Exciton photoluminescence and benign defect complex formation in zinc tin nitride

Angela N. Fioretti, Jie Pan, Brenden R. Ortiz, Celeste L. Melamed, Patricia C. Dippo, Laura T. Schelhas, John D. Perkins, Darius Kuciauskas, Stephan Lany, Andriy Zakutayev, Eric S. Toberer, Adele C. Tamboli

Research output: Contribution to journalArticlepeer-review

38 Scopus citations

Abstract

Emerging photovoltaic materials need to prove their viability by demonstrating excellent electronic properties. In ternary and multinary semiconductors, disorder and off-stoichiometry often cause defects that limit the potential for high-efficiency solar cells. Here we report on Zn-rich ZnSnN2 (Zn/(Zn + Sn) = 0.67) photoluminescence, high-resolution X-ray diffraction, and electronic structure calculations based on Monte-Carlo structural models. The mutual compensation of Zn excess and O incorporation affords a desirable reduction of the otherwise degenerate n-type doping, but also leads to a strongly off-stoichiometric and disordered atomic structure. It is therefore remarkable that we observe only near-edge photoluminescence from well-resolved excitons and shallow donors and acceptors. Based on first principles calculations, this result is explained by the mutual passivation of ZnSn and ON defects that renders both electronically benign. The calculated bandgaps range between 1.4 and 1.8 eV, depending on the degree of non-equilibrium disorder. The experimentally determined value of 1.5 eV in post-deposition annealed samples falls within this interval, indicating that further bandgap engineering by disorder control should be feasible via appropriate annealing protocols.

Original languageEnglish
Pages (from-to)823-830
Number of pages8
JournalMaterials Horizons
Volume5
Issue number5
DOIs
StatePublished - Sep 2018
Externally publishedYes

Funding

This material is based upon work supported by the U.S. Department of Energy’s (DOE) Office of Energy Efficiency and Renewable Energy (EERE) under Solar Energy Technologies Office (SETO) Agreement Number 30302. This work used computational resources sponsored by EERE, located at the National Renewable Energy Laboratory (NREL). Use of the Stanford Synchrotron Radiation Lightsource, SLAC National Accelerator Laboratory, is supported by DOE’s Office of Science (SC), Basic Energy Sciences (BES) under Contract No. DE-AC02-76SF00515. X-ray diffraction measurements at SLAC were also supported by DOE-SC-BES, Materials Sciences and Engineering Division.

FundersFunder number
DOE Office of Science
U.S. Department of Energy’s
U.S. Department of Energy
Office of Energy Efficiency and Renewable Energy
Basic Energy Sciences
Solar Energy Technologies Office30302

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