Inverse free electron lasers and laser wakefield acceleration driven by CO sub(2) lasers

The staged electron laser acceleration (STELLA) experiment demonstrated staging between two laser-driven devices, high trapping efficiency of microbunches within the accelerating field and narrow energy spread during laser acceleration. These are important for practical laser-driven accelerators. ST...

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Veröffentlicht in:Philosophical transactions of the Royal Society of London. Series A: Mathematical, physical, and engineering sciences physical, and engineering sciences, 2006-03, Vol.364 (1840), p.611-622
Hauptverfasser: Kimura, W D, Andreev, N E, Babzien, M, Ben-Zvi, I, Cline, D B, Dilley, CE, Gottschalk, S C, Hooker, S M, Kusche, K P, Kuznetsov, S V, Pavlishin, I V, Pogorelsky, I V, Pogosova, A A, Steinhauer, L C, Ting, A, Yakimenko, V, Zigler, A, Zhou, F
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Sprache:eng
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Zusammenfassung:The staged electron laser acceleration (STELLA) experiment demonstrated staging between two laser-driven devices, high trapping efficiency of microbunches within the accelerating field and narrow energy spread during laser acceleration. These are important for practical laser-driven accelerators. STELLA used inverse free electron lasers, which were chosen primarily for convenience. Nevertheless, the STELLA approach can be applied to other laser acceleration methods, in particular, laser-driven plasma accelerators. STELLA is now conducting experiments on laser wakefield acceleration (LWFA). Two novel LWFA approaches are being investigated. In the first one, called pseudo-resonant LWFA, a laser pulse enters a low-density plasma where nonlinear laser/plasma interactions cause the laser pulse shape to steepen, thereby creating strong wakefields. A witness e-beam pulse probes the wakefields. The second one, called seeded self-modulated LWFA, involves sending a seed e-beam pulse into the plasma to initiate wakefield formation. These wakefields are amplified by a laser pulse following shortly after the seed pulse. A second e-beam pulse (witness) follows the seed pulse to probe the wakefields. These LWFA experiments will also be the first ones driven by a CO sub(2) laser beam.
ISSN:1364-503X
1471-2962
DOI:10.1098/rsta.2005.1726