Infrared optical responses of wurtzite InxGa1 − xN thin films with porous surface morphology

Room temperature infrared (IR) optical responses of wurtzite indium gallium nitride (InxGa1 − xN) in the composition range of 0.174 ≤ x ≤ 0.883 were investigated by the polarized IR reflectance spectroscopy. Analyses of the amplitudes of oscillation fringes in the non-reststrahlen region revealed th...

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Main Authors: Yew, P., Lee, S.C., Ng, S.S., Abu Hassan, H., Chen, W.L., Osipowicz, T., Ren, M.Q.
Format: Article
Language:English
Published: Elsevier B.V. 2016
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Online Access:http://eprints.intimal.edu.my/735/1/Infrared%20optical%20responses%20of%20wurtzite%20InxGa1%20%E2%88%92%20xN%20thin%20films%20with%20porous.pdf
http://eprints.intimal.edu.my/735/
http://dx.doi.org/10.1016/j.tsf.2016.02.039
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spelling my-inti-eprints.7352017-03-14T07:54:43Z http://eprints.intimal.edu.my/735/ Infrared optical responses of wurtzite InxGa1 − xN thin films with porous surface morphology Yew, P. Lee, S.C. Ng, S.S. Abu Hassan, H. Chen, W.L. Osipowicz, T. Ren, M.Q. QC Physics Room temperature infrared (IR) optical responses of wurtzite indium gallium nitride (InxGa1 − xN) in the composition range of 0.174 ≤ x ≤ 0.883 were investigated by the polarized IR reflectance spectroscopy. Analyses of the amplitudes of oscillation fringes in the non-reststrahlen region revealed that the high frequency dielectric constants of the samples were unusually smaller than the values predicted from the Clausius–Mossotti relation. This odd behavior was attributed to the porous surface morphology of the InxGa1 − xN samples. The E1 optical phonon modes of the InxGa1 − xN were deduced from the composition dependent reststrahlen features. The obtained values were compared to those calculated through the modified random element iso-displacement (MREI) model. The deviation between the measured data and the MREI model prediction were explained in detail from the aspects of strain, thermal expansion and anharmonic phonon-coupling. Finally, it was found that the large discrepancy of the E1(LO) mode is mainly attributed to the effects of the longitudinal phonon–plasmon coupling. Elsevier B.V. 2016 Article PeerReviewed text en http://eprints.intimal.edu.my/735/1/Infrared%20optical%20responses%20of%20wurtzite%20InxGa1%20%E2%88%92%20xN%20thin%20films%20with%20porous.pdf Yew, P. and Lee, S.C. and Ng, S.S. and Abu Hassan, H. and Chen, W.L. and Osipowicz, T. and Ren, M.Q. (2016) Infrared optical responses of wurtzite InxGa1 − xN thin films with porous surface morphology. Thin Solid Films, 603. pp. 334-341. ISSN 0040-6090 http://dx.doi.org/10.1016/j.tsf.2016.02.039
institution INTI International University
building INTI Library
collection Institutional Repository
continent Asia
country Malaysia
content_provider INTI International University
content_source INTI Institutional Repository
url_provider http://eprints.intimal.edu.my
language English
topic QC Physics
spellingShingle QC Physics
Yew, P.
Lee, S.C.
Ng, S.S.
Abu Hassan, H.
Chen, W.L.
Osipowicz, T.
Ren, M.Q.
Infrared optical responses of wurtzite InxGa1 − xN thin films with porous surface morphology
description Room temperature infrared (IR) optical responses of wurtzite indium gallium nitride (InxGa1 − xN) in the composition range of 0.174 ≤ x ≤ 0.883 were investigated by the polarized IR reflectance spectroscopy. Analyses of the amplitudes of oscillation fringes in the non-reststrahlen region revealed that the high frequency dielectric constants of the samples were unusually smaller than the values predicted from the Clausius–Mossotti relation. This odd behavior was attributed to the porous surface morphology of the InxGa1 − xN samples. The E1 optical phonon modes of the InxGa1 − xN were deduced from the composition dependent reststrahlen features. The obtained values were compared to those calculated through the modified random element iso-displacement (MREI) model. The deviation between the measured data and the MREI model prediction were explained in detail from the aspects of strain, thermal expansion and anharmonic phonon-coupling. Finally, it was found that the large discrepancy of the E1(LO) mode is mainly attributed to the effects of the longitudinal phonon–plasmon coupling.
format Article
author Yew, P.
Lee, S.C.
Ng, S.S.
Abu Hassan, H.
Chen, W.L.
Osipowicz, T.
Ren, M.Q.
author_facet Yew, P.
Lee, S.C.
Ng, S.S.
Abu Hassan, H.
Chen, W.L.
Osipowicz, T.
Ren, M.Q.
author_sort Yew, P.
title Infrared optical responses of wurtzite InxGa1 − xN thin films with porous surface morphology
title_short Infrared optical responses of wurtzite InxGa1 − xN thin films with porous surface morphology
title_full Infrared optical responses of wurtzite InxGa1 − xN thin films with porous surface morphology
title_fullStr Infrared optical responses of wurtzite InxGa1 − xN thin films with porous surface morphology
title_full_unstemmed Infrared optical responses of wurtzite InxGa1 − xN thin films with porous surface morphology
title_sort infrared optical responses of wurtzite inxga1 − xn thin films with porous surface morphology
publisher Elsevier B.V.
publishDate 2016
url http://eprints.intimal.edu.my/735/1/Infrared%20optical%20responses%20of%20wurtzite%20InxGa1%20%E2%88%92%20xN%20thin%20films%20with%20porous.pdf
http://eprints.intimal.edu.my/735/
http://dx.doi.org/10.1016/j.tsf.2016.02.039
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