Epitaxial stannate pyrochlore thin films: Limitations of cation stoichiometry and electron doping

Felix V. E. Hensling, Diana Dahliah, Prabin Dulal, Patrick Singleton, Jiaxin Sun, Jürgen Schubert, Hanjong Paik, Indra Subedi, Biwas Subedi, Gian-Marco Rignanese, Nikolas J. Podraza, Geoffroy Hautier, and Darrell G. Schlom

We have studied the growth of epitaxial films of stannate pyrochlores with a general formula A2Sn2O7 (A = La and Y) and find that it is possible to incorporate  25% excess of the A-site constituent; in contrast, any tin excess is expelled. We unravel the defect chemistry, allowing for the incorporation of excess A-site species and the mechanism behind the tin expulsion. An A-site surplus is manifested by a shift in the film diffraction peaks, and the expulsion of tin is apparent from the surface morphology of the film. In an attempt to increase La2Sn2O7 conductivity through n-type doping, substantial quantities of tin have been substituted by antimony while maintaining good film quality. The sample remained insulating as explained by first-principles computations, showing that both the oxygen vacancy and antimony to tin substitutional defects are deep. Similar conclusions are drawn on Y2Sn2O7. An alternative n-type dopant, fluorine on oxygen, is shallow according to computations and more likely to lead to electrical conductivity. The bandgaps of stoichiometric La2Sn2O7 and Y2Sn2O7 films were determined by spectroscopic ellipsometry to be 4.2 eV and 4.48 eV, respectively.

Growth Data
ItemTypeFile
MBE Raw Growth Files - 48 sampleszipped folderGrowthData.zip
La2Sn2-xSbxO7 RHEED Data
ItemTypeFile
Sample 4tifFH004_end_green.tif
Sample 5pngFH05_right_angle.png
Sample 5pngFH005end.png
Sample 5tifImage13.tif
Sample 6tifFH006_end.tif
Sample 7tifFH007_end_green.tif
Sample 13tifFH088_end_green.tif
Sample 13tifFH088_end.tif
Sample 14bmpendFH089.bmp
Sample 14pngendFH089.png
Sample 15pngEnd.png
Sample 16tifFH091_end.tif
Sample 29bmpFH104.bmp
La2Sn2-xSbxO7 XRD Data
ItemTypeFile
Sample 3csv2ThetaOmega27_33.csv
Sample 3csv5_75_XRD.csv
Sample 3csvFH003_2ThetaOmega_57_67.csv
Sample 9csvFH022_2Theta_Omega_5_75.csv
Sample 9csvFH022_2Theta_Omega_25_35.csv
Sample 9csvFH022_2Theta_Omega_57_67.csv
Sample 9PNG41_85.PNG
Sample 13csvFH088_rocking_better.csv
Sample 13csvFH088_rocking_final.csv
Sample 13csvFH088_rocking_new.csv
Sample 13csvFH088_rocking.csv
Sample 14PNG44_2nm.PNG
Sample 14csvFH089_2ThetaOmega_5_75.csv
Sample 14csvRocking_222_0_0997.csv
Sample 14csvXRR Quick Pixel_29.csv
Sample 15csvFH090_2ThetaOmega_5_75.csv
Sample 16csvFH091_2ThetaOmega_10_70.csv
Sample 22csvFH097_2ThetaOmega_24_60.csv
Sample 29csvFH104_2ThetaOmega_10_70.csv
Sample 31csvFH106_2ThetaOmega_10_70.csv
Y2Sn2-xSbxO7 RHEED Data
ItemTypeFile
Sample 7bmpFH114end.bmp
Sample 7pngEndYSO1h.png
Sample 9bmpfh116END.bmp
Sample 9pngFH116END2.png
Sample 11pngFH152_RHEED.png
Sample 12pngFH153_13_285.png
Sample 13pngFH154_20_630.png
Sample 14pngFH155_32_000.png
Sample 15pngFH156_2_19_043.png
Sample 16bmpFH157_end.bmp
Sample 16pngFH157_end.png
Sample 16tifFH157_end.tif
Y2Sn2-xSbxO7 XRD Data
ItemTypeFile
Sample 1csvFH108_2ThetaOmega_10_70.csv
Sample 2csvFH109_2ThetaOmega_10_70.csv
Sample 3csvFH110_2ThetaOmega_10_70.csv
Sample 7csvfh114_2tHETAoMEGA_5_75.csv
Sample 8PNG43_62.PNG
Sample 9csvFH116_2ThetaOmega_10_70.csv