Although strain engineering provides
a unique opportunity to dramatically
alter the properties of various oxides, precise determination of the
crystalline structure of the strained thin films is not a straightforward
experimental task. Fortunately, the situation can be improved by combining
experimental efforts with theoretical modeling. In this work, we present
a first-principles investigation of the crystalline structure of tensile
strained SrRuO3 thin film grown in the (110) orientation
on the DyScO3 substrate. Previous experimental findings
suggest that investigated SrRuO3 thin film prefers Cmcm or I4/mmm space group
symmetry; however, our systematic analysis based on energetic and
geometric considerations reveals that P21/m symmetry with its tilt system a
+
b
–
c
– is the most favorable one among 15 octahedral
rotation patterns inherent for perovskites. The results of performed
modeling indicate the need for low-temperature crystalline data in
order to ensure a more accurate comparison between experiment and ab initio calculations.