Bulletin of the American Physical Society
66th Annual Meeting of the APS Division of Plasma Physics
Monday–Friday, October 7–11, 2024; Atlanta, Georgia
Session ZI03: Invited: Post Deadline
9:30 AM–1:00 PM,
Friday, October 11, 2024
Hyatt Regency
Room: Centennial IV
Chair: Navid Vafaei-Najafabadi, Stony Brook University
Abstract: ZI03.00002 : Reliable operation of a laser plasma accelerator driven free electron laser*
10:00 AM–10:30 AM
Presenter:
Sam Barber
(Lawrence Berkeley National Laboratory)
Authors:
Sam Barber
(Lawrence Berkeley National Laboratory)
Finn Kohrell
(Lawrence Berkeley National Laboratory)
Kyle Jensen
(Lawrence Berkeley National Laboratory)
Christopher E Doss
(Lawrence Berkeley National Laboratory)
Curtis Berger
(University of California, Berkeley)
Anthony J Gonsalves
(Lawrence Berkeley National Laboratory)
Kei Nakamura
(Lawrence Berkeley National Laboratory)
Guillaume Plateau
(TAU Systems, Inc)
Reinier van Mourik
(TAU Systems, Inc)
Stephen Milton
(TAU Systems, Inc)
Carl B Schroeder
(Lawrence Berkeley National Laboratory)
Eric Esarey
(Lawrence Berkeley National Laboratory)
Jeroen Van Tilborg
(Lawrence Berkeley National Laboratory)
beams and much higher accelerating gradients. This enables more compact designs for future light sources, such as free electron lasers (FELs). FEL technology leveraging LPA sources is
progressing swiftly, with several key milestones achieved in recent years. However, significant work remains to be done to move from proof-of-concept experiments to the dependable
operation of LPA-driven FELs. Recent initiatives at the BELLA center's Hundred Terawatt Undulator beamline, which includes an electron beam transport section leading to a 4-meter-
long, strong focusing undulator, have successfully demonstrated the consistent operation of a high-gain FEL in the SASE regime. SASE gain is detectable on 90% of shots with measured
SASE gain in excess of 1000.
*This work was supported by the U.S. Department of Energy (DOE) Office of Science under Contract No. DE-AC02-05CH11231, and through a CRADA with Tau Systems.
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