Detailed experimental results for high-trapping efficiency and narrow energy spread in a laser-driven accelerator

Presented are details of the staged electron laser acceleration (STELLA) experiment, which demonstrated high-trapping efficiency and narrow energy spread in a staged laser-driven accelerator. Trapping efficiencies of up to 80% and energy spreads down to 0.36% (1σ ) were demonstrated. The experiment...

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Veröffentlicht in:Physical review special topics. PRST-AB. Accelerators and beams 2004-09, Vol.7 (9), p.091301, Article 091301
Hauptverfasser: Kimura, W. D., Campbell, L. P., Dilley, C. E., Gottschalk, S. C., Quimby, D. C., Babzien, M., Ben-Zvi, I., Gallardo, J. C., Kusche, K. P., Pogorelsky, I. V., Skaritka, J., Yakimenko, V., Cline, D. B., Zhou, F., Steinhauer, L. C., Pantell, R. H.
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Sprache:eng
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Zusammenfassung:Presented are details of the staged electron laser acceleration (STELLA) experiment, which demonstrated high-trapping efficiency and narrow energy spread in a staged laser-driven accelerator. Trapping efficiencies of up to 80% and energy spreads down to 0.36% (1σ ) were demonstrated. The experiment validated an approach that may be suitable for the basic design of a laser-driven accelerator system. In this approach, a laser-driven modulator together with a chicane creates a train of microbunches spaced apart by the laser wavelength. These microbunches are sent into a second laser-driven accelerator designed to efficiently trap the microbunches in the ponderomotive potential well of the laser electric field while maintaining a narrow energy spread. The STELLA scientific apparatus and procedures are described in detail. In-depth comparisons between the data and model are given including the predicted energy spectrum, energy-phase plot, and microbunch length profile. Data and model comparisons as a function of the phase delay between the microbunches and the accelerating wave are presented. The model is exercised to reveal how the high-trapping efficiency process evolves during the acceleration process.
ISSN:1098-4402
1098-4402
2469-9888
DOI:10.1103/PhysRevSTAB.7.091301