Infrared ellipsometry study of the photo-generated charge carriers at the (001) and (110) surfaces of SrTiO$_3$ crystals and the interface of corresponding LaAlO$_3$/SrTiO$_3$ heterostructures
M. Yazdi-Rizi, P. Marsik, B.P.P. Mallett, K. Sen, A. Cerreta, A., Dubroka, M. Scigaj, F. S\'anchez, G. Herranz, C. Bernhard

TL;DR
This study uses infrared ellipsometry and transport measurements to analyze photo-generated charge carriers at SrTiO3 surfaces and LaAlO3/SrTiO3 interfaces, revealing persistent carriers linked to oxygen vacancies and defect trapping, with implications for mobility anisotropy.
Contribution
It provides new insights into the origin and behavior of photo-induced charge carriers and their relation to oxygen vacancies and structural defects in SrTiO3 and heterostructures.
Findings
Photo-generated carriers accumulate near the SrTiO3 surface with similar profiles to confined electrons in heterostructures.
Persistent charge carriers remain at low temperature after UV illumination, originating from oxygen vacancies trapped at domain boundaries.
Mobility anisotropy at the interface can be controlled and inverted through thermal, optical, or mechanical means.
Abstract
With infrared (IR) ellipsometry and DC resistance measurements we investigated the photo-doping at the (001) and (110) surfaces of SrTiO (STO) single crystals and at the corresponding interfaces of LaAlO/SrTiO (LAO/STO) heterostructures. In the bare STO crystals we find that the photo-generated charge carriers, which accumulate near the (001) surface, have a similar depth profile and sheet carrier concentration as the confined electrons that were previously observed in LAO/STO (001) heterostructures. A large fraction of these photo-generated charge carriers persist at low temperature at the STO (001) surface even after the UV light has been switched off again. These persistent charge carriers seem to originate from oxygen vacancies that are trapped at the structural domain boundaries which develop below the so-called antiferrodistortive transition at T* = 105 K. This is most…
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