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 UO4: Direct and Indirect Drive
2:00 PM–4:36 PM,
Thursday, November 8, 2018
OCC
Room: B110-112
Chair: Laurent Masse, Lawrence Livermore National Laboratory
Abstract ID: BAPS.2018.DPP.UO4.13
Abstract: UO4.00013 : Signatures of Laser Imprint in OMEGA Cryogenic Implosions*
4:24 PM–4:36 PM
Presenter:
Radha Bahukutumbi
(Laboratory for Laser Energetics)
Authors:
Radha Bahukutumbi
(Laboratory for Laser Energetics)
Kenneth Anderson
(Laboratory for Laser Energetics)
Ricccardo Betti
(Lab for Laser Energetics)
Edward Campbell
(Laboratory for Laser Energetics)
Duc M Cao
(Lab for Laser Energetics)
Timothy J Collins
(Univ of Rochester)
Timothy J Collins
(Univ of Rochester)
Chad Forrest
(Lab for Laser Energetics)
Suxing Hu
(Univ of Rochester)
James P Knauer
(Univ of Rochester)
John A Marozas
(Univ of Rochester)
Vladimir Glebov
(Lab for Laser Energetics)
Valeri N Goncharov
(Univ of Rochester)
Sean P Regan
(Univ of Rochester)
Thomas C Sangster
(Univ of Rochester)
Rahul C Shah
(Lab for Laser Energetics)
A. Shvydky
(Laboratory for Laser Energetics)
Christian Stoeckl
(Univ of Rochester)
Johan Frenje
(Massachusetts Inst of Tech-MIT)
Maria Gatu Johnson
(Massachusetts Inst of Tech-MIT)
Richard David Petrasso
(Massachusetts Inst of Tech-MIT)
The growth of single-beam nonuniformity or laser imprint can compromise target performance in direct-drive implosions. With increasing in-flight aspect ratio (IFAR is the ratio of the shell radius to shell thickness), the imprint front can penetrate through the shell, reducing the in-flight shell density. This results in a less-efficient piston for assembling the hot spot. The role of laser imprint on target performance is discussed in this presentation. Simulations of OMEGA cryogenic implosions with varying IFAR are presented. These DRACO simulations include a 3-D ray trace with the effect of cross-beam energy transfer, nonlocal heat conduction, and calculated first‑principles equations of state and opacities of the ablator and ice. Observables including ablation-surface trajectories, neutron yields, areal densities, neutron rates, ion temperatures, and hot-spot images are compared to experiment. Specific signatures including broadened neutron rates, reduced areal densities, and thicker shells relative to spherically symmetric simulations are presented.Â
*This material is based upon work supported by the Department of Energy National Nuclear Security Administration under Award Number DE-NA0001944.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.UO4.13
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