Authors: Kazuhiko Kusunoki, Kazuhito Kamei, Nobuhiro Okada, Nobuyoshi Yashiro, Akihiro Yauchi, Toru Ujihara, Kazuo Nakajima
Abstract: We performed solution growth of SiC single crystals from Si-Ti-C ternary solution using
the accelerated crucible rotation technique (ACRT). It was confirmed that the growth rate exceeding
200 μm/hr was achievable by several ACRT conditions. This high growth rate might be due to the
enhancement of the carbon transport from the graphite crucible to the growth interface using the
ACRT. Moreover, the incorporation of inclusions of the Si-Ti solvent in the grown crystal was
significantly suppressed by using the ACRT. It was thought that the intensive convection near the
growth interface resulted in not only the marked increase of SiC growth rate but also the superior
homogeneity in the surface morphology. It was concluded that faster stable growth can be
accomplished in the SiC solution growth using the ACRT.
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Authors: Nobuyoshi Yashiro, Kazuhiko Kusunoki, Kazuhito Kamei, Mitsuhiro Hasebe, Toru Ujihara, Kazuo Nakajima
Abstract: We carried out the growth of single crystalline silicon carbide (SiC) from Si-C-X (X= Co,
Fe) ternary solutions. These ternary solutions are expected to show large carbon solubility
compared with Si solvent (self-flux) by means of CALPHAD (CALculation of PHAse Diagrams)
method. We investigated the growth rate and the polytype of the grown crystal from the ternary
solutions. Then we found that the growth rate from the ternary solutions is much larger than that
from the self-flux. The growth rate from Si-C-Co (Si-C-Fe) system was about 6mm/hr (12mm/hr)
while that from the self-flux was only 2mm/hr. The grown crystal from the ternary solutions is
classified into 6H that takes over the seed polytype.
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Authors: Kazuhiko Kusunoki, Kazuhito Kamei, Y. Ueda, S. Naga, Y. Ito, Mitsuhiro Hasebe, Toru Ujihara, Kazuo Nakajima
Abstract: The growth of 6H-SiC crystal from Si-Ti-C ternary solution was conducted under the
temperature gradient and the crystalline quality evaluations of the grown crystals were carried out. 6H-SiC(0001) on-axis pvt-grown crystal was used as a seed crystal. Micropipes in the seed crystal were terminated during the solution growth and 28mm28mm self-standing micropipe-free SiC crystals were obtained. The quality of the grown crystals was investigated by SIMS, high-resolution
x-ray diffraction and molten KOH etching. The content of residual impurities in the SiC were very low. The X-ray -rocking curves of the solution grown SiC showed single peak with high peak intensity ,while that of the seed crystal showed several peaks due to the misoriented domains. Moreover, it was found that the number of etch-pit in the grown crystal is much less than that in the seed crystal and it decreases with the increase of the growth thickness. These results indicate that the
crystalline quality of grown crystal was significantly improved during the solution growth.
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Authors: Toru Ujihara, S. Munetoh, Kazuhiko Kusunoki, Kazuhito Kamei, N. Usami, K. Fujiwara, G. Sazaki, Kazuo Nakajima
633
Authors: Kazuhito Kamei, Kazuhiko Kusunoki, S. Munetoh, Toru Ujihara, Kazuo Nakajima
347
Authors: Kazuhiko Kusunoki, S. Munetoh, Kazuhito Kamei, Mitsuhiro Hasebe, Toru Ujihara, Kazuo Nakajima
123
Authors: Shigeru Okada, Kunio Kudou, T. Mori, Takaaki Shishido, I. Higashi, Naoki Kamegashira, Kazuo Nakajima, T. Lundström
Abstract: Single crystals of AlMgB 14 and AlMgB 22 were grown from a high-temperature aluminum metal flux in an Ar atmosphere. The optimum conditions for growing AlMgB 22 and AlMgB 14 were established using the starting mixtures of B/Mg=0.5-1.0 and B/Mg=2.0-6.0. The AlMgB 14 and AlMgB 22 crystals obtained have well-developed {001} and {100} faces, and were black with a metallic luster. The maximum dimensions of these crystals were about 5.2 mm and 4.6 mm, respectively. The values of micro-Vickers hardness of the AlMgB 14 and AlMgB 22 crystals are in the ranges of 23.9±0.6-27.6±0.6 GPa. The oxidation process of AlMgB 14 and AlMgB 22 crystals were studied up to 1473 K by TG-DTA method. The susceptibility of AlMgB14 with an increase at low temperatures does not show any particular features, being indicative of a paramagnetic contribution, which is likely due to impurities. The susceptibility of the AlMgB 22 sample shows no apparent
contribution from impurities and also does not have any anomalous behavior.
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Authors: Atsuro Eitoku, Rita Vos, James Snow, M. Sato, S. Hirae, Kazuo Nakajima, M. Nonomura, M. Imai, Paul W. Mertens, Marc Heyns
157
Authors: S. Okamoto, Kazuo Nakajima
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