α- and β-phases of Sn thin films grown on GaSb(001) surface by molecular beam epitaxy
ORAL
Abstract
Tin (Sn) is known to show distinct phases depending on temperature and pressure. The cubic α-Sn is stable below 13.7 C for bulk (higher for thin films), while tetragonal β-Sn is well known metallic phase present at room temperature and shows superconductivity at 3.7 K. Recently, Sn is gaining interest as a unique and promising candidate because of various topological phases of α-Sn by tuning strain, orientation, and thickness configurations as well as excellent superconducting features of β-Sn for quantum devices. We investigate Sn thin films with different α- and β-phases on GaSb(001) surface using molecular beam epitaxy with active liquid Nitrogen cooling as well as by first-principles calculations. We observed β-Sn(110), β-Sn(001), and α-Sn(110) phases with varying growth temperatures for the same film thickness (40 nm). Transport measurement revealed superconductivity for β-Sn(001) phase whereas no superconductivity and large weak localization-like features were seen down to 0.04 K for β-Sn(110) phase. We also study the crystal structure with temperature-dependent Raman spectroscopy. This work highlights a strong connection among novel electronic phases and structure metastability that is critical for controlling the topological and superconducting nature of Sn.
*This work was supported by the Science Alliance at the University of Tennessee, Knoxville, thorough the Support for Affiliated Research Teams program and the U. S. Department of Energy (DOE), Office of Science, Basic Energy Sciences (BES), Materials Sciences and Engineering Division.
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Presenters
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Anjali Rathore
- University of Tennessee