4.8 Article

Persistent Room-Temperature Photodarkening in Cu-Doped β-Ga2O3

期刊

PHYSICAL REVIEW LETTERS
卷 128, 期 7, 页码 -

出版社

AMER PHYSICAL SOC
DOI: 10.1103/PhysRevLett.128.077402

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资金

  1. Air Force Office of Scientific Research [FA9550-18-1-0507]
  2. U.S. Department of Energy, Office of Basic Energy Sciences, Division of Materials Science and Engineering [DE-FG02-07ER46386]
  3. Air Force Institute of Technology by an NRC Research Associateship Award
  4. U.S. DOE by Lawrence Livermore National Laboratory (LLNL) [DE-AC52-07NA27344]
  5. LLNL Laboratory Directed Research and Development [22-SI-003]
  6. Critical Materials Institute, an Energy Innovation Hub - U.S. DOE, Office of Energy Efficiency and Renewable Energy, Advanced Manufacturing Office

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This study finds that exposure of Cu-doped beta-Ga2O3 to UV light (>4 eV) causes large, persistent photo induced darkening at room temperature. Light exposure converts Cu2+ to Cu3+ and leads to the appearance of O-H vibrational modes. Cu acceptors can form favorable complexes with hydrogen donors, and when these complexes absorb light, hydrogen is released, resulting in the formation of Cu3+ species and O-H modes.
beta-Ga2O3 is an ultrawide band gap semiconductor with emerging applications in power electronics. The introduction of acceptor dopants yields semi-insulating substrates necessary for thin-film devices. In the present work, exposure of Cu-doped beta-Ga2O3 to UV light >4 eV is shown to cause large, persistent photo induced darkening at room temperature. Electron paramagnetic resonance spectroscopy indicates that light exposure converts Cu2+ to Cu3+, a rare oxidation state that is responsible for the optical absorption. The photodarkening is accompanied by the appearance of O-H vibrational modes in the infrared spectrum. Hybrid function calculations show that Cu acceptors can favorably complex with hydrogen donors incorporated as interstitial (H-i) or substitutional (H-O) defects. When Cu-Ga-H-O complexes absorb light, hydrogen is released, contributing to the observed Cu3+ species and O-H modes.

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