Physics-inspired spatiotemporal-graph AI ensemble for the detection of higher order wave mode signals of spinning binary black hole mergers

Minyang Tian, Eliu Huerta, Huihuo Zheng, Prayush Kumar
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Abstract

We present a new class of AI models for the detection of quasi-circular, spinning, non-precessing binary black hole mergers whose waveforms include the higher order gravitational wave modes $(\ell, |m|)=\{(2, 2), (2, 1), (3, 3), (3, 2), (4, 4)\}$, and mode mixing effects in the \(\ell = 3, |m| = 2\) harmonics. These AI models combine hybrid dilated convolution neural networks to accurately model both short- and long-range temporal sequential information of gravitational waves; and graph neural networks to capture spatial correlations among gravitational wave observatories to consistently describe and identify the presence of a signal in a three detector network encompassing the Advanced LIGO and Virgo detectors. We first trained these spatiotemporal-graph AI models using synthetic noise, using 1.2 million modeled waveforms to densely sample this signal manifold, within 1.7 hours using 256 NVIDIA A100 GPUs in the Polaris supercomputer at the Argonne Leadership Computing Facility. This distributed training approach exhibited optimal classification performance, and strong scaling up to 512 NVIDIA A100 GPUs. With these AI ensembles we processed data from a three detector network, and found that an ensemble of 4 AI models achieves state-of-the-art performance for signal detection, and reports two misclassifications for every decade of searched data. We distributed AI inference over 128 GPUs in the Polaris supercomputer and 128 nodes in the Theta supercomputer, and completed the processing of a decade of gravitational wave data from a three detector network within 3.5 hours. Finally, we fine-tuned these AI ensembles to process the entire month of February 2020, which is part of the O3b LIGO/Virgo observation run, and found 6 gravitational waves, concurrently identified in Advanced LIGO and Advanced Virgo data, and zero false positives. This analysis was completed in one hour using one NVIDIA A100 GPU.
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受物理学启发的用于探测旋转双黑洞合并的高阶波模信号的时空图人工智能组合
我们提出了一类新的人工智能模型,用于探测准圆的、旋转的、非前处理的双黑洞合并,其波形包括高阶引力波模式$(\ell, |m|)=\{(2, 2), (2, 1), (3, 3), (3, 2), (4, 4)\}$,以及\(\ell = 3, |m| = 2\) 谐波中的模式混合效应。这些人工智能模型结合了混合扩张卷积神经网络,以准确模拟引力波的短程和长程时间序列信息;以及图神经网络,以捕捉引力波观测站之间的空间相关性,从而在包括高级 LIGO 和室女座探测器在内的三个探测器网络中一致地描述和识别信号的存在。我们首先使用合成噪声对这些时空图人工智能模型进行了训练,使用阿贡领导计算设施北极星超级计算机中的 256 个英伟达 A100 GPU,在 1.7 小时内使用 120 万个建模波形对信号流形进行了密集采样。这种分布式训练方法表现出最佳的分类性能,并可扩展到 512 个英伟达 A100 GPU。利用这些人工智能模型集,我们处理了来自三个探测器网络的数据,发现由 4 个人工智能模型组成的模型集在信号检测方面达到了最先进的性能,并且每搜索十年数据就会报告两次误分类。我们将人工智能推理分布在北极星超级计算机的 128 个 GPU 和 Theta 超级计算机的 128 个节点上,并在 3.5 小时内完成了对来自三个探测器网络的十年引力波数据的处理。最后,我们对这些人工智能集合进行了微调,以处理 2020 年 2 月(O3b LIGO/Virgo 观测运行的一部分)的整个月份,并在高级 LIGO 和高级 Virgo 数据中同时发现了 6 个引力波,误报率为零。该分析使用一个英伟达 A100 GPU 在一小时内完成。
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