2016
DOI: 10.1016/j.optmat.2016.09.003
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Yellow luminescence band in undoped GaN revealed by two-wavelength excited photoluminescence

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Cited by 34 publications
(16 citation statements)
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“…In this study, the YL band of GaN exhibited a peak at 540 nm (2.3 eV), which can be ascribed to the Ga vacancies (V Ga ) point defects [41,42]. For carrier recombination through defect states in undoped GaN films, considerable research has been conducted on the origin of YL emissions, and a model of carrier transition from the shallow donor to the deep acceptor levels was established and studied [43]. Moreover, recent investigations have proposed that the YL emission in GaN films can be due to a V Ga -O N , single C N defect, or C N-O N compound [44][45][46].…”
Section: Resultsmentioning
confidence: 99%
“…In this study, the YL band of GaN exhibited a peak at 540 nm (2.3 eV), which can be ascribed to the Ga vacancies (V Ga ) point defects [41,42]. For carrier recombination through defect states in undoped GaN films, considerable research has been conducted on the origin of YL emissions, and a model of carrier transition from the shallow donor to the deep acceptor levels was established and studied [43]. Moreover, recent investigations have proposed that the YL emission in GaN films can be due to a V Ga -O N , single C N defect, or C N-O N compound [44][45][46].…”
Section: Resultsmentioning
confidence: 99%
“…Meanwhile, the yellow luminescence at 550 nm is increased as the irradiation fluence increases up to 1.32×10 16 cm -2 . The yellow luminescence comes from the recombination from shallow donor to deep states [10]. The electron irradiation leads to formation of various defects such as vacancies causing the appearance of deep defect levels in the bandgap [11].…”
Section: Methodsmentioning
confidence: 99%
“…Vacancy complexes with oxygen (V Ga -O N ) or silicon (V Ga -Si Ga ) might be responsible for YG luminescence. Additionally, C N -O N technological defects may also be a reason for YG luminescence [54]. It seems that Ga vacancies are most probable non-radiative recombination centres.…”
Section: Evolution Of the Photoluminescence Spectramentioning
confidence: 99%