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Temperature-dependent Schottky barrier parameters of Ni/Au on n-type (001) β-Ga2O3 Schottky barrier diode

  • P. R.Sekhar Reddy
  • , V. Janardhanam
  • , Kyu Hwan Shim
  • , V. Rajagopal Reddy
  • , Sung Nam Lee
  • , Se Jeong Park
  • , Chel Jong Choi*
  • *Corresponding author for this work
  • Jeonbuk National University
  • Sri Venkateswara University
  • Tech University of Korea
  • Ltd

Research output: Contribution to journalJournal articlepeer-review

Abstract

This study examined the temperature-dependent current-voltage (I–V) characteristics of the Ni/Au Schottky contact to β-Ga2O3. The Au/Ni/β-Ga2O3 Schottky diode showed a good rectifying behavior. The on-resistance and rectification ratio decreased with increasing temperature, which could be ascribed to the increase in the number of thermally activated electrons. The Au/Ni/β-Ga2O3 Schottky diode exhibited the strong temperature-dependence of Schottky barrier parameters, indicating the presence of inhomogeneous Schottky barrier prevailing in the interface between Ni and β-Ga2O3. The inhomogeneities were analyzed using thermionic emission with assuming a Gaussian distribution of barrier heights. The results revealed the existence of a double Gaussian distribution of barrier heights in the diode with a transition occurring at 225 K. The modified Richardson plot was evaluated using a Gaussian distribution approach and yielded a Richardson constant closely matching with the theoretical value of β-Ga2O3. The density of interface states, extracted using I–V characteristics, increased with decreasing temperature, which could be associated with the thermally-driven restructuring and reordering of the Ni/β-Ga2O3 interface state.

Original languageEnglish
Article number109012
JournalVacuum
Volume171
DOIs
StatePublished - 2020.01

Keywords

  • Barrier inhomogeneities
  • Double Gaussian distribution
  • Interface state density
  • Schottky barrier parameters
  • Schottky diodes
  • β-GaO

Quacquarelli Symonds(QS) Subject Topics

  • Materials Science
  • Physics & Astronomy

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