Abstract
While cubic to tetragonal phase transition at 105 K is well characterized in SrTiO3, the influence of dopants on the phase transition temperature remains an active area of research. For cation substitution, the phase transition temperature is dopant-dependent and generally linear with respect to the Goldschmidt tolerance factor. Whether this trend continues with anion substitution or oxygen vacancies has not been studied as much. In this work, we explore the impact of anion substitution by characterizing an oxyhydride, where the oxide anion of the parent SrTiO3 phase is partially replaced by hydride (H-) and anion site vacancies. We present the structural changes associated with the phase transition in hydride-doped STO by utilizing Inelastic Neutron Scattering (INS), phonon simulations, and high-resolution X-Ray Diffraction (XRD). By performing INS and phonon simulations, we demonstrate that at low hydride content, there is a preference for hydride to occupy the apical site of the tetragonal cell, while at higher hydride contents the two sites have similar occupations. Using high-resolution XRD from 11 BM at Argonne, we characterize the relationship between phase transition temperature and hydride content. This work will establish whether anion substitution results in qualitatively different phase transition behavior than cation substitution in doped SrTiO3, setting the stage for assessing the relative roles of anion and cation chemistry more broadly.
*This work was supported as part of the Hydrogen in Information and Energy Sciences (HEISs) Center, an Energy Frontier Research Center funded by the U.S. Department of Energy, Office of Science, Basic Energy Sciences under Award # DE-SC0023450. This research used resources at the SNS, a DOE Office of Science User Facility operated by the Oak Ridge National Laboratory, the National Energy Research Scientific Computing Center (NERSC), a Department of Energy Office of Science User Facility using NERSC award BES-ERCAP0032806 and the Advanced Photon Source at Argonne National Laboratory was supported by the U. S. Department of Energy, Office of Science, Office of Basic Energy Sciences, under Contract No. DE-AC02-06CH11357.