2021
DOI: 10.1016/j.spmi.2021.107053
|View full text |Cite
|
Sign up to set email alerts
|

Research on the crystal phase and orientation of Ga2O3 Hetero-epitaxial film

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1

Citation Types

0
3
0

Year Published

2023
2023
2024
2024

Publication Types

Select...
3

Relationship

1
2

Authors

Journals

citations
Cited by 3 publications
(3 citation statements)
references
References 23 publications
0
3
0
Order By: Relevance
“…By increasing the oxygen flow, the ε-Ga 2 O 3 (0002) and ε-Ga 2 O 3 (0004) diffraction peaks were effectively eliminated at oxygen flow rates of 1600 and 1800 sccm, respectively, and the diffraction peaks reappeared when the oxygen flow rate reached 2100 sccm. Besides, in all curves, there are two remaining faint diffraction peaks located at 30.4 and 60.7°, which can be attributed to (004), and (512) β-Ga 2 O 3 , respectively . Apparently, the films appear to consist of a blend of β-Ga 2 O 3 and ε-Ga 2 O 3 phase, and it has not obtained pure ε-Ga 2 O 3 through control temperature and oxygen flow.…”
Section: Resultsmentioning
confidence: 92%
See 1 more Smart Citation
“…By increasing the oxygen flow, the ε-Ga 2 O 3 (0002) and ε-Ga 2 O 3 (0004) diffraction peaks were effectively eliminated at oxygen flow rates of 1600 and 1800 sccm, respectively, and the diffraction peaks reappeared when the oxygen flow rate reached 2100 sccm. Besides, in all curves, there are two remaining faint diffraction peaks located at 30.4 and 60.7°, which can be attributed to (004), and (512) β-Ga 2 O 3 , respectively . Apparently, the films appear to consist of a blend of β-Ga 2 O 3 and ε-Ga 2 O 3 phase, and it has not obtained pure ε-Ga 2 O 3 through control temperature and oxygen flow.…”
Section: Resultsmentioning
confidence: 92%
“…Besides, in all curves, there are two remaining faint diffraction peaks located at 30.4 and 60.7°, which can be attributed to (004), and (512) β-Ga 2 O 3 , respectively. 31 Apparently, the films appear to consist of a blend of β-Ga 2 O 3 and ε-Ga 2 O 3 phase, and it has not obtained pure ε-Ga 2 O 3 through control temperature and oxygen flow. This could be attributed to a smaller lattice mismatch between the β-Ga 2 O 3 films and the sapphire substrate during the film growth, in contrast to ε-Ga 2 O 3 , and it is difficult to avoid forming a nucleus to form a β-Ga 2 O 3 in the thin film and the substrate interface.…”
Section: Resultsmentioning
confidence: 96%
“…20,21 Compared to b-Ga 2 O 3 , e-Ga 2 O 3 has a similar wide bandgap (B4.9 eV), higher lattice symmetry, lower anisotropic crystal structure, and lower growth temperature. [22][23][24][25] In recent years, research studies on solar-blind UV detectors based on e-Ga 2 O 3 thin films have begun to rise and are receiving increasing attention. [26][27][28] Although many efforts are being dedicated towards developing high-performance e-Ga 2 O 3 thin film solar-blind detectors, it is still a big challenge to simultaneously achieve low dark current, high specific detectivity, high UVvisible rejection ratio and quick response speed.…”
Section: Introductionmentioning
confidence: 99%