抄録
The structures of comet defects in a 4H-SiC homoepitaxially grown film are investigated by deep-ultraviolet micro-Raman spectroscopy. Spatial distribution of the 4H- and 3C-SiC is clearly distinguished both from the intensities of the folded longitudinal acoustic phonon mode and the peak energies of the nonfolded longitudinal optical phonon mode. The mappings of these parameters indicate the existence of two types of comets. The mechanisms of heteropolytypic inclusion in comets are discussed.
本文言語 | English |
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論文番号 | 241906 |
ページ(範囲) | 1-3 |
ページ数 | 3 |
ジャーナル | Applied Physics Letters |
巻 | 87 |
号 | 24 |
DOI | |
出版ステータス | Published - 2005 |
外部発表 | はい |
ASJC Scopus subject areas
- 物理学および天文学(その他)