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 KI3: Magnetized-Liner Inertial Fusion
3:00 PM–5:24 PM,
Tuesday, November 6, 2018
OCC
Room: Oregon Ballroom 204
Chair: Matthew Weis, Sandia National Laboratory
Abstract ID: BAPS.2018.DPP.KI3.4
Abstract: KI3.00004 : Laser-Driven Magnetized Liner Inertial Fusion on OMEGA*
4:48 PM–5:24 PM
Presenter:
Jonathan Davies
(Univ of Rochester)
Author:
Jonathan Davies
(Univ of Rochester)
Laser-driven magnetized liner inertial fusion (MagLIF) has been developed on the OMEGA Laser System in a joint SNL-LLE project funded by ARPA-E. MagLIF relies on compressing cylindrical, magnetized, and preheated plasma to achieve fusion with inertial confinement. The magnetic field reduces electron heat flow into the shell (liner), allowing compressional heating at implosion velocities < 200 km/s, and confines the alpha particles, replacing the radial areal density requirement for ignition with a BR requirement of 0.6 T m. Preheating to > 100 eV reduces the fuel convergence ratio required to achieve fusion temperatures to < 30. MagLIF experiments on Z have achieved temperatures of 3 keV, BR of 0.4 T m, and DD neutron yields of 1013. However, these are the only MagLIF experiments being carried out. Laser-driven MagLIF on OMEGA is providing the first experimental data on scaling, with 1000× less drive energy and targets 10× smaller in linear dimensions. OMEGA also allows more shots than Z with better diagnostic access and a greater dynamic range. OMEGA targets are 0.6-mm-outer-diam, 20-μm-thick, D2-filled plastic cylinders. MIFEDS (magneto-inertial fusion electrical discharge system) provides an axial magnetic field up to 28 T (the highest to date). A single OMEGA beam preheats the D2 up to 200 eV, and then 40 OMEGA beams delivering 14 kJ compress the target. A full overview of the project will be given, from the initial point design process, preheat experiments, compression optimization experiments, up to the most recent fully integrated experiments.
*This material is based upon work supported by the Advanced Research Projects Agency-Energy (ARPA-E), U.S. Department of Energy, under Award Number DE-AR0000568, the Department of Energy Office of Fusion Energy Science under award DESC0016258 and 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.KI3.4
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