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 PO6: Compression and Burn III
2:00 PM–4:48 PM,
Wednesday, November 7, 2018
OCC
Room: B115-116
Chair: Hans Rinderknecht, University of Rochester
Abstract ID: BAPS.2018.DPP.PO6.2
Abstract: PO6.00002 : Nuclear and x-ray burn widths in recent high-yield implosions on the National Ignition Facility*
2:12 PM–2:24 PM
Presenter:
Gerald Williams
(Lawrence Livermore Natl Lab)
Authors:
Gerald Williams
(Lawrence Livermore Natl Lab)
Tammy Yee Wing Ma
(Lawrence Livermore Natl Lab)
Pravesh K Patel
(Lawrence Livermore Natl Lab)
Shahab Khan
(Lawrence Livermore Natl Lab)
Michael K Kruse
(Lawrence Livermore Natl Lab)
Hans Herrmann
(Los Alamos Natl Lab)
Kevin Meaney
(Los Alamos Natl Lab)
Hermann Geppert-Kleinrath
(Los Alamos Natl Lab)
Yongho Kim
(Los Alamos Natl Lab)
Daniel T Casey
(Lawrence Livermore Natl Lab)
Cliff A Thomas
(Lawrence Livermore Natl Lab)
Kevin L Baker
(Lawrence Livermore Natl Lab)
Brian K. Spears
(Lawrence Livermore Natl Lab)
Matthias Hohenberger
(Lawrence Livermore Natl Lab)
Christopher Weber
(Lawrence Livermore Natl Lab)
Ryan Nora
(Lawrence Livermore Natl Lab)
Sebastien Le Pape
(Lawrence Livermore Natl Lab)
Laura Berzak Hopkins
(Lawrence Livermore Natl Lab)
Laurent Divol
(Lawrence Livermore Natl Lab)
Arthur Pak
(Lawrence Livermore Natl Lab)
Eduard L. Dewald
(Lawrence Livermore Natl Lab)
Laura Robin Benedetti
(Lawrence Livermore Natl Lab)
Daniel Clark
(Lawrence Livermore Natl Lab)
Cryogenic implosions on the National Ignition Facility (NIF) are primarily used to produce high neutron yields in the effort to achieve the goal of ignition. Two campaigns using high-density carbon ablator designs are leading this effort using low- and high-adiabat implosions that have achieved yields of more than 50 kJ, the highest to date on NIF. The time-history of the DT neutrons and x-rays emitted during the implosion with ~10-20 ps temporal resolution in the form of MeV photons (gammas) released from fusion events and 10s of keV x-ray photons from the hot dense core. These burn durations are typically longer than predicted by simulations and could be a signature of degradation mechanisms like preheat, fuel-ablator mix, or 3D effects. We also observe a second x-ray peak post-stagnation at lower photon energies, which we attribute to the outgoing shock propagating through the ablator. We discuss how this signature can provide insight into the conditions of the shell at late time.
*This work was performed under the auspices of the U.S. DOE by LLNL under Contract DE-AC52-07NA27344. LLNL-ABS-753495
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.PO6.2
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