Strong absorption, intense forward-Raman scattering and relativistic electrons driven by a short, high intensity laser pulse through moderately underdense plasmas

被引:36
作者
Rousseaux, C
le Gloahec, MR
Baton, SD
Amiranoff, F
Fuchs, J
Gremillet, L
Adam, JC
Héron, A
Mora, P
机构
[1] Ctr Etud Bruyeres Le Chatel, DIF, CEA, F-91680 Bruyeres Le Chatel, France
[2] Univ Paris 07, Ecole Polytech, CEA, CNRS,UMR 7605,LULI, F-91128 Palaiseau, France
[3] Ecole Polytech, Ctr Phys Theor, CNRS, UMR 7644, F-91128 Palaiseau, France
关键词
D O I
10.1063/1.1504715
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
The propagation of a short and intense laser pulse (1.057 mum, 350 fs, 10(17) W/cm(2)-2x10(19) W/cm(2)) through preformed undercritical plasmas (approximate to5%-40% of n(c)) has been experimentally investigated on the 100-TW laser facility at the Laboratoire pour l'Utilisation des Lasers Intenses. The transmission and reflection of the 1 mum laser pulse, the forward- and backward-Raman (respectively, F-SRS and B-SRS) scattered light and the emission of fast electrons are reported. Significant absorption occurs in these plasmas, which is found to increase with the laser intensity. B-SRS is strongly driven at 10(17) W/cm(2) and gradually decreases at higher intensities. It is shown that the transmission is low and only weakly dependent on the laser intensity. In contrast, the forward Raman scattering continuously increases with the laser intensity, up to 7% of the incident energy at 2x10(19) W/cm(2) in the lowest density case. The relativistic electrons accelerated in the forward direction appear to be correlated with the F-SRS. The experimental data are discussed in the light of recent theoretical and numerical investigations, indicating that intense electron heating is likely to play a major role in the temporal growth or inhibition of the instabilities. The theoretical predictions are in agreement with the experiments. (C) 2002 American Institute of Physics.
引用
收藏
页码:4261 / 4269
页数:9
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