ログイン
Language:

WEKO3

  • トップ
  • ランキング
To
lat lon distance
To

Field does not validate



インデックスリンク

インデックスツリー

メールアドレスを入力してください。

WEKO

One fine body…

WEKO

One fine body…

アイテム

  1. 学術雑誌論文
  2. 4 自然科学

Comparison of Ab initio Low-Energy Models for LaFePO, LaFeAsO, BaFe2As2, LiFeAs, FeSe, and FeTe: Electron Correlation and Covalency

http://hdl.handle.net/10228/00008755
http://hdl.handle.net/10228/00008755
b83bbbed-ac4a-452c-887b-08d4c3845607
名前 / ファイル ライセンス アクション
JPSJ.79.044705.pdf JPSJ.79.044705.pdf (4.0 MB)
アイテムタイプ 学術雑誌論文 = Journal Article(1)
公開日 2022-03-08
資源タイプ
資源タイプ識別子 http://purl.org/coar/resource_type/c_6501
資源タイプ journal article
タイトル
タイトル Comparison of Ab initio Low-Energy Models for LaFePO, LaFeAsO, BaFe2As2, LiFeAs, FeSe, and FeTe: Electron Correlation and Covalency
言語
言語 eng
著者 Miyake, Takashi

× Miyake, Takashi

WEKO 32604

Miyake, Takashi

Search repository
中村, 和磨

× 中村, 和磨

WEKO 20202
e-Rad 60525236
Scopus著者ID 47961309100
九工大研究者情報 100000601

en Nakamura, Kazuma

ja 中村, 和磨

ja-Kana ナカムラ, カズマ


Search repository
Arita, Ryotaro

× Arita, Ryotaro

WEKO 32606

Arita, Ryotaro

Search repository
Imada, Masatoshi

× Imada, Masatoshi

WEKO 32607

Imada, Masatoshi

Search repository
抄録
内容記述タイプ Abstract
内容記述 Effective low-energy Hamiltonians for several different families of iron-based superconductors are compared after deriving them from the downfolding scheme based on first-principles calculations. Systematic dependences of the derived model parameters on the families are elucidated, many of which are understood from the systematic variation of the covalency between Fe-3 d and pnictogen-/chalcogen- p orbitals. First, LaFePO, LaFeAsO (1111), BaFe 2 As 2(122), LiFeAs (111), FeSe, and FeTe (11) have overall similar band structures near the Fermi level, where the total widths of 10-fold Fe-3 d bands are mostly around 4.5 eV. However, the derived effective models of the 10-fold Fe-3 d bands (d model) for FeSe and FeTe have substantially larger effective onsite Coulomb interactions U ∼4.2 and 3.4 eV, respectively, after the screening by electrons on other bands and after averaging over orbitals, as compared to ∼2.5 eV for LaFeAsO. The difference is similar in the effective models containing p orbitals of As, Se or Te(d p or d p p model), where U ranges from ∼4 eV for the 1111 family to ∼7 eV for the 11 family. The exchange interaction J has a similar tendency. The family dependence of models indicates a wide variation ranging from weak correlation regime (LaFePO) to substantially strong correlation regime (FeSe). The origin of the larger effective interaction in the 11 family is ascribed to smaller spread of the Wannier orbitals generating larger bare interaction, and to fewer screening channels by the other bands. This variation is primarily derived from the distance h between the pnictogen/chalcogen position and the Fe layer: The longer h for the 11 family generates more ionic character of the bonding between iron and anion atoms, while the shorter h for the 1111 family leads to more covalent-bonding character, the larger spread of the Wannier orbitals, and more efficient screening by the anion p orbitals. The screened interaction of the d model is strongly orbital dependent, which is also understood from the Wannier spread. The d p and d p p models show much weaker orbital dependence. The larger h also explains why the 10-fold 3 d bands for the 11 family are more entangled with the smearing of the “pseudogap” structure above the Fermi level seen in the 1111 family. While the family-dependent semimetallic splitting of the bands primarily consists of d y z / d z x and d x 2 - y 2 orbitals, the size of the pseudogap structure is controlled by the hybridization between these orbitals and d x y / d 3 z 2 - r 2 : A large hybridization in the 1111 family generates a large “band-insulating”-like pseudogap ( hybridization gap ), whereas a large h in the 11 family weakens them, resulting in a “half-filled” like bands of orbitals. This may enhance strong correlation effects in analogy with Mott physics and causes the orbital selective crossover in the three orbitals. On the other hand, the geometrical frustration t '/ t, inferred from the ratio of the next-nearest transfer t ' to the nearest one t of the d model is relatively larger for the 1111 family than the 11 one. The models comprehensively derived here may serve as a firm starting basis of understanding both common and diverse properties of the iron-based superconductors including magnetism and superconductivity.
書誌情報 Journal of the Physical Society of Japan

巻 79, 号 4, p. 044705-1-044705-20, 発行日 2010-03-25
出版社
出版者 日本物理学会
DOI
関連タイプ isIdenticalTo
識別子タイプ DOI
関連識別子 https://doi.org/10.1143/JPSJ.79.044705
日本十進分類法
主題Scheme NDC
主題 427
NCID
収録物識別子タイプ NCID
収録物識別子 AA00704814
ISSN
収録物識別子タイプ ISSN
収録物識別子 1347-4073
ISSN
収録物識別子タイプ ISSN
収録物識別子 0031-9015
著作権関連情報
権利情報 Copyright (c) 2010 The Author(s). This article is published by the Physical Society of Japan under the terms of the Creative Commons Attribution 4.0 License. Any further distribution of this work must maintain attribution to the author(s) and the title of the article, journal citation, and DOI.
キーワード
主題Scheme Other
主題 first-principles calculation
キーワード
主題Scheme Other
主題 effective Hamiltonian
キーワード
主題Scheme Other
主題 downfolding
キーワード
主題Scheme Other
主題 constrained RPA method
キーワード
主題Scheme Other
主題 LaFePO
キーワード
主題Scheme Other
主題 LaFeAsO
キーワード
主題Scheme Other
主題 BaFe2As2
キーワード
主題Scheme Other
主題 LiFeAs
キーワード
主題Scheme Other
主題 FeSe
キーワード
主題Scheme Other
主題 FeTe
キーワード
主題Scheme Other
主題 oxypnictide
キーワード
主題Scheme Other
主題 oxychalcogenide
キーワード
主題Scheme Other
主題 high-temperature superconductivity
出版タイプ
出版タイプ VoR
出版タイプResource http://purl.org/coar/version/c_970fb48d4fbd8a85
査読の有無
値 yes
研究者情報
URL https://hyokadb02.jimu.kyutech.ac.jp/html/100000601_ja.html
連携ID
値 10169
戻る
0
views
See details
Views

Versions

Ver.1 2023-05-15 13:02:09.076843
Show All versions

Share

Share
tweet

Cite as

Other

print

エクスポート

OAI-PMH
  • OAI-PMH JPCOAR 2.0
  • OAI-PMH JPCOAR 1.0
  • OAI-PMH DublinCore
  • OAI-PMH DDI
Other Formats
  • JSON
  • BIBTEX
  • ZIP

コミュニティ

確認

確認

確認


Powered by WEKO3


Powered by WEKO3