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Condensed Matter > Superconductivity

arXiv:2501.17451 (cond-mat)
[Submitted on 29 Jan 2025 (v1), last revised 28 Mar 2025 (this version, v2)]

Title:Enhancement of superconductivity on thin film of Sn under high pressure

Authors:Misaki Sasaki, Masahiro Ohkuma, Ryo Matsumoto, Toru Shinmei, Tetsuo Irifune, Yoshihiko Takano, Katsuya Shimizu
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Abstract:We investigated the pressure effects of a superconductivity on thin films of Sn. Elemental superconductor Sn with a body-centered tetragonal structure, $\beta$-Sn, exhibits superconductivity below the superconducting transition temperature ($T_{\rm c}=3.72$ K) at ambient pressure. $T_{\rm c}$ of Sn increases with lowering dimension such as in thin film and nanowire growth, or by high-pressure application. For thin films, $T_{\rm c}$ exhibits a slight increase up to approximately 4 K compared to the bulk value, attributable to the crystalline size and lattice disorder. By applying pressure on a bulk Sn, $T_{\rm c}$ initially decreases from 3.72 K as the pressure increases. Further increasing pressure up to 10 GPa, $T_{\rm c}$ increases to 5.3 K with the structural transformation. However, the combination of these effects on thin films of Sn, namely, thin-film growth and pressure effects, remains underexplored. In this study, we combined film-growth and pressure-application techniques to further increase $T_{\rm c}$ using a diamond anvil cell with boron-doped diamond electrodes. The drop of the electrical resistance suggesting the onset of $T_{\rm c}$ on the thin film reached above 6 K in $\gamma$-Sn phase. Further, the upper critical magnetic field was drastically enhanced. Atomic force microscopy suggests that the refinement of the grain size of the thin film under the non-hydrostatic pressure conditions contributes to stabilizing the higher $T_{\rm c}$ of $\gamma$-Sn.
Subjects: Superconductivity (cond-mat.supr-con)
Cite as: arXiv:2501.17451 [cond-mat.supr-con]
  (or arXiv:2501.17451v2 [cond-mat.supr-con] for this version)
  https://doi.org/10.48550/arXiv.2501.17451
arXiv-issued DOI via DataCite
Journal reference: Phys. Rev. B 111, 104513 (2025)
Related DOI: https://doi.org/10.1103/PhysRevB.111.104513
DOI(s) linking to related resources

Submission history

From: Masahiro Ohkuma [view email]
[v1] Wed, 29 Jan 2025 07:14:14 UTC (1,535 KB)
[v2] Fri, 28 Mar 2025 01:54:04 UTC (1,490 KB)
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