WoU-MMA: Collaborative Research: Supermassive Binary Black Holes: Accretion Dynamics and Electromagnetic Output

超大质量黑洞（SMBH）合并是宇宙中最引人注目的现象之一。 在几个小时内，它们可以在引力波中发出与宇宙中所有恒星产生的光一样多的能量。 然而，目前还没有人被发现，部分原因是没有人知道他们应该发出什么样的光沿着引力波。 该项目将SMBH双星的天体物理学知识与气体流动的详细物理模拟和随时间变化的时空的显式计算相结合，以预测观测者应该寻找的光。 初级研究人员将学习这个新领域和超大规模计算，加强技术人员队伍。PI的辅助努力增强了他们每个大学的教学计划，并有助于公共宣传。这个小组已经建立了进行这些预测所需的知识库和计算方法，包括建立一个多补丁模拟基础设施来计算不断变化的时空，并允许单独处理子区域。 代码库包括后处理工具，将流体模拟数据转换为光子辐射的预测，占主要辐射机制，不透明度和光子传播通过动态时空。 这项研究从合并前的状态开始，以了解其物理机制，并准备实际的初始数据。 第二步将计算物质在合并和随后的弛豫阶段的行为。 后处理机器然后预测EM光谱和光变曲线。 该项目推进了NSF宇宙大创意窗口的目标。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。

Supermassive black hole (SMBH) mergers are one of the most dramatic phenomena in the Universe. For a few hours, they can emit as much power in gravitational waves as all the stars in the Universe produce in light. However, none has yet been caught in the act, partly because no one knows what sort of light they should emit along with the gravitational waves. This project combines astrophysical knowledge of SMBH binaries with detailed physical simulation of gas flows and explicit computation of time-dependent spacetimes, to predict the light observers should search for. Junior researchers will learn about this new field and about very large-scale computation, strengthening the technical workforce. Ancillary efforts by the PIs enhance the teaching program at each of their universities and contribute to public outreach.This group has built the knowledge base and computational methods needed to make these predictions, including building a multi-patch simulation infrastructure to compute the changing spacetime and permit separate treatment of subregions. The code base includes post-processing tools that transform fluid simulation data into predictions of photon radiation, accounting for the principal radiation mechanisms, opacities, and photon propagation through dynamical spacetimes. This study starts at the immediate pre-merger state, to understand its physical mechanisms and to prepare realistic initial data. The second step will compute how matter behaves during the merger proper and the subsequent relaxation phase. The post-processing machinery then predicts EM spectra and light curves. This project advances the goals of the NSF Windows on the Universe Big Idea.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.