Tuning the Optical Absorption of Anatase Thin Films Across the Visible-To-Near-Infrared Spectral Region

Pasquale Orgiani, Andrea Perucchi, Daniel Knez, Regina Ciancio, Chiara Bigi, Sandeep Kumar Chaluvadi, Jun Fujii, Ivana Vobornik, Giancarlo Panaccione, Giorgio Rossi, Stefano Lupi, and Paola Di Pietro
Phys. Rev. Applied 13, 044011 – Published 6 April 2020

Abstract

The electronic properties of anatase titanium dioxide (TiO2) thin films epitaxially grown on LaAlO3 substrates are investigated by synchrotron-x-ray spectroscopy [x-ray absorption spectroscopy (XAS), x-ray photoemission spectroscopy (XPS), and angle-resolved photoemission spectroscopy (ARPES)] and infrared spectroscopy. The Ti3+ fraction in TiO2x is varied either by changing the oxygen pressure during deposition or by postgrowth annealing in ultrahigh vacuum (UHV). Structural investigation of the TiO2 thin films provides evidence of highly uniform crystallographic order in both as-grown and in situ UHV-annealed samples. The increased amount of Ti3+ as a consequence of UHV annealing is calibrated by in situ XPS and XAS analysis. The as-grown TiO2 samples, with a low Ti3+ concentration, show distinct electronic properties with respect to the annealed films, namely, absorption in the midinfrared (MIR) region correlated with polaron formation, and another peak in the visible range at 1.6 eV correlated with the presence of localized defect states (DSs). With the increasing level of Ti3+ induced by the postannealing process, the MIR peak disappears, while the DS peak is redshifted to the near-infrared region at about 1.0 eV. These results indicate the possibility of tailoring the optical absorption of anatase TiO2 films from the visible to the near-infrared region.

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  • Received 25 October 2019
  • Revised 6 March 2020
  • Accepted 19 March 2020

DOI:https://doi.org/10.1103/PhysRevApplied.13.044011

© 2020 American Physical Society

Physics Subject Headings (PhySH)

Condensed Matter, Materials & Applied Physics

Authors & Affiliations

Pasquale Orgiani1,2,*, Andrea Perucchi3, Daniel Knez1, Regina Ciancio1, Chiara Bigi1,4, Sandeep Kumar Chaluvadi1, Jun Fujii1, Ivana Vobornik1, Giancarlo Panaccione1, Giorgio Rossi1,4, Stefano Lupi1,5, and Paola Di Pietro3

  • 1CNR-IOM TASC Laboratory, Trieste 34139, Italy
  • 2CNR-SPIN, UOS Salerno, Fisciano, SA 84084, Italy
  • 3Elettra Sincrotrone Trieste S.C.p.A., Trieste 34139, Italy
  • 4Department of Physics, University of Milano, Milano 20133, Italy
  • 5Department of Physics, University of Roma La Sapienza, Roma 00185, Italy

  • *pasquale.orgiani@spin.cnr.it

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Vol. 13, Iss. 4 — April 2020

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