Crystallite size and microstrain in the structure of SrTiO3 formed by magnetron deposition with and without O2 flow through the deposition chambre

TL;DR

This study investigates how different deposition conditions and nickel doping levels affect the crystallite size and microstrain in SrTiO3 thin films prepared by magnetron deposition, aiming to understand their structural properties related to photocatalytic activity.

Contribution

It provides new insights into how oxygen flow and nickel doping influence the microstructure of SrTiO3 films prepared via magnetron deposition.

Findings

Oxygen flow affects crystallite size and microstrain.

Nickel doping modifies the structural properties.

Deposition conditions influence oxygen vacancy formation.

Abstract

Transition metal oxides, which have a perovskite structure, have received much attention in recent decades. This is because of the very suitable properties that can be used in various industries. One of the fields where the properties of Perovskites can and have already been applied is in the power industry. Experimental studies of the last few years have reliably demonstrated that, using simple modifications, perovskite oxides can be used in applications utilizing direct sunlight and photocatalytic applications. The original strontium titanate oxide SrTiO3 (abbreviated STO) is only able to use the UV component of incident radiation and is inactive in visible light, remaining transparent to visible light. The reason for this state is its wide band gap, which at room temperature has a value of 3.2 - 3.25 eV. Studies have shown that doping the structure of these oxides with transition metals (TM) can cause a shift in the valence and/or conduction band. This is because of the 3d dopant bands that create new energy levels in the mentioned band gap, effectively reducing it. One of the elements of the TM group is nickel. According to some studies, it is likely that the Ni ion occurs in the cubic structure of STO in the form of Ni2+ and substitutes the Ti4+ sites. In the case of using this dopant, the shift of the absorption edge of STO:Nix relative to NiO was found to be 1.1 eV. The present work investigates the differences in the structure of STO:Nix prepared by magnetron deposition method with different dopant amount settings. At the same time, the difference in structure was observed when prepared under vacuum with Ar working gas and when O2 was flowed through the deposition chamber. The premise of this experiment was to verify the formation of oxygen vacancies in the STO structure on which the photocatalytic phenomenon could occur.