The kagome metal FeSn consists of alternating layers of kagome-lattice FeSn and honeycomb Sn and exhibits great potential for applications in future low-energy electronics and spintronics because of an ideal combination of topological phases and high-temperature magnetic ordering. Robust synthesis methods for ultrathin FeSn films, as well as an understanding of their air stability, are crucial for its development and long-term operation in future devices. In this work, we realize large-area, <10 nm thick, epitaxial FeSn thin films and explore the oxidation process synchrotron-based photoelectron spectroscopy using oxygen and water dosing, as well as air exposure. Upon exposure to the atmosphere, the FeSn films are shown to be highly reactive, with a stable ∼3 nm thick oxide layer forming at the surface within 10 min. Notably, the surface Fe remains largely unoxidized when compared with Sn, which undergoes near-complete oxidation. Additionally, the band structure remains metallic under oxygen exposure. These are further confirmed with controlled dosing of O and HO, where only the Sn (stanene) interlayers within the FeSn lattice oxidize, suggesting the FeSn kagome layers remain almost pristine. These results are in excellent agreement with first-principles calculations, which show that Fe-O bonds to the FeSn layer are energetically unfavorable and a large formation energy preference of 1.37 eV for Sn-O bonds in the stanene Sn layer over Sn-O bonds in the kagome FeSn layer. The demonstration that oxidation only occurs within the stanene layers and the preservation of the Dirac bands may provide additional avenues in how to engineer, handle, and prepare future kagome metal devices.

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http://dx.doi.org/10.1021/acsnano.4c08600DOI Listing

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