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 NO08: Laser-plasma ion acceleration
9:30 AM–12:18 PM,
Wednesday, October 9, 2024
Hyatt Regency
Room: The Learning Center (Fixed)
Chair: Douglas Storey, SLAC National Accelerator Laboratory
Abstract: NO08.00007 : Optimization of laser-driven ion acceleration from pre-expanded liquid water microjets*
10:42 AM–10:54 AM
Presenter:
Griffin D Glenn
(SLAC National Accelerator Laboratory)
Authors:
Griffin D Glenn
(SLAC National Accelerator Laboratory)
Girik Jain
(SLAC National Accelerator Laboratory)
Daniel P Deponte
(SLAC National Accelerator Laboratory)
Michal Elkind
(Tel-Aviv University, Israel)
Stefano Faubel
(SLAC National Accelerator Laboratory)
Jhonnatan Gama Vazquez
(Stanford University - SLAC National Accelerator Laboratory)
Assaf Levanon
(Tel-Aviv University, Israel)
Aviv Levinson
(Tel-Aviv University, Israel)
Ishay Pomerantz
(Tel-Aviv University, Israel)
Siegfried H Glenzer
(SLAC National Accelerator Laboratory)
Maxence Gauthier
(SLAC - National Accelerator Laboratory)
Here we present results from a high repetition rate experiment studying proton acceleration from liquid water targets that were pre-expanded by an independent ps-duration pulse. This experiment was performed at the 0.5 J, 30 fs NePTUN laser facility at Tel Aviv University, which delivers high-contrast pulses at 10 Hz. The targets were ambient-temperature planar liquid water sheets developed by our group. We will describe the characteristics of the proton beams and the target pre-expansion conditions for optimized ion beam energies and yields. These results will guide future experiments studying ion acceleration from targets in the near-critical density regime at higher laser intensities to demonstrate ion acceleration to energies beyond those accessible from the conventional TNSA mechanism.
*This work was supported by the U.S. DOE Office of Science, Fusion Energy Sciences under FWP 100182, by the National Science Foundation under grant numbers 1632708 and PHY-1903414, and by the NSF-BSF under grant number 2308860. G. D. G. acknowledges support from the DOE NNSA SSGF program under DE-NA0003960.
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