2004
DOI: 10.1016/j.jmmm.2003.12.1355
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Evolution of properties of epitaxial bismuth iron garnet films with increasing thickness

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Cited by 32 publications
(16 citation statements)
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“…Figure 8 shows the specific Faraday rotation for all films in the spectral range of 1.9 to 2.4 eV. Films B, D, and E exhibit the same spectral variation with a pronounced peak at ϳ2.32 eV, whereas this peak occurs at lower energies of ϳ2.27 eV for films A and C. It must be pointed out that films A and C are somewhat thicker than films B, D, and E. A qualitatively similar red shift was observed by Kahl et al 25,26 when increasing the thickness of BIG films grown in otherwise identical conditions. These authors could not identify the cause of this apparent thickness dependence of the red shift, although a possible correlation with the x-ray coherence length was detected by x-ray diffraction.…”
Section: Room-temperature Magneto-optical Propertiessupporting
confidence: 76%
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“…Figure 8 shows the specific Faraday rotation for all films in the spectral range of 1.9 to 2.4 eV. Films B, D, and E exhibit the same spectral variation with a pronounced peak at ϳ2.32 eV, whereas this peak occurs at lower energies of ϳ2.27 eV for films A and C. It must be pointed out that films A and C are somewhat thicker than films B, D, and E. A qualitatively similar red shift was observed by Kahl et al 25,26 when increasing the thickness of BIG films grown in otherwise identical conditions. These authors could not identify the cause of this apparent thickness dependence of the red shift, although a possible correlation with the x-ray coherence length was detected by x-ray diffraction.…”
Section: Room-temperature Magneto-optical Propertiessupporting
confidence: 76%
“…1 for film C. This confirms that the garnet phase is obtained for a rather large range of experimental conditions as reported by most other authors. 26,30 Tepper et al 28 reported a narrower window of deposition conditions, maybe due to the fact that they used a low laser energy density for the deposition ͑1.4 J / cm 2 ͒. Traces of BiFeO 3 are observed in films A, C, and E. Slightly more intense BiFeO 3 peaks are found in film D. Adachi et al 22 also detected a weak BiFeO 3 peak in films grown by PLD with oxygen pressure above 30 mTorr.…”
Section: A Structure and Composition Of The Filmsmentioning
confidence: 99%
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