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 PO4: Hydrodynamic Instability
2:00 PM–5:00 PM,
Wednesday, November 7, 2018
OCC
Room: B110-112
Chair: Elizabeth Merritt, Los Alamos National Laboratory
Abstract ID: BAPS.2018.DPP.PO4.15
Abstract: PO4.00015 : Simulations of Gas-Ablator Mix in Symcap Implosions at the National Ignition Facility*
(Author Not Attending)
Presenter:
Jesse Pino
(Lawrence Livermore Natl Lab)
Authors:
Jesse Pino
(Lawrence Livermore Natl Lab)
Eduard L. Dewald
(Lawrence Livermore Natl Lab)
Jeff Greenough
(Lawrence Livermore Natl Lab)
Stephan A MacLaren
(Lawrence Livermore Natl Lab)
Joseph E Ralph
(Lawrence Livermore Natl Lab)
Vladimir Smalyuk
(Lawrence Livermore Natl Lab)
Robert E Tipton
(Lawrence Livermore Natl Lab)
Ryan F Sacks
(Los Alamos National Laboratory)
Two longstanding questions in ICF physics have been the extent to which capsule ablator material mixes into the burning fusion fuel and degrades performance, and the mechanism by which this mixing occurs. Several recent campaigns at the National Ignition Facility have examined this question through the use of separated reactants. A layer of CD plastic is placed on the inner surface of the CH shell and the shell is filled with a gas mixture of H and T. This allows for a direct measurement of neutron yield proportional to the amount of gas-ablator mixing. More recently, Ge dopant has been added to the CD layer, in order to move the mix into the partially ionized regime, as a stepping stone to higher-Z platforms which hope to use radiation trapping to lower the threshold for ignition.
This presentation will examine simulations of ablator-gas mix using two mixing paradigms: a Reynolds-averaged model which assumes fully-developed turbulence, and a Multicomponent Navier-Stokes diffusion-like model. We assess the ability of each model to simultaneously match the Ge doped and undoped capsules, and suggest future improvements to the models.
*This work was performed under the auspices of the U.S. Department of Energy by LLNL under Contract DE-AC52-07NA27344, LLNS, LLC.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.PO4.15
Follow Us |
Engage
Become an APS Member |
My APS
Renew Membership |
Information for |
About APSThe American Physical Society (APS) is a non-profit membership organization working to advance the knowledge of physics. |
© 2024 American Physical Society
| All rights reserved | Terms of Use
| Contact Us
Headquarters
1 Physics Ellipse, College Park, MD 20740-3844
(301) 209-3200
Editorial Office
100 Motor Pkwy, Suite 110, Hauppauge, NY 11788
(631) 591-4000
Office of Public Affairs
529 14th St NW, Suite 1050, Washington, D.C. 20045-2001
(202) 662-8700