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Measuring the EUV-induced contamination rates of TiO_2-capped multilayer optics by anticipated production-environment hydrocarbons

机译:通过预期的生产环境碳氢化合物测量EUV引起的TiO_2封顶的多层光学器件的污染率

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The primary, publicly reported cause of optic degradation in pre-production extreme-ultraviolet (EUV) lithography systems is carbon deposition. This results when volatile organics adsorb onto optic surfaces and then are cracked by EUV-induced reactions. Hence the deposition rate depends on the adsorption-desorption kinetics of the molecule-surface system as well as the basic photon-stimulated reaction rates, both of which may vary significantly for different organic species. The goal of our ongoing optics-contamination program is to estimate the contamination rate of species expected in the tool environment by exposing samples to in-band 13.5 nm light from our synchrotron in the presence of fixed partial pressures of admitted gases. Here we report preliminary results of contamination rates on TiO_2-capped samples for species observed in resist-outgassing measurements (benzene, isobutene, toluene and tert-butylbenzene) in the pressure range (10~(-6) to 10~(-4)) Pa which all display an unexpected logarithmic dependence on pressure. This scaling is in agreement with previous EUV exposures of other species at NIST as well as independent measurements of coverage performed at Rutgers University. These results are consistent with a molecular desorption energy that decreases with coverage due to molecular interactions (Temkin model). Use of the proper scaling law is critical when estimating optic lifetimes by extrapolating over the 3-to-6 orders of magnitude between accelerated-testing and tool-environment partial pressures.
机译:公开报道的生产前的极紫外(EUV)光刻系统中光学性能下降的主要原因是碳沉积。当挥发性有机物吸附到光学表面上,然后被EUV诱导的反应裂解时,会导致这种情况。因此,沉积速率取决于分子-表面系统的吸附-解吸动力学以及基本的光子刺激的反应速率,这两种速率对于不同的有机物可能会发生显着变化。我们正在进行的光学污染程序的目标是,在允许的固定气体分压存在的情况下,通过将样品暴露于来自同步加速器的带内13.5 nm光中,来估计工具环境中预期物质的污染率。在这里,我们报告了在压力范围(10〜(-6)至10〜(-4))中,在抗蚀剂除气测量(苯,异丁烯,甲苯和叔丁基苯)中观察到的物种中,被TiO_2覆盖的样品的污染率的初步结果。 )Pa都显示出对压力的意外对数依赖关系。此比例与之前在NIST上其他物种的EUV暴露以及罗格斯大学进行的覆盖率独立测量一致。这些结果与分子解吸能量一致,该分子解吸能量由于分子相互作用而随着覆盖率的降低而降低(Temkin模型)。当通过在加速测试和工具环境分压之间的3到6个数量级外推来估计光学器件寿命时,使用适当的定标定律至关重要。

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