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 GO7: Relativistic Laser Plasma Interaction and Particles (ions, electrons, positrons, neutrons) II
9:30 AM–11:54 AM,
Tuesday, November 6, 2018
OCC
Room: B117-119
Chair: Derek Mariscal, Lawrence Livermore National Lab
Abstract ID: BAPS.2018.DPP.GO7.6
Abstract: GO7.00006 : Ion Acceleration from Near-Critical-Density Plasmas via Magnetic Vortex Acceleration in 3D Particle-in-cell Simulations*
10:30 AM–10:42 AM
Presenter:
Jaehong Park
(Lawrence Berkeley Natl Lab)
Authors:
Jaehong Park
(Lawrence Berkeley Natl Lab)
Stepan Bulanov
(Univ of California - Berkeley)
Jean-Luc Vay
(Lawrence Berkeley Natl Lab)
Sven Steinke
(Lawrence Berkeley Natl Lab)
Jianhui Bin
(Lawrence Berkeley Natl Lab)
Qing Ji
(Lawrence Berkeley Natl Lab)
Cameron Guy Robinson Geddes
(Lawrence Berkeley Natl Lab)
Carl B Schroeder
(Lawrence Berkeley Natl Lab)
Eric Esarey
(Lawrence Berkeley Natl Lab)
Thomas Schenkel
(Lawrence Berkeley Natl Lab)
Wim Pieter Leemans
(Lawrence Berkeley Natl Lab)
We explored laser-driven ion acceleration via the Magnetic Vortex Acceleration scheme using 3D Warp+PICSAR and WarpX PIC simulation codes. In this scheme a high intensity and short pulse laser pulse propagates in near critical density plasma targets, making a channel in both electron and ion density. When the laser pulse exits the plasma, it establishes strong longitudinal electric fields that can accelerate the ions, which are pinched by the electrons in a thin filament along the laser propagation axis. We found that under the optimum conditions of the target thickness and density [1], the maximum ion energy in 3D is about 50% lower than that in 2D due to the smaller channel size in 3D. Particle tracking method is used to understand the acceleration process in more detail. [1] S. S. Bulanov, et al, Phys. Plasmas 17,043105(2010)
*The work was supported by the LDRD program of LBNL, the U.S. DOE Office of Science Offices of HEP and FES, under Contract DE-AC02-05CH11231, and by the U.S. DOE Exascale Computing Project (17-SC-20-SC). This research used resources (Edison, Cori) of NERSC, and an award of computation time by the INCITE program using resources of ALCF both supported by the Office of Science of the U.S. DOE under Contracts DE-AC02-05CH11231 and AC02-06CH11357, respectively.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.GO7.6
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. |
© 2025 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