Generating images of the M87* black hole using GANs

Author:

Mohan Arya1ORCID,Protopapas Pavlos2,Kunnumkai Keerthi3,Garraffo Cecilia4,Blackburn Lindy56,Chatterjee Koushik56ORCID,Doeleman Sheperd S56,Emami Razieh6,Fromm Christian M789,Mizuno Yosuke101112ORCID,Ricarte Angelo56

Affiliation:

1. Univ.AI , Singapore , 050531

2. John A. Paulson School of Engineering and Applied Science, Harvard University , Cambridge, MA 02138 , USA

3. Department of Physics, Carnegie Mellon University , Pittsburgh, PA 15213 , USA

4. AstroAI at the Center for Astrophysics | Harvard & Smithsonian , 60 Garden St, Cambridge, MA 02138 , USA

5. Black Hole Initiative at Harvard University , 20 Garden St, Cambridge, MA 02138 , USA

6. Center for Astrophysics | Harvard & Smithsonian , 60 Garden St, Cambridge, MA 02138 , USA

7. Institut für Theoretische Physik, Goethe-Universität, Max-von-Laue-Strasse 1, 60438 Frankfurt, Germany

8. Institut für Theoretische Physik und Astrophysik, Universität Würzburg, Emil-Fischer-Strasse 31, 97074 Würzburg, Germany , D-60438 Frankfurt , Germany

9. Max-Planck-Institut für Radioastronomie , Auf dem Hügel 69, D-53121 Bonn , Germany

10. Tsung-Dao Lee Institute, Shanghai Jiao-Tong University , Shanghai, 520 Shengrong Road, 201210 , P. R. China

11. School of Physics & Astronomy, Shanghai Jiao-Tong University , Shanghai, 800 Dongchuan Road, 200240 , P. R. China

12. Institut für Theoretische Physik, Goethe Universität , Max-von-Laue-Str. 1, D-60438 Frankfurt am Main , Germany

Abstract

ABSTRACT 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 data set 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 data sets for other parametrization algorithms.

Funder

DFG

National Natural Science Foundation of China

NSF

Gordon and Betty Moore Foundation

John Templeton Foundation

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 1 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Most frequent value analysis of distance measurements to M87;Monthly Notices of the Royal Astronomical Society;2024-08-14

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