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Stimulated spin-flip Raman scattering in a Pb0.88 Sn0.12 Te single crystal
https://nitech.repo.nii.ac.jp/records/3714
https://nitech.repo.nii.ac.jp/records/37140f73b0ff-c69f-4820-9eaa-a2f113e90dec
名前 / ファイル | ライセンス | アクション |
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本文_fulltext (238.3 kB)
|
Copyright (1979) American Institute of Physics. This article may be downloaded for personal use only. Any other use requires prior permission of the author and the American Institute of Physics.The following article appeared in Applied physics letters, 34(10),pp.661-663 ; 1979 and may be found at http://link.aip.org/link/?apl/34/661
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Item type | 学術雑誌論文 / Journal Article(1) | |||||
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公開日 | 2012-11-06 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Stimulated spin-flip Raman scattering in a Pb0.88 Sn0.12 Te single crystal | |||||
言語 | ||||||
言語 | eng | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_6501 | |||||
資源タイプ | journal article | |||||
著者 |
Yasuda, Kazuhito
× Yasuda, Kazuhito× Shirafuji, Junji |
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著者別名 | ||||||
姓名 | 安田, 和人 | |||||
書誌情報 |
APPLIED PHYSICS LETTERS 巻 34, 号 10, p. 661-663, 発行日 1979-05-15 |
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出版者 | ||||||
出版者 | American Institute of Physics | |||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 00036951 | |||||
書誌レコードID(NCID) | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AA00543431 | |||||
著者版フラグ | ||||||
出版タイプ | VoR | |||||
出版タイプResource | http://purl.org/coar/version/c_970fb48d4fbd8a85 | |||||
DOI | ||||||
関連タイプ | isIdenticalTo | |||||
識別子タイプ | DOI | |||||
関連識別子 | http://dx.doi.org/10.1063/1.90628 | |||||
関連名称 | 10.1063/1.90628 | |||||
内容記述 | ||||||
内容記述タイプ | Other | |||||
内容記述 | Stimulated spin‐flip Raman emission assisted by resonance enhancement has been observed in an n‐type Pb0.88Sn0.12Te single crystal pumped by a TE CO2 laser. The wavelength of the Stokes emission can be tuned in a range from 10.8 to 11.8 μm for the pumping wavelength at 10.54 μm in the magnetic field range between 8 and 40 kG. The effective g value, when a magnetic field is applied along the 〈100〉 axis, is from 50 to 64, depending on the magnetic field. The intensity of the Stokes emission is strongly dependent upon the magnetic field. | |||||
フォーマット | ||||||
内容記述タイプ | Other | |||||
内容記述 | application/pdf |