English

Large Rashba spin-orbit coupling in metallic SrTaO$_3$ thin films

Strongly Correlated Electrons 2024-03-20 v1

Abstract

Epitaxial thin films of SrTaO3_3 with thickness (tt) smaller than 74 nm were successfully fabricated on an insulator (LaAlO3_3)0.3_{0.3}(Sr2_2AlTaO6_6)0.7_{0.7} substrate. Films with tt above 8.6 nm showed metallic conduction. Both conductivity and a mobility showed a decrease with increasing tt above 42 nm, suggesting the instability of thick SrTaO3_3 films. This instability was also supported by TEM image and XRD intensity. For the metallic films with tt below 25 nm, energy band splitting due to spin-orbit coupling (Δ\Deltaso_{so}) and Rashba parameter (α\alphaR_R) were deduced from an analysis of a magnetoresistance using two-dimensional weak antilocalization theory. The values of Δ\Deltaso_{so} ranged from 26 to 120 meV, which were the largest among other metallic oxide films, such as SrNbO3_3, SrIrO3_3, and La2/3_{2/3}Sr1/3_{1/3}MnO3_3 thin films, indicating that spin-orbit coupling in SrTaO3_3 was the largest among the metallic perovskite oxides reported so far. The values of α\alphaR_R for our SrTaO3_3 films ranged from 8.8×8.8 \times1013^{-13} to 1.7×1.7 \times1012^{-12} eV m, which were much larger than those reported for other metallic oxide thin films.

Keywords

Cite

@article{arxiv.2403.12612,
  title  = {Large Rashba spin-orbit coupling in metallic SrTaO$_3$ thin films},
  author = {Hikaru Okuma and Yumiko Katayama and Fukunobu Kadowaki and Yuki Tokumoto and Kazunori Ueno},
  journal= {arXiv preprint arXiv:2403.12612},
  year   = {2024}
}

Comments

17 pages, 8 figures

R2 v1 2026-06-28T15:25:33.404Z