播。研究人员制作的模拟电影将继续提供公共宣传。为了求解爱因斯坦方程，研究人员将使用适合方程数学性质的高精度计算技术。这些方法以比其他技术小得多的计算成本求解方程。研究人员将在模拟中包括对微观物理的更真实的描述，例如核物质的状态方程，中微子效应和磁场。研究人员还将为计算天体物理学开发一种新的代码，旨在以当前代码无法利用的方式利用即将到来的exascale机器。 这个新的代码将基于不连续Galerkin方法和基于任务的并行性。该奖项反映了NSF的法定使命，并通过使用基金会的知识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

Eccentric binary black holes: Comparing numerical relativity and small mass-ratio perturbation theory

• DOI: 10.1103/physrevd.106.124040
• 发表时间: 2022-09
• 期刊: Physical Review D
• 影响因子: 5
• 作者: A. Ramos-Buades;Maarten van de Meent;H. Pfeiffer;H. Rüter;M. Scheel;M. Boyle;Lawrence E. Kidder

Numerical simulations of black hole-neutron star mergers in scalar-tensor gravity

• DOI: 10.1103/physrevd.107.124051
• 发表时间: 2023-04
• 期刊: Physical Review D
• 影响因子: 5
• 作者: Sizheng Ma;V. Varma;L. Stein;F. Foucart;Matthew D. Duez;Lawrence E. Kidder;H. Pfeiffer;M. Scheel

High-accuracy numerical models of Brownian thermal noise in thin mirror coatings

薄镜涂层中布朗热噪声的高精度数值模型

• DOI: 10.1088/1361-6382/acad62
• 发表时间: 2023
• 期刊: Classical and Quantum Gravity
• 影响因子: 3.5
• 作者: Vu, Nils L.;Rodriguez, Samuel;Włodarczyk, Tom;Lovelace, Geoffrey;P Pfeiffer, Harald;S Bonilla, Gabriel;Deppe, Nils;Hébert, François;E Kidder, Lawrence;Moxon, Jordan
• 通讯作者: Moxon, Jordan

Surrogate model for gravitational wave signals from nonspinning, comparable-to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity

• DOI: 10.1103/physrevd.106.104025
• 发表时间: 2022-04
• 期刊: Physical Review D
• 影响因子: 5
• 作者: Tousif Islam;Scott E. Field;S. Hughes;G. Khanna;V. Varma;M. Giesler;M. Scheel;Lawrence E. Kidder;H. Pfeiffer

Simulating neutron stars with a flexible enthalpy-based equation of state parametrization in spectre

• DOI: 10.1103/physrevd.107.123017
• 发表时间: 2023-01
• 期刊: Physical Review D
• 影响因子: 5
• 作者: I. Legred;Yoonsoo Kim;N. Deppe;K. Chatziioannou;F. Foucart;F. H'ebert;Lawrence E. Kidder