Relativistic electron acceleration by surface plasma waves excited with high intensity laser pulses

被引:9
|
作者
Zhu, X. M. [1 ,2 ,3 ]
Prasad, R. [1 ]
Swantusch, M. [1 ]
Aurand, B. [1 ]
Andreev, A. A. [4 ,5 ]
Willi, O. [1 ]
Cerchez, M. [1 ]
机构
[1] Heinrich Heine Univ Dusseldorf, Inst Laser & Plasmaphys, Univ Str 1, Dusseldorf 40225, Germany
[2] Chinese Acad Sci, Natl Astron Observ, Nanjing Inst Astron Opt & Technol, Nanjing 210042, Peoples R China
[3] Chinese Acad Sci, Nanjing Inst Astron Opt & Technol, Key Lab Astron Opt & Technol, Nanjing 210042, Peoples R China
[4] St Petersburg State Univ, 7-9 Univ Skaya Nab, St Petersburg 199034, Russia
[5] ELI ALPS, Dugon Ter 13, H-6722 Szeged, Hungary
关键词
laser-driven electron sources; relativistic plasmas; structured targets; surface electrons; HARMONICS; TARGETS;
D O I
10.1017/hpl.2020.14
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
The process of high energy electron acceleration along the surface of grating targets (GTs) that were irradiated by a relativistic, high-contrast laser pulse at an intensity $I=2.5\times 10<^>{20}\text{W}/\text{cm}<^>{2}$ was studied. Our experimental results demonstrate that for a GT with a periodicity twice the laser wavelength, the surface electron flux is more intense for a laser incidence angle that is larger compared to the resonance angle predicted by the linear model. An electron beam with a peak charge of ${\sim}2.7\text{nC}/\text{sr}$, for electrons with energies ${>}1.5\text{MeV}$, was measured. Numerical simulations carried out with parameters similar to the experimental conditions also show an enhanced electron flux at higher incidence angles depending on the preplasma scale length. A theoretical model that includes ponderomotive effects with more realistic initial preplasma conditions suggests that the laser-driven intensity and preformed plasma scale length are important for the acceleration process. The predictions closely match the experimental and computational results.
引用
收藏
页数:10
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