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タイトル: Negative ionic states of tin in the oxide superconductor Sr3−xSnO revealed by Mössbauer spectroscopy
著者: Ikeda, Atsutoshi  kyouindb  KAKEN_id  orcid https://orcid.org/0000-0002-9345-2967 (unconfirmed)
Koibuchi, Shun
Kitao, Shinji
Oudah, Mohamed
Yonezawa, Shingo  kyouindb  KAKEN_id  orcid https://orcid.org/0000-0002-7476-3604 (unconfirmed)
Seto, Makoto
Maeno, Yoshiteru
著者名の別形: 池田, 敦俊
鯉渕, 駿
北尾, 真司
米澤, 進吾
瀬戸, 誠
前野, 悦輝
発行日: 15-Dec-2019
出版者: American Physical Society (APS)
誌名: Physical Review B
巻: 100
号: 24
論文番号: 245145
抄録: We report the temperature variation of the ¹¹⁹Sn-Mössbauer spectra of the antiperovskite (inverse perovskite) oxide superconductor Sr₃₋ₓ SnO. Both superconductive (Sr deficient) and nonsuperconductive (nearly stoichiometric) samples exhibit major γ-ray absorption with an isomer shift similar to that of Mg₂ Sn. This fact shows that Sr₃-ₓ SnO contains the metallic anion Sn⁴⁻, which is rare, especially among oxides. In both samples, we observed another γ-ray absorption with a larger isomer shift, indicating that there is another ionic state of Sn with a higher oxidation number. The temperature dependence of the absorption intensities reveals that the Sn ions exhibiting larger isomer shifts have a lower energy of the local vibration. The larger isomer shift and lower vibration energy are consistent with the values estimated from the first-principles calculations for hypothetical structures with various Sr-deficiency arrangements. Therefore, we conclude that the additional γ-ray absorptions originate from the Sn atoms neighboring the Sr deficiency.
著作権等: ©2019 American Physical Society
許諾条件に基づいて掲載しています。
URI: http://hdl.handle.net/2433/250418
DOI(出版社版): 10.1103/PhysRevB.100.245145
出現コレクション:学術雑誌掲載論文等

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