Deep learning for NLTE spectral opacities

• Published in: Physics of plasmas 2020-05, Vol.27 (5)
• Main Authors: Kluth, G., Humbird, K. D., Spears, B. K., Peterson, J. L., Scott, H. A., Patel, M. V., Koning, J., Marinak, M., Divol, L., Young, C. V.
• Format: Article
• Language: English
• Subjects: Acceleration; Artificial neural networks; Atomic physics; Computational efficiency; Computational fluid dynamics; Computer simulation; Computing time; Deep learning; Fluid flow; Flux density; Hydrodynamics; Inertial confinement fusion; Local thermodynamic equilibrium; Machine learning; Mathematical analysis; Neural networks; Nuclear reactions; Packages; Physics; Plasma interactions; Plasma physics; Plasmas (physics); Radiation transport; Supercomputers
• ISSN: 1070-664X; 1089-7674
• DOI: 10.1063/5.0006784

Computer simulations of high energy density science experiments are computationally challenging, consisting of multiple physics calculations including radiation transport, hydrodynamics, atomic physics, nuclear reactions, laser–plasma interactions, and more. To simulate inertial confinement fusion (ICF) experiments at high fidelity, each of these physics calculations should be as detailed as possible. However, this quickly becomes too computationally expensive even for modern supercomputers, and thus many simplifying assumptions are made to reduce the required computational time. Much of the research has focused on acceleration techniques for the various packages in multiphysics codes. In this work, we explore a novel method for accelerating physics packages via machine learning. The non-local thermodynamic equilibrium (NLTE) package is one of the most expensive calculations in the simulations of indirect drive inertial confinement fusion, taking several tens of percent of the total wall clock time. We explore the use of machine learning to accelerate this package, by essentially replacing the physics calculation with a deep neural network that has been trained to emulate the physics code. We demonstrate the feasibility of this approach on a simple problem and perform a side-by-side comparison of the physics calculation and the neural network inline in an ICF Hohlraum simulation. We show that the neural network achieves a 10× speed up in NLTE computational time while achieving good agreement with the physics code for several quantities of interest.