Spin-integrated and spin-resolved photoemission study of Fe chalcogenides
Physical Review B - Condensed Matter and Materials Physics Volume 57 Issue 15
Page 8845-8853
published_at 1998-04-15
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Title ( eng ) |
Spin-integrated and spin-resolved photoemission study of Fe chalcogenides
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Creator |
Mizokawa Takashi
Mamiya Kazutoshi
Saitoh Tomohiko
Fujimori Atsushi
Ono Kanta
Kakizaki Akito
Ishii Takehiko
Shirai Masafumi
Kamimura Takashi
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Source Title |
Physical Review B - Condensed Matter and Materials Physics
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Volume | 57 |
Issue | 15 |
Start Page | 8845 |
End Page | 8853 |
Abstract |
The electronic structures of the antiferromagnetic semiconductor FeS and ferrimagnetic metals Fe7S8 and Fe7Se8 have been studied by spin-integrated and spin-resolved photoemission spectroscopy and inverse-photoemission spectroscopy. The overall Fe 3d bandwidth in the photoemission spectra is 25-30 % narrower than the density of states (DOS) predicted by first-principles band-structure calculations and is accompanied by an intense tail on the high-binding-energy side, indicating the correlated nature of electrons in the Fe 3d band. Deviation from the band DOS is more significant in Fe7S8 than in Fe7Se8, and in the minority-spin spectra than in the majority-spin spectra. Cluster-model calculation for FeS has shown satellite structures at high binding energies, but the calculated spectral line shape is not in good agreement with experiment compared to the band DOS. By introducing a self-energy correction to the band DOS, we could explain the narrowing of the overall Fe 3d bandwidth and the high-binding-energy tail shape but not for the unusual broadening of the Fe 3d band within ∼ 1 eV of the Fermi level.
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Language |
eng
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Resource Type | journal article |
Publisher |
American Physical Society
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Date of Issued | 1998-04-15 |
Rights |
Copyright (c) 1998 The American Physical Society.
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Publish Type | Version of Record |
Access Rights | open access |
Source Identifier |
[ISSN] 0163-1829
[DOI] 10.1103/PhysRevB.57.8845
[NCID] AA11187113
[DOI] http://dx.doi.org/10.1103/PhysRevB.57.8845
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