2007
DOI: 10.1016/j.actamat.2006.07.031
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Raman study of gap mode and lattice disorder effect in InN films prepared by plasma-assisted molecular beam epitaxy

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Cited by 29 publications
(35 citation statements)
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“…31 In our Raman scattering experiments, the A1(TO) and A1(LO) modes of hexagonal InN were observed at wave numbers of 447 cm -1 and 586 cm -1 together with peaks ascribed to yet unidentified defects at 180 cm -1 and 375 cm -1 . 32,33 The band peaking at 436 cm -1 is due to second-order Raman scattering from the Si substrate. 34 The sharp rise in parts (c, d) of the Figure 12 is due to the wings of the strong Raman peak of the substrate at 520 cm -1 .…”
Section: Resultsmentioning
confidence: 99%
“…31 In our Raman scattering experiments, the A1(TO) and A1(LO) modes of hexagonal InN were observed at wave numbers of 447 cm -1 and 586 cm -1 together with peaks ascribed to yet unidentified defects at 180 cm -1 and 375 cm -1 . 32,33 The band peaking at 436 cm -1 is due to second-order Raman scattering from the Si substrate. 34 The sharp rise in parts (c, d) of the Figure 12 is due to the wings of the strong Raman peak of the substrate at 520 cm -1 .…”
Section: Resultsmentioning
confidence: 99%
“…That means this wafer can be used as the novel substrate for MEMS sensors in the future. Meanwhile, the Raman spectrum is different with Figure 2 c; there are two peaks in Figure 3 c. Because of that, as described in reference [ 19 , 20 ], the phonon characteristic length reduces as the defect density increases. The transverse mode of phonon is an even parity and a Raman active mode, different from longitudinal mode.…”
Section: Resultsmentioning
confidence: 81%
“…Raman scattering experiments, the A 1 (TO) and A 1 (LO) modes of hexagonal InN were observed at wave numbers of 447 cm -1 and 586 cm -1 together with peaks ascribed to yet unidentified defects at 180 cm -1 and 375 cm -1 . 28,29 The band peaking at 436 cm -1 is due to second-order Raman scattering from the Si substrate. 30 The sharp rise in parts (c, d) of the Figure 13 is due to the wings of the strong Raman peak of the substrate at 520 cm -1 .…”
Section: Resultsmentioning
confidence: 99%