Microscopic origin of electron accumulation in In2O3
There are only a handful of materials combining optical transparency in the visible region with high electrical conductivity. This unusual conjunction is exploited in liquid crystal and electroluminescent displays, as well as in photovoltaic cells. One of the mostly widely used so-called transparent conducting oxides is Sn-doped In2O3, aka ITO. Despite its almost ubiquitous application, several aspects of the physics of this material are still controversial. A striking example is provided the band gap of In2O3. By using photoemission spectroscopy, a team of scientists of Elettra and the University of Oxford have recently determined a value of 2.7 eV, almost 1 eV lower than previous estimates. This important finding points to the existence of a pronounced downward band bending, giving rise to an electron accumulation layer, contrary to the established picture of an upward band bending generating a depletion layer. The cause of such electron accumulation has so far remained elusive. |
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In order to gain further insight on this intriguing system, the high brightness and high energy and momentum resolution of the BaDElPh beamline was used to acquire photoemission spectra from single crystal thin films of In2O3 grown by oxygen plasma assisted molecular beam epitaxy. The low photon energies used in the measurements ensured a probing depth comparable with the electron accumulation layer thickness. The measured photoemission intensity close to the Fermi energy for a sample with a bulk carrier density of only 1.5x1019 cm-3 is very much stronger than expected in comparison with ITO where the carrier density is 30 times higher (see Figure 1).
This qualitatively demonstrates the existence of an accumulation layer. Interestingly, we found that the intensity of this feature is strongly suppressed by annealing in oxygen, suggesting that doubly ionized oxygen vacancies in the outermost ionic layer act as the source of the electrons in the accumulation layer. Theoretical calculations support this picture and demonstrate that surface oxygen vacancies have a much reduced formation energy than bulk vacancies and act as shallow donors. |
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This research was conducted by the following research teams:
- Kelvin Hongliang Zhang, Russell G. Egdell, Inorganic Chemistry Laboratory, University of Oxford, Oxford, United Kingdom
- Francesco Offi, CNISM and Dipartimento di Fisica, Università Roma Tre, Roma, Italy
- Stefano Iacobucci, CNR-IFN and Dipartimento di Fisica, Università Roma Tre, Roma, Italy
- Luca Petaccia, Sergey Gorovikov, Elettra - Sincrotrone Trieste, Trieste, Italy
- Philip D.C. King, School of Physics and Astronomy, University of St. Andrews, St. Andrews, United Kingdom
Reference
K.H. Zhang, R.G. Egdell, F. Offi, S. Iacobucci, L. Petaccia, S. Gorovikov and P.D.C. King, “Microscopic Origin of Electron Accumulation in In2O3”, Phys. Rev. Lett. 110, 056803 (2013), DOI: 10.1103/PhysRevLett.110.056803 |
This paper was highlighted as an “Editor’s Suggestion”. |