首页> 外文会议>IEEE International Conference on Plasma Science;ICOPS 2012 >Accurate calculation of high harmonics generated by interactions between very intense laser fields and electron plasmas
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Accurate calculation of high harmonics generated by interactions between very intense laser fields and electron plasmas

机译:精确计算由非常强的激光场和电子等离子体之间的相互作用产生的高次谐波

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we proved that the analytical expression of the intensity of the relativistic Thomson scattered field for a system composed of an electron interacting with a plane electromagnetic field can be written as a periodic function of only one variable, that is the phase of the incident field. This property was proved without using any approximation, except for neglecting the radiative corrections, in the most general case, in which the field is elliptically polarized, the initial phase of the incident field and the initial velocity of the electron are taken into consideration, and the direction in which the radiation is scattered is arbitrary. This property led to an exact method for calculating the angular and spectral distributions of the scattered field. We present the application of the method to the case of the interaction of very intense laser beams with electron plasmas resulted during the ionization of gas. We prove that the frequency of the fundamental scattered radiation does not depend on the relativistic parameters, this result being in very good agreement with the result of the Compton model approach. We calculate the shape of the spectrum of the scattered radiations and show that the number of the harmonics increases as the value of the relativistic parameter increases. The high harmonics spectrum has a maximum shifting to the shorter wavelengths. The method accurately predicts the angular distribution of the scattered radiations. All these properties are in good agreement with the experimental data from literature.
机译:我们证明,由电子与平面电磁场相互作用的系统的相对论汤姆森散射场强度的解析表达式可以写成只有一个变量的周期函数,即入射场的相位。在不使用任何近似的情况下证明了该性质,只是在大多数情况下忽略了辐射校正,在这种情况下,场是椭圆极化的,入射场的初始相位和电子的初始速度都被考虑在内,并且辐射的散射方向是任意的。这种性质导致了一种精确的方法来计算散射场的角度和光谱分布。我们介绍了该方法在气体离子化过程中产生非常强烈的激光束与电子等离子体相互作用的情况下的应用。我们证明了基本散射辐射的频率不依赖于相对论参数,这一结果与康普顿模型方法的结果非常吻合。我们计算了散射辐射的频谱形状,并表明谐波的数量随着相对论参数值的增加而增加。高次谐波光谱最大程度地移向了较短的波长。该方法准确地预测了散射辐射的角度分布。所有这些性质与文献中的实验数据非常吻合。

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