Inverse free electron lasers and laser wakefield acceleration driven by CO2 lasers

被引:5
|
作者
Kimura, WD [1 ]
Andreev, NE
Babzien, M
Ben-Zvi, I
Cline, DB
Dilley, CE
Gottschalk, SC
Hooker, SM
Kusche, KP
Kuznetsov, SV
Pavlishin, IV
Pogorelsky, IV
Pogosova, AA
Steinhauer, LC
Ting, A
Yakimenko, V
Zigler, A
Zhou, F
机构
[1] STI Optron Inc, Bellevue, WA 98004 USA
[2] Brookhaven Natl Lab, Upton, NY 11973 USA
[3] Univ Calif Los Angeles, Los Angeles, CA 90095 USA
[4] Russian Acad Sci, Inst High Energy Densities, Moscow 125412, Russia
[5] Hebrew Univ Jerusalem, Racah Inst Phys, IL-91904 Jerusalem, Israel
[6] Univ Oxford, Oxford OX1 3PU, England
[7] Univ Washington, Redmond Plasma Phys Lab, Redmond, WA 98052 USA
[8] USN, Res Lab, Washington, DC 20375 USA
关键词
laser acceleration; laser wakefield acceleration; inverse free electron laser; CO2; laser; microbunch;
D O I
10.1098/rsta.2005.1726
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
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 CO2 laser beam.
引用
收藏
页码:611 / 622
页数:12
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