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 GO08: Laser-wakefield and direct laser acceleration
9:30 AM–12:30 PM,
Tuesday, October 31, 2023
Room: Grand Ballroom II
Chair: Isabella Pagano, University of Texas at Austin
Abstract: GO08.00006 : Controlled electron injection from wake shaping using co-propagating laser pulses*
10:30 AM–10:42 AM
Presenter:
Nicholas Ernst
(University of Michigan - Ann Arbor)
Authors:
Nicholas Ernst
(University of Michigan - Ann Arbor)
Alexander G Thomas
(University of Michigan)
Karl Krushelnick
(University of Michigan)
celeration (LWFA) operating in the high-intensity bubble regime. In this scheme, the
plasma acts to couple a high-intensity “driver” pulse to a phase controlled, low power
“satellite” pulse co-propagating off-axis. The satellite is tightly focused such that it
perturbs and drives a transient, asymmetric plasma wave before depleting. Doing so al-
lows for spatio-temporal manipulation or “shaping” of the wakefield to create a trigger
for overcoming the wave-breaking threshold and leads to efficient particle trapping and
acceleration. Supported by 2D and 3D Particle-in-Cell simulations using OSIRIS, we
demonstrate systematic investigation of the two-beam parameter space (e.g. temporal de-
lay, beam displacement, etc.) leads to control over beam pointing, charge, and emittance.
Results indicate this technique could be used to induce self-injection at plasma densities
and laser intensities well below theoretical predictions using satellites of less than 1% the
driver energy. Further scaling to additional co-propagating pulses proves to distort the
initial plasma wave formation in a predictable manner for near arbitrary wake-shaping.
This allows for an ad hoc spatiotemporal setup to control the momentum space of in-
jected electrons, leading to a route for enhanced and polarized betatron oscillations. The
results show promise for an all-optical knob to transition between a high charge, mono-
energetic, GeV accelerator and an enhanced x-ray source from betatron radiation through
independent tuning of the satellite.
*This work is supported in part by the U.S Department of Energy Office of Science under Award No. DE-SC0020070, AFOSR Grant No. FA9550-19-1-0072, and the OSIRIS Consortium consisting of UCLA and IST (Lisbon, Portugal).
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