TY - JOUR
T1 - Fe Chalcogenides by X-ray Photoemission Spectroscopy
AU - Shimada, Kenya
AU - Mizokawa, Takashi
AU - Mamiya, Kazutoshi
AU - Saitoh, Tomohiko
AU - Fujimori, Atsushi
AU - Kamimura, Takashi
N1 - Publisher Copyright:
© 2000 American Vacuum Society.
PY - 1999/10/1
Y1 - 1999/10/1
N2 - In this article, x-ray photoelectron spectroscopy (XPS) spectra of iron chalcogenides, FeS, Fe7S8, and Fe7Se8 are presented. FeS (troilite) and Fe7S8 (pyrrhotite) are among the most common iron compounds on earth. FeS is antiferromagnetic below the Néel temperature of TN=593-598 K. Above Tα=420 K, FeS is a metal with an NiAs-type crystal structure, but becomes an insulator with a narrow band gap of 0.04 eV below Tα. This transition known as the α-transition is accompanied by a small displacement of the Fe and S atoms from the regular NiAs-type structure. Fe7S8 and Fe7Se8 are ferrimagnetic metals with Néel temperatures of TN=578 and 423-460 K, respectively. The crystal structures of Fe7S8 and Fe7Se8 are derived from the NiAs-type one by introducing ordered Fe vacancies. The polycrystalline samples were synthesized by the Bridgman method. Clean surfaces were obtained by scraping in situ with a diamond file. All the XPS spectra of the iron chalcogenides are taken at room temperature.
AB - In this article, x-ray photoelectron spectroscopy (XPS) spectra of iron chalcogenides, FeS, Fe7S8, and Fe7Se8 are presented. FeS (troilite) and Fe7S8 (pyrrhotite) are among the most common iron compounds on earth. FeS is antiferromagnetic below the Néel temperature of TN=593-598 K. Above Tα=420 K, FeS is a metal with an NiAs-type crystal structure, but becomes an insulator with a narrow band gap of 0.04 eV below Tα. This transition known as the α-transition is accompanied by a small displacement of the Fe and S atoms from the regular NiAs-type structure. Fe7S8 and Fe7Se8 are ferrimagnetic metals with Néel temperatures of TN=578 and 423-460 K, respectively. The crystal structures of Fe7S8 and Fe7Se8 are derived from the NiAs-type one by introducing ordered Fe vacancies. The polycrystalline samples were synthesized by the Bridgman method. Clean surfaces were obtained by scraping in situ with a diamond file. All the XPS spectra of the iron chalcogenides are taken at room temperature.
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U2 - 10.1116/1.1247931
DO - 10.1116/1.1247931
M3 - Article
AN - SCOPUS:71149093926
SN - 1055-5269
VL - 6
SP - 321
EP - 336
JO - Surface Science Spectra
JF - Surface Science Spectra
IS - 4
ER -