Key advancements toward eliminating the “drive deficit” in ICF hohlraum simulations
Hui Chen, D. T. Woods, W. A. Farmer, N. Aybar, D. A. Liedahl, S. A. MacLaren, M. B. Schneider, H. A. Scott, J. A. Harte, D. E. Hinkel, O. L. Landen, J. D. Moody, M. D. Rosen, J. S. Ross, S. Rogers, N. Roskopf, G. F. Swadling, S. Vonhof, G. B. Zimmerman
Abstract
This paper, extended from a Letter [Chen et al., Phys. Rev. E 110, L013201 (2024)] published in Phys. Rev. E in 2024, presents detailed results from a set of experiments studying the x-ray drive produced in laser-heated ignition-scale hohlraums at the National Ignition Facility. The results reveal that deficiencies in non-local thermodynamic equilibrium atomics physics calculations of gold emissivity lead to the overestimation of the “M-band” radiation and are responsible for discrepancies in drive predictions vs measurements in these hohlraums. These experiments were performed on ViewFactor targets with the same gas fill and laser pulse shapes as currently used in ongoing ignition experiments. The common hohlraum model with a magnetohydrodynamics heat transport model and a 10%–20% reduction to the M-band absorption and emission opacity can bring the simulations into agreement with several independent measurements, including the absolute radiation flux, the radiation flux in the 2–4 keV spectral range, and spectroscopic measurements of both K-shell dopant and L-shell gold. This new model is applicable to ICF and high-energy density experiments that use gold hohlraums as drivers.