Bulletin of the American Physical Society
65th Annual Meeting of the APS Division of Plasma Physics
Monday–Friday, October 30–November 3 2023; Denver, Colorado
Session BO06: Magneto-Inertial Fusion, Z-pinches, X-pinches & Pulsed Power-Driven Plasmas
9:30 AM–12:30 PM,
Monday, October 30, 2023
Room: Governor's Square 15
Chair: David Strozzi, Lawrence Livermore Natl Lab
Abstract: BO06.00009 : Studying Gas Puff Xe Liner Staged Z-Pinch stability with FLASH simulations*
11:06 AM–11:18 AM
Presenter:
Victor Tranchant
(University of Rochester)
Authors:
Victor Tranchant
(University of Rochester)
Edward C Hansen
(University of Rochester)
Fernando Garcia Rubio
(Laboratory for Laser Energetics)
Kasper Moczulski
(University of Rochester)
Adam Reyes
(University of Rochester)
Petros Tzeferacos
(University of Rochester)
Marissa B Adams
(Sandia National Laboratories)
Paul Ney
(Magneto Inertial Fusion Technologies Inc.)
Hafiz U Rahman
(Magneto-Inertial Fusion Technology Inc.)
Emil Ruskov
(Magneto-Inertial Fusion Technology, Inc.)
The staged Z-pinch (SZP) is a pulsed-power–driven magneto inertial fusion concept under development at Magneto-Inertial Fusion Technology, Inc. (MIFTI). A new study has been focused onto a setup including a low-density gas-puff Xe liner, driven by the pulsed-power Z machine at Sandia National Laboratories, imploding on DT fuel. In particular, 1D FLASH simulations in cylindrical coordinates gave hope to achieve fuel ion temperatures > 15 keV and compression ratios (CR) > 300. Here, we show that the new capabilities of FLASH have made it possible to simulate this experiment in 2D, including magneto-Rayleigh Taylor instability (MRTI) growth. This inevitably caused those values to decrease in previous Z-pinches configurations. Here we present new results that support the viability of FLASH SZP simulations, and that shed light on potential stabilization of MRTI, by an applied axial magnetic field or modifications on the liner density profile, in order to make such an experiment plausible for fusion. Finally, first 3D simulations of this gas-puff Xe liner SZP are shown to illustrate the brand-new capabilities of the FLASH code.
*This material is based upon work supported by the Department of Energy (DOE) National Nuclear Security Administration (NNSA) under Award Numbers DE-NA0003856 and DE-NA0003842, the U.S. DOE Advanced Research Projects Agency-Energy (ARPA-E) under Award Number DE-AR0001272 and the U.S. DOE NNSA under subcontracts no. 536203 and 630138 with Los Alamos National Laboratory, and subcontract B632670 with Lawrence Livermore National Laboratory. We acknowledge support from the U.S. DOE Office of Science through the INFUSE program award DE-SC0023246. Sandia National Laboratories is a multi-mission laboratory managed and operated by National Technology & Engineering Solutions of Sandia, LLC, a wholly owned subsidiary of Honeywell International Inc., for the US DOE’s National Nuclear Security Administration (NNSA) under contract DE-NA0003525.
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