CosmoFlow: Using Deep Learning to Learn the Universe at Scale
CosmoFlow: Using Deep Learning to Learn the Universe at Scale
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DOI:
10.1109/sc.2018.00068
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发表时间:
2018-08
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通讯作者:
Amrita Mathuriya;D. Bard;P. Mendygral;Lawrence Meadows;James A. Arnemann;Lei Shao;Siyu He;Tuomas Kärnä;Diana Moise;S. Pennycook;K. Maschhoff;J. Sewall;Nalini Kumar;S. Ho;Michael F. Ringenburg;P. Prabhat;Victor W. Lee
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作者:
Amrita Mathuriya;D. Bard;P. Mendygral;Lawrence Meadows;James A. Arnemann;Lei Shao;Siyu He;Tuomas Kärnä;Diana Moise;S. Pennycook;K. Maschhoff;J. Sewall;Nalini Kumar;S. Ho;Michael F. Ringenburg;P. Prabhat;Victor W. Lee
Deep learning is a promising tool to determine the physical model that describes our universe. To handle the considerable computational cost of this problem, we present CosmoFlow: a highly scalable deep learning application built on top of the TensorFlow framework. CosmoFlow uses efficient implementations of 3D convolution and pooling primitives, together with improvements in threading for many element-wise operations, to improve training performance on Intel® Xeon Phi™ processors. We also utilize the Cray PE Machine Learning Plugin for efficient scaling to multiple nodes. We demonstrate fully synchronous data-parallel training on 8192 nodes of Cori with 77% parallel efficiency, achieving 3.5 Pflop/s sustained performance. To our knowledge, this is the first large-scale science application of the TensorFlow framework at supercomputer scale with fully-synchronous training. These enhancements enable us to process large 3D dark matter distribution and predict the cosmological parameters ΩsubM/sub, σsub8/sub and nsubs/sub with unprecedented accuracy.