2002
DOI: 10.1088/0953-8984/14/5/302
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Evolution of Raman spectra as a function of layer thickness in ultra-thin InSe films

Abstract: Experimentally, when compared with III-V, II-VI, or IV-IV layered systems, the InSe Raman spectrum does not change very much as a function of the number of InSe layers. A simple linear chain model is sufficient to explain this effect. In our model, two parameters are used to characterize Raman spectra: the halfwidth Γ characterizing the sample quality and the coherence length Λ determined by the sample thickness n. Our analysis shows that the coherence length Λ is linear in n. We obtain a fair agreement betw… Show more

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Cited by 14 publications
(6 citation statements)
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“…Second‐order modes are also visible at RT and result from overtones of E 1 2g (402 cm −1 ) and A 2u (423 cm −1 ) . It is worth noting that the peak positions of all modes have no significant energy shift in the ex‐InSe sample as is the case for c‐InSe (Figure S5, Supporting Information), which is in agreement with previous experimental studies . Interestingly, no modes relating to other InSe‐based compounds are observed, confirming that the stoichiometry is preserved without the formation of other chemical species during the exfoliation process .…”
Section: Resultssupporting
confidence: 89%
“…Second‐order modes are also visible at RT and result from overtones of E 1 2g (402 cm −1 ) and A 2u (423 cm −1 ) . It is worth noting that the peak positions of all modes have no significant energy shift in the ex‐InSe sample as is the case for c‐InSe (Figure S5, Supporting Information), which is in agreement with previous experimental studies . Interestingly, no modes relating to other InSe‐based compounds are observed, confirming that the stoichiometry is preserved without the formation of other chemical species during the exfoliation process .…”
Section: Resultssupporting
confidence: 89%
“…Using the estimated values of η 0 , we obtain G 0 ∼ 1.0 and 1.5 THz for InSe and hBN, respectively. These values are smaller than the zone edge phonon frequencies for propagation perpendicular to the layers, i.e., f = 1.2 and 2.4 THz for InSe [81] and hBN [75], respectively, but much higher than the maximum phonon frequency f ∼ 100 GHz measured in our experiments. Thus we conclude that our use of the continuous approximation with bulk elastic parameters and sound velocity of InSe and hBN is valid in our analysis of the phonon spectra.…”
Section: A Elastic Properties Of Inse and Hbncontrasting
confidence: 77%
“…The inset of figure 3(a) shows the Raman shift versus layer thickness of the A 1 (LO+TO), A 1 (TO), and A 1 (LO) peaks of as-grown β-In 2 Se 3 . The A 1 (LO+TO) mode at ∼110 cm −1 does not depend on the layer thickness, although, the A 1 (TO), and A 1 (LO) phonon modes exhibit a small shift to lower wavenumbers with decreasing L. This could arise from the smaller vibration coherence length along the c-axis due to the weak van der Waals force along this direction [26].…”
Section: Resultsmentioning
confidence: 91%