Modulating the magneto-transport properties of epitaxial SrRuO<sub>3</sub> (111) thin films by controlling the defects
POSTER
Abstract
(111) oriented perovskite transition metal-oxide is believed to host topological states due to their buckled honeycomb lattice structure1. Further, SrRuO3 (SRO) films along (111) are predicted to have emergent phases such as Haldane’s quantum Hall state even without the presence of any magnetic field2. In this regard, we have grown high-quality epitaxial SRO thin films using the RHEED-assisted PLD on atomically terminated SrTiO3 (111). These films are characterized using XRD, magnetic, and magnetoresistance (MR) /Hall transport studies.
We have investigated the dependency of the Residual Resistivity Ratio (RRR) on the transport properties of SRO. Although the variation of RRR has a minimal effect on the magnetic properties, its influence is found to be prominent on the transport regime. Films grown under different deposition conditions show a systematic change in RRR, but no such systematic correlation with the MR data, like the reports in the literature. We have observed an unusually high positive MR and a consistent Hall transport study in the ultra-thin films of (111) oriented SRO, which are promising for future studies on this Weyl semimetal candidate.
1D. Xiao et. al Nat. Commun. 2, 596 (2011).
2L. Si et. al PRL 119, 026402 (2017).
We have investigated the dependency of the Residual Resistivity Ratio (RRR) on the transport properties of SRO. Although the variation of RRR has a minimal effect on the magnetic properties, its influence is found to be prominent on the transport regime. Films grown under different deposition conditions show a systematic change in RRR, but no such systematic correlation with the MR data, like the reports in the literature. We have observed an unusually high positive MR and a consistent Hall transport study in the ultra-thin films of (111) oriented SRO, which are promising for future studies on this Weyl semimetal candidate.
1D. Xiao et. al Nat. Commun. 2, 596 (2011).
2L. Si et. al PRL 119, 026402 (2017).
*DST, INDIA Nano MissionINSPIRE Faculty Fellowship, DST, INDIA
Presenters
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Santosh K Khetan
- Indian Institute of Science