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Evolution analysis of EUV radiation from laser-produced tin plasmas based on a radiation hydrodynamics model

机译:基于辐射流体动力学模型的激光产生锡等离子体的EUV辐射演化分析

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摘要

One of fundamental aims of extreme ultraviolet (EUV) lithography is to maximize brightness or conversion efficiency of laser energy to radiation at specific wavelengths from laser produced plasmas (LPPs) of specific elements for matching to available multilayer optical systems. Tin LPPs have been chosen for operation at a wavelength of 13.5 nm. For an investigation of EUV radiation of laser-produced tin plasmas, it is crucial to study the related atomic processes and their evolution so as to reliably predict the optimum plasma and experimental conditions. Here, we present a simplified radiation hydrodynamic model based on the fluid dynamic equations and the radiative transfer equation to rapidly investigate the evolution of radiation properties and dynamics in laser-produced tin plasmas. The self-absorption features of EUV spectra measured at an angle of 45° to the direction of plasma expansion have been successfully simulated and explained, and the evolution of some parameters, such as the plasma temperature, ion distribution and density, expansion size and velocity, have also been evaluated. Our results should be useful for further understanding of current research on extreme ultraviolet and soft X-ray source development for applications such as lithography, metrology and biological imaging.
机译:极紫外(EUV)光刻的基本目标之一是使特定元素的激光产生等离子体(LPP)产生的特定波长的激光能量向特定波长的辐射的亮度或转换效率最大化,以匹配现有的多层光学系统。锡LPP已选择在13.5nm的波长下运行。为了研究激光产生的锡等离子体的EUV辐射,至关重要的是研究相关的原子过程及其演变过程,以便可靠地预测最佳等离子体和实验条件。在这里,我们提出了一个基于流体动力学方程和辐射传递方程的简化辐射流体动力学模型,以快速研究激光产生的锡等离子体中辐射特性和动力学的演变。已经成功地模拟和解释了以45°角与等离子体膨胀方向成角度测量的EUV光谱的自吸收特征,以及一些参数的演变,例如等离子体温度,离子分布和密度,膨胀尺寸和速度,也已被评估。我们的研究结果对于进一步了解目前用于光刻,计量学和生物成像等应用的极紫外和软X射线源研究应是有用的。

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