Backward Raman amplification of broad-band pulses

被引:12
作者
Balakin, A. A. [1 ,2 ]
Dodin, I. Y. [3 ]
Fraiman, G. M. [1 ,2 ]
Fisch, N. J. [3 ]
机构
[1] RAS, Inst Appl Phys, Nizhnii Novgorod, Russia
[2] State Univ Nizhny Novgorod, Nizhnii Novgorod, Russia
[3] Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA
基金
俄罗斯基础研究基金会;
关键词
PLASMA; FOCUSABILITY; AMPLIFIER; REGIME;
D O I
10.1063/1.4960835
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
A reduced fluid model of Raman backscattering is proposed that describes backward Raman amplification ( BRA) of pulses with duration tau(0) comparable to or even smaller than the plasma period 2 pi/omega(p). At such a small tau(0), a seed pulse can be amplified even if it has the same frequency as the pump ( which is technologically advantageous), as opposed to that satisfying the Raman resonance condition. Using our theoretical model, we numerically calculate the BRA efficiency for such pulses as a function of tau(0) and show that it remains reasonably high up to tau(0) approximate to 2 pi/omega(p). We also show that using short seed pulses in BRA makes the amplification less sensitive to quasistatic inhomogeneities of the plasma density. Amplification can persist even when the density perturbations are large enough to violate the commonly known condition of resonant amplification. Published by AIP Publishing.
引用
收藏
页数:9
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