The 68th JSAP Spring Meeting 2021

Presentation information

Oral presentation

7 Beam Technology and Nanofabrication » 7.1 X-ray technologies

[18a-Z14-1~11] 7.1 X-ray technologies

Thu. Mar 18, 2021 9:00 AM - 12:15 PM Z14 (Z14)

Akira Sasaki(QST), Mitsunori Toyoda(Tokyo Polytechnic Univ.)

9:45 AM - 10:00 AM

[18a-Z14-4] Two-photon laser-induced fluorescence of hydrogen atom in EUV photoionized plasma

〇(P)Baojun Zhu1, Chang Liu1, Nozomi Tanaka1, Katsunobu Nishihara1, Shinsuke Fujioka1, Kyung Sik Kang2, Youngduk Suh2, Jeong-Gil Kim2, Ken Ozawa3, Minoru Kubo3 (1.ILE, Osaka Univ., 2.MRD, Samsung, 3.Samsung R&D Inst.)

Keywords:EUV source EUV source, EUV photoionized plasma, Two-photon laser-induced fluorescence

Extreme-ultraviolet (EUV) light sources are being investigated intensively as a promoting application for lithography. Laser-produced Tin (Sn) plasma is one of the most significant EUV sources with a peak emission at 13.5 nm. Molybdenum silicon layered hetero structures (Mo/Si multilayers) are usually used as artificial Bragg crystals to collect the EUV light. However, the laser-produced Sn ions deposits on the highly delicate collector, and the reflectivity will be reduced. Hydrogen flow is applied to buffer the Sn ions and reduce the deposition rate on collector in the EUV lithography. Simultaneously, the hydrogen gas can be photoionized by the EUV radiation. Hydrogen radical (H*) is one of the most important production due to EUV dissociative photoionization. H* can be used to clean the EUV highly delicate optics based on the reaction of Sn + 4H* → SnH4. Detailed H* information under various conditions is needed in order to understand and predict their long-term impact on EUV optics. Laser-induced-fluorescence (LIF) is used to evaluate the spatial distribution and temporal evolution of the hydrogen radical’s density on ground state. In the experiment, H* is excited from 1s2S to the 3s2S and 3d2D levels with two photons near 205.14 nm at a laser intensity of 4.45×106 W/cm2. Then, the fluorescence at Balmer-α near 656.28 nm can be observed with the photomultiplier tube. The temporal evolution of H* density on ground state is determined from the fluorescence intensity.