Raman scattering investigation of RB6 (R=Ca, La, Ce, Pr, Sm, Gd, Dy, and Yb)
Physical Review B - Condensed Matter and Materials Physics 68 巻 22 号
224305-1-224305-9 頁
2003-12-30 発行
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PhysRevB_68_224305.pdf
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種類 :
全文
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タイトル ( eng ) |
Raman scattering investigation of RB6 (R=Ca, La, Ce, Pr, Sm, Gd, Dy, and Yb)
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作成者 |
Nagai Shinji
Okamoto Naoki
Iga Fumitoshi
Kunii Satoru
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収録物名 |
Physical Review B - Condensed Matter and Materials Physics
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巻 | 68 |
号 | 22 |
開始ページ | 224305-1 |
終了ページ | 224305-9 |
抄録 |
The excitation-energy, polarization, and temperature dependeces of Raman scattering spectra have been measured for the RB6 crystals (R=Ca 2+, La3+, Ce3+, Pr3+, Sm 2.6+, Gd3+, Dy3+, and Yb2+). In the divalent crystals of CaB6 and YbB6, the Eg phonon shows doublet, while the line shape is a broad single peak for the trivalent case. In the trivalent crystals, two kinds of the extra peaks have been clearly observed at around 200 cm-1 and at around 1400 cm -1 in addition to the Raman-active phonons and crystal electric-field (CEF) excitations. The peak intensities at around 200 cm -1 show the anomalous decrease with decreasing temperature, and this temperature dependence correlates with that of the mean-square displacement of the R ion. Furthermore, their energies decrease with the increase of the cage space due to B6. These peaks are originated from the second-order excitation of acoustic phonons. The broad peak at around 1400 cm-1 is assigned as the second-order excitation of the T2g phonon. For the T2g phonon, the energy difference and its line-shape change between the trivalent and divalent crystals suggests the existence of electron-phonon interaction. We have observed the CEF excitation in PrB 6 and have obtained the Lea, Leask, and Wolf parameters with x=0.94 and W=9.2 K.
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言語 |
英語
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資源タイプ | 学術雑誌論文 |
出版者 |
American Physical Society
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発行日 | 2003-12-30 |
権利情報 |
Copyright (c) 2003 American Physical Society.
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出版タイプ | Version of Record(出版社版。早期公開を含む) |
アクセス権 | オープンアクセス |
収録物識別子 |
[ISSN] 0163-1829
[DOI] 10.1103/PhysRevB.68.224305
[NCID] AA11187113
[DOI] http://dx.doi.org/10.1103/PhysRevB.68.224305
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