AVS 57th International Symposium & Exhibition
    Energy Frontiers Topical Conference Monday Sessions
       Session EN+PS-MoM

Paper EN+PS-MoM1
Combinatorial Plasma CVD of Si Thin Films with a Multihollow Discharge Plasma CVD Reactor

Monday, October 18, 2010, 8:20 am, Room Mesilla

Session: Plasmas for Photovoltaics & Energy Applications
Presenter: M. Shiratani, Kyushu University, Japan
Authors: M. Shiratani, Kyushu University, Japan
K. Koga, Kyushu University, Japan
T. Matsunaga, Kyushu University, Japan
Y. Kawashima, Kyushu University, Japan
W. Nakamura, Kyushu University, Japan
G. Uchida, Kyushu University, Japan
N. Itagaki, Kyushu University, Japan
Correspondent: Click to Email

A-Si and micro-crystalline thin films for solar cells are widely deposited by plasma CVD in industry. To realize combinatorial plasma CVD of such Si thin films, we have developed a multi-hollow discharge plasma CVD method, by which fluxes of H and SiH3 as well as their flux ratio on the substrate placed perpendicular to the electrodes depend on the distance from the discharges [1-4]. Thus, we can simultaneously deposit Si thin films with various structures and properties. For 60 MHz discharges of H2+SiH4 (0.3%), no films were deposited just near the discharge regions due to Si etching by H, micro-crystalline films were deposited in a rather narrow area around the no film regions, and a-Si:H films were obtained in the rest wide area far from the discharges. The spatial distribution of film structures indicate that the density ratio of H to SiH3 decreases sharply with increasing the distance from the discharges and the surface reaction probability of H is much higher than that of SiH3, being consistent with the reported surface reaction probabilities [5, 6]. For 2-6 Torr, the micro-crystalline film structure such as crystalline volume fraction and grain size varies sharply not only along the direction perpendicular to the electrodes but also along the direction parallel to the electrodes. These results suggest that the micro-crystalline film structure is highly sensitive to spatial and temporal uniformity of fluxes of H and SiH3 as well as their flux ratio.

[1] K. Koga, et al., Jpn. J. Appl. Phys. 44, L1430 (2005).

[2] W. M. Nakamura, et al., IEEE Trans. Plasma Sci. 36, 888 (2008).

[3] W. M. Nakamura, et al., J. Phys.: Conf. Series 100, 082018 (2008).

[4] H. Sato, et al., J. Plasma Fusion Res. SERIES, 8, 1435 (2009).

[5] A. Matsuda, et al., Surface Sci. 227, 50 (1990).

[6] J. Perrin, et al., J. Vac. Sci. Technol. A, 16, 278 (1998).