Skip to content

Preparation and ultraviolet detection performance of Cu doped <i>β</i>-Ga<sub>2</sub>O<sub>3</sub> thin films

MetadataDetails
Publication Date2023-01-01
JournalActa Physica Sinica
AuthorsWei Liu, Qiu-Ju Feng, Ziqi Yi, Yu Chen, Shuo Wang
Citations2
AnalysisFull AI Review Included

This research successfully synthesized p-type Cu-doped beta-Ga2O3 (β-Ga2O3) thin films using Chemical Vapor Deposition (CVD) and demonstrated their high performance as solar-blind ultraviolet (UV) photodetectors.

  • P-Type Conductivity Achieved: Hall measurements confirmed successful p-type doping, with the highest hole concentration reaching 1.69 x 1016 cm-3 in the film with the highest Cu content (Sample C).
  • CVD Synthesis: A cost-effective CVD method was utilized on sapphire substrates, yielding films with high crystallinity, confirmed by XRD analysis showing Cu2+ substitution into the Ga2O3 lattice.
  • High Sensitivity: The fabricated Metal-Semiconductor-Metal (MSM) photodetector (Sample C) achieved a maximum photo-to-dark current ratio (Ilight/Idark) of 3.81 x 102 under 254 nm UV illumination at 10 V bias.
  • Exceptional Efficiency: The device demonstrated a high responsivity (R) of 1.72 A/W and a corresponding External Quantum Efficiency (EQE) of 841% at a low light intensity of 64 µW/cm2.
  • Fast Response: The detector exhibited rapid switching characteristics, with a rise time (τr) of 0.11 s and a decay time (τd) of 0.13 s.
  • Bandgap Engineering: Increased Cu doping concentration resulted in a bandgap redshift, narrowing the optical bandgap from 4.87 eV (low Cu) to 4.80 eV (high Cu).
ParameterValueUnitContext
Material SystemCu-doped β-Ga2O3N/AGrown on Sapphire (Al2O3)
Doping Typep-typeN/AConfirmed by Hall measurement
Max Hole Concentration1.69 x 1016cm-3Sample C (Highest Cu content)
Max Photo-to-Dark Current Ratio3.81 x 102N/ASample C, 10 V bias, 254 nm
Peak Responsivity (R)1.72A/WSample C, 64 µW/cm2 light intensity
Peak External Quantum Efficiency (EQE)841%Sample C, 64 µW/cm2 light intensity
Rise Time (τr)0.11sSample C response time
Decay Time (τd)0.13sSample C recovery time
Optical Bandgap (Eg) Range4.87 to 4.80eVDecreases with increasing Cu content
Operating Wavelength254nmSolar-blind UV
Operating Bias10VStandard test voltage
Detector StructureMSMN/AAu interdigitated electrodes
Electrode Finger Width/Spacing20 / 20µmAu electrodes
Max Detectivity (D*)5.65 x 1012JonesCalculated at 64 µW/cm2

The Cu-doped β-Ga2O3 thin films were grown on sapphire substrates using a low-cost Chemical Vapor Deposition (CVD) method, followed by MSM device fabrication.

  1. Substrate Preparation: Sapphire substrates were cleaned sequentially using acetone, ethanol, and deionized water via ultrasonic agitation (10 min per step).
  2. Precursor Mixing: The reaction source consisted of mixed powders: Ga2O3 (99.99%), CuO (99.99%), and Carbon (C, 99.99%). Carbon served as the reducing agent.
  3. CVD Growth Parameters:
    • Growth Temperature: 1000 °C.
    • Reaction Time: 30 min.
    • Carrier Gas (Ar) Flow Rate: 200 mL·min-1.
    • Reaction Gas (O2) Flow Rate: 50 mL·min-1.
  4. Doping Control: Three samples (A, B, C) were prepared by varying the Ga2O3/CuO mass ratio (25:1, 25:2, and 25:3, respectively) to control the Cu doping concentration.
  5. Structural and Compositional Analysis:
    • Scanning Electron Microscopy (SEM) assessed surface morphology (films became rougher with increased Cu content).
    • X-ray Diffraction (XRD) confirmed the monoclinic β-Ga2O3 structure and showed a shift in the (201) peak to lower angles, verifying Cu2+ incorporation.
    • Energy Dispersive Spectroscopy (EDS) confirmed Cu molar percentages (1.3% to 2.4%).
  6. Electrical and Optical Characterization: Hall effect measurements confirmed p-type conductivity. UV-Vis spectroscopy determined the optical absorption and bandgap.
  7. Device Fabrication: Au interdigitated electrodes (1000 µm length, 20 µm width, 20 µm spacing) were deposited onto the Cu-doped β-Ga2O3 films using electron beam evaporation to form the MSM photodetector structure.

The development of p-type β-Ga2O3 and high-performance solar-blind UV detectors based on this material opens doors for applications requiring high sensitivity and immunity to background visible light.

  • Aerospace and Defense:
    • Missile tracking and guidance systems (solar-blind detection prevents false alarms from sunlight).
    • Space-to-space communication links.
  • Safety and Security:
    • High-speed, reliable flame and fire detection systems in industrial plants, aircraft, and hazardous environments.
  • Environmental Monitoring:
    • Detection and monitoring of atmospheric ozone (O3) and other UV-absorbing pollutants.
  • Power Electronics (Future Potential):
    • While this study focuses on detection, β-Ga2O3’s intrinsic properties (4.9 eV bandgap, 8 MV/cm breakdown field) are foundational for next-generation high-power switches and rectifiers.
  • Biomedical and Sterilization:
    • UV dosage monitoring in sterilization equipment (e.g., water purification, medical tools).
View Original Abstract

Solar-blind UV photodetectors (SBPs) have attracted great attention because they are widely used in missile tracking, fire detection, biochemical analysis, astronomical observations, space-to-space communications, etc. At present, it is found that wide bandgap semiconductor materials such as Al<sub><i>x</i></sub>Ga<sub>1-<i>x</i></sub>N, Mg<sub>1</sub>Zn<sub>1-<i>x</i></sub>O, diamond and <i>β</i>-Ga<sub>2</sub>O<sub>3</sub> are ideal semiconductor materials for developing high-performance SBPs. The ultra-wide band gap semiconductor material, <i>β</i>-Ga<sub>2</sub>O<sub>3</sub>, has a large band gap width of 4.9 eV, strong breakdown electric field, absorption edge located in the solar blind ultraviolet band (200-280 nm), and it also has high transmittance in the near ultraviolet and the whole visible band. Therefore, <i>β</i>-Ga<sub>2</sub>O<sub>3</sub> is a very suitable material for making solar blind UV photodetectors. However, the p-type <i>β</i>-Ga<sub>2</sub>O<sub>3</sub> is difficult to dope, which limits the further development of <i>β</i>-Ga<sub>2</sub>O<sub>3</sub> devices. In this work, the <i>β</i>-Ga<sub>2</sub>O<sub>3</sub> thin films with different Cu doping content are grown on sapphire substrates by chemical vapor deposition method, and the morphology, crystal structure and optical properties of <i>β</i>-Ga<sub>2</sub>O<sub>3</sub> films are measured. The test results show that the surfaces of <i>β</i>-Ga<sub>2</sub>O<sub>3</sub> films with different Cu content are relatively smooth, and the (<inline-formula><tex-math id=“M2”>\begin{document}$ \bar 201 $\end{document}</tex-math><alternatives><graphic xmlns:xlink=“http://www.w3.org/1999/xlink” xlink:href=“19-20230971_M2.jpg”/><graphic xmlns:xlink=“http://www.w3.org/1999/xlink” xlink:href=“19-20230971_M2.png”/></alternatives></inline-formula>) diffraction peak positions shift toward the lower degree side with the increase of Cu content, which indicates that Cu<sup>2+</sup> replaces Ga<sup>3+</sup> and enters into the <i>β</i>-Ga<sub>2</sub>O<sub>3</sub> lattice. The optical absorption spectrum measurement indicates that the energy gaps of samples are evidently narrowed with the increase of Cu doping concentration. Hall measurements indicate that the Cu doped <i>β</i>-Ga<sub>2</sub>O<sub>3</sub> thin films have a p-type conductivity with a hole concentration of 7.36 × 10<sup>14</sup>, 4.83 × 10<sup>15</sup> and 1.69 × 10<sup>16 </sup>cm<sup>-3</sup>, respectively. In addition, a photoconductive UV detector with metal-semiconductor-metal structure is prepared by evaporating Au on a Cu-doped <i>β</i>-Ga<sub>2</sub>O<sub>3</sub> thin film, and its UV detection performance is studied. The results show that the photocurrent value of the device increases with Cu content increasing. The photo-to-dark current ratio (<i>I</i><sub>l</sub>/<i>I</i><sub>d</sub>) is about 3.8×10<sup>2</sup> of 2.4% Cu content device under 254 nm-wavelength light at 10 V. The rise time and decay time are 0.11 s and 0.13 s, respectively. Furthermore, the responsivity and external quantum efficiency can reach 1.72 A/W and 841% under 254 nm-wavelength light with a light intensity of 64 μW/cm<sup>2</sup>.