Bulletin of the American Physical Society
60th Annual Meeting of the APS Division of Plasma Physics
Volume 63, Number 11
Monday–Friday, November 5–9, 2018; Portland, Oregon
Session GP11: Poster Session III: Basic Plasma Physics: General; Space and Astrophysical Plasmas; ICF Measurement and Computational Techniques, Direct and Indirect Drive; MIF Science and Technology (9:30am-12:30pm)
Tuesday, November 6, 2018
OCC
Room: Exhibit Hall A1&A
Abstract ID: BAPS.2018.DPP.GP11.106
Abstract: GP11.00106 : Super-configuration-accounting opacity of CH and its applications*
Presenter:
Teck Lee
(U.S. Naval Research Lab)
Authors:
Teck Lee
(U.S. Naval Research Lab)
Michel P Busquet
(Research Support Instruments, Lanham, MD 20706, USA)
Marcel Klapisch
(Syntek Technologies, Arlington, VA, 22203, USA)
Jason Wilson Bates
(U.S. Naval Research Lab)
Andrew J Schmitt
(U.S. Naval Research Lab)
John L Giuliani
(U.S. Naval Research Lab)
Polystyrene CH is an essential material in inertial-confinement-fusion (ICF) target designs [1]. Based on super transition arrays (STA) calculations [2], we generate a wide range polyethylene (CH) opacity table of density ρ= 1.0 × 10-6 to ρ = 500 g/cm3 and temperature T = 0.015 to 2.5 keV. Contrasting the STA calculated opacities to the results obtained using the first principle quantum molecular dynamics (QMD) code developed at the Laboratory for Laser Energetic of University of Rochester and the ATOMIC code from Los Alamos National Laboratory [3], we find that the STA results are in reasonable agreement with the data from QMD and ATOMIC codes down to plasma temperature of about 20 eV where comparisons are possible. Additionally, we present samples of assessment on the reliability of the present CH dataset through a radiation hydrodynamic simulation.
[1] D.T. Michel, V.N. Goncharov, I.V. Igumenshchev, R. Epstein and D.H. Froula, Phys. Rev. Lett. 111, 245005 (2013).
[2] A. Bar-Shalom, J. Oreg, W. H. Goldstein, D. Shvarts, and A. Zigler, Phys. Rev. A, 40, 3183, (1989).
[3] S.X. Hu et al., Phys. Rev. B., 96, 144203 (2017)
**This work is made possible by a financial support from DOE/NNSA.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.GP11.106
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