论文标题

平行平行谐振器配置高NNA EUV光刻的建议

Proposal of Plane-Parallel Resonator Configuration for High-NA EUV Lithography

论文作者

Shintake, Tsumoru

论文摘要

为高NA EUV光刻提出了平行 - 平行的谐振器构型,其中光刻掩码和晶片是通过两个聚焦镜进行排列的。 EUV光通过后焦平面的离轴旋转镜注入,并向面罩提供离轴照明(进型光束),并两次反弹(在面罩和晶圆上),最终从谐振器中脱离谐振器。这是一个单个路径腔,没有共鸣效应。旋转镜的轨道误差或振动不会影响成像质量。离轴照明对于恢复高空间频率并改善边缘对比度的高NA光学元件至关重要。匹配的环形孔位位于投影镜镜的后焦平面上,该镜像仅通过密度调制f(kx,ky,0)反射的水平散射波(0):0-th z订单傅立叶分量。在光束的单个进动过程中,该系统在晶圆上创建了掩模图案的正常投影密度图的2D图像,其中纵向变化(3D效应)消失,因此掩盖了遮罩问题。焦点(DOF)的深度很长,并且图像对比度也很高。作为客观镜,Schwarzschild物镜或沃尔特望远镜将是合适的候选人。沃尔特望远镜比传统的固体凹面镜是轴对称和较轻的,因此,可以在高进液中制造较大的直径。通过优化沃尔特望远镜,可以覆盖晶圆尺寸26毫米x 33毫米的单图案。进行了示例参数设计,在技术上似乎是可行的。

Plane-parallel resonator configuration is proposed for high-NA EUV lithography, where the lithography mask and the wafer are parallelly arranged through two focusing mirrors. EUV light is injected through an off-axis rotating mirror at the back focal plane and provides off-axis illumination (precession beam) to the mask and bounces back twice (at the mask and the wafer), finally goes out from the resonator through the rotating mirror. This is a single path cavity, there is no resonant effect. The orbital error or vibration of the rotating mirror do not affect on the imaging quality. The off-axis illumination is essential for high-NA optics, which recovers the high spatial frequency, and improves the edge contrast. The matched annular-aperture is located at the back-focal plane of the projector mirror, which acts as Fourier filter passing only the horizontally scattered waves reflected by the density modulations F(kx,ky,0) : 0-th z-order Fourier component of the mask. During single precession of the beam, this system creates 2D image of the normally projected density map of the mask pattern onto the wafer, where the longitudinal variation (3D effect) disappears, and thus the mask-shadowing problem is moderated. The depth-of-focus (DOF) is long, and also the image contrast becomes very high. As the objective mirror, Schwarzschild objective or Wolter telescope will be a suitable candidate. Wolter telescope is axisymmetric and lighter than conventional solid concave mirror, therefore, a larger diameter can be fabricated in high precession. By optimizing Wolter telescope, it may be possible to cover the wafer field size 26 mm x 33 mm of single patterning. Example parameter design was performed, seems technically feasible.

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