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

机译:短的高强度激光脉冲通过中等密度的等离子体驱动的强吸收,强向前拉曼散射和相对论电子

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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. [References: 32]
机译:短而强的激光脉冲(1.057 mum,350 fs,10(17)W / cm(2)-2x10(19)W / cm(2))通过预先形成的临界等离子体的传播(大约为5%-40% n(c))已在位于Labouratoire pour l'Utilization des Lasers Intenses的100-TW激光设备上进行了实验研究。报告了1毫米激光脉冲的透射和反射,向前和向后拉曼(分别为F-SRS和B-SRS)散射光以及快速电子的发射。在这些等离子体中发生明显的吸收,发现吸收随着激光强度的增加而增加。 B-SRS在10(17)W / cm(2)下受到强烈驱动,并在较高强度下逐渐降低。结果表明,透射率低,并且仅弱依赖于激光强度。相反,在最低密度情况下,前向拉曼散射会随着激光强度的增加而不断增加,在2x10(19)W / cm(2)的情况下,高达7%的入射能量。正向加速的相对论电子似乎与F-SRS相关。根据最近的理论和数值研究讨论了实验数据,表明强烈的电子加热很可能在时间增长或抑制不稳定性中起主要作用。理论预测与实验一致。 (C)2002美国物理研究所。 [参考:32]

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