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arXiv 2312.01005astro-ph.GAcs.LGeess.IV
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使用GAN生成M87*黑洞图像

Generating Images of the M87* Black Hole Using GANs

Harvard University(哈佛大学);Carnegie Mellon University(卡内基梅隆大学);Center for Astrophysics | Harvard & Smithsonian(哈佛-史密森天体物理中心);Universität Würzburg(维尔茨堡大学);Goethe Universität(歌德大学);Max-Planck-Institut für Radioastronomie(马克斯·普朗克射电天文学研究所)
Arya Mohan, Pavlos Protopapas, Keerthi Kunnumkai, Cecilia Garraffo, Lindy Blackburn, Koushik Chatterjee, Sheperd S. Doeleman, Razieh Emami, Christian M. Fromm, … 展开作者

Arya Mohan, Pavlos Protopapas, Keerthi Kunnumkai, Cecilia Garraffo, Lindy Blackburn, Koushik Chatterjee, Sheperd S. Doeleman, Razieh Emami, Christian M. Fromm, Yosuke Mizuno, Angelo Ricarte

AI总结:

本文提出基于条件渐进式GAN的黑洞图像生成方法,可覆盖任意自旋和电子温度分布,实验证明其增强数据能显著提升黑洞参数估计性能。

摘要:

本文提出一种基于条件渐进式生成对抗网络(CPGAN)的新型数据增强方法,用于生成多样化的黑洞(BH)图像,并考虑自旋和电子温度分布的变化。这些生成的图像是训练深度学习算法从观测数据中准确估计黑洞参数的宝贵资源。给定电子温度分布,我们的模型可以生成自旋值在[-1, 1]范围内任意取值的黑洞图像。为验证方法的有效性,我们使用卷积神经网络分别基于GRMHD图像和所提模型生成的图像来预测黑洞自旋。结果表明,使用增强数据集进行训练、并使用GRMHD模拟数据进行测试时,性能显著提升,表现为较高的R2分数。因此,我们认为GAN可以作为低成本的黑洞图像生成模型,并可靠地增强其他参数化算法的训练数据集。

英文摘要:

In this paper, we introduce a novel data augmentation methodology based on Conditional Progressive Generative Adversarial Networks (CPGAN) to generate diverse black hole (BH) images, accounting for variations in spin and electron temperature prescriptions. These generated images are valuable resources for training deep learning algorithms to accurately estimate black hole parameters from observational data. Our model can generate BH images for any spin value within the range of [-1, 1], given an electron temperature distribution. To validate the effectiveness of our approach, we employ a convolutional neural network to predict the BH spin using both the GRMHD images and the images generated by our proposed model. Our results demonstrate a significant performance improvement when training is conducted with the augmented dataset while testing is performed using GRMHD simulated data, as indicated by the high R2 score. Consequently, we propose that GANs can be employed as cost effective models for black hole image generation and reliably augment training datasets for other parameterization algorithms.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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