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j.physb.2017.10.089.pdf8.49 MBAdobe PDF見る/開く
タイトル: Theoretical band structure of the superconducting antiperovskite Sr₃₋ₓ SnO
著者: Ikeda, Atsutoshi,
Fukumoto, Toshiyuki
Oudah, Mohamed
Hausmann, Niklas Jan
Yonezawa, Shingo  kyouindb  KAKEN_id  orcid https://orcid.org/0000-0002-7476-3604 (unconfirmed)
Kobayashi, Shingo
Sato, Masatoshi  kyouindb  KAKEN_id
Tassel, Cedric  kyouindb  KAKEN_id  orcid https://orcid.org/0000-0002-8867-4813 (unconfirmed)
Takeiri, Fumitaka
Takatsu, Hiroshi  kyouindb  KAKEN_id  orcid https://orcid.org/0000-0001-5792-0113 (unconfirmed)
Kageyama, Hiroshi  kyouindb  KAKEN_id
Maeno, Yoshiteru
著者名の別形: 池田, 敦俊
米澤, 進吾
佐藤, 昌利
高津, 浩
陰山, 洋
前野, 悦輝
キーワード: Superconductivity
Antiperovskite oxide
Inverse perovskite oxide
First-principles band calculation
発行日: 1-May-2018
出版者: Elsevier BV
誌名: Physica B: Condensed Matter
巻: 536
開始ページ: 752
終了ページ: 756
抄録: In order to investigate the position of the strontium deficiency in superconductive Sr₃₋ₓ SnO, we synthesized and measured X-ray-diffraction patterns of Sr₃₋ₓ SnO (x ~ 0.5). Because no clear peaks originating from superstructures were observed, strontium deficiency is most likely to be randomly distributed. We also performed first-principles band-structure calculations on Sr₃₋ₓ SnO (x = 0, 0.5) using two methods: full-potential linearized-augmented plane-wave plus local orbitals method and the Korringa-Kohn-Rostoker Green function method combined with the coherent potential approximation. We revealed that the Fermi energy of Sr₃₋ₓ SnO in case of x ~ 0.5 is about 0.8 eV below the original Fermi energy of the stoichiometric Sr₃SnO, where the mixing of the valence p and conduction d orbitals are considered to be small.
著作権等: © 2018. This manuscript version is made available under the CC-BY-NC-ND 4.0 license http://creativecommons.org/licenses/by-nc-nd/4.0/.
The full-text file will be made open to the public on 1 May 2020 in accordance with publisher's 'Terms and Conditions for Self-Archiving'.
This is not the published version. Please cite only the published version.
この論文は出版社版でありません。引用の際には出版社版をご確認ご利用ください。
URI: http://hdl.handle.net/2433/250419
DOI(出版社版): 10.1016/j.physb.2017.10.089
出現コレクション:学術雑誌掲載論文等

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