論文

2019年12月

Electronic structure of Au-Sn compounds grown on Au(111)

PHYSICAL REVIEW B
  • Pampa Sadhukhan
  • ,
  • Sajal Barman
  • ,
  • Tufan Roy
  • ,
  • Vipin Kumar Singh
  • ,
  • Shuvam Sarkar
  • ,
  • Aparna Chakrabarti
  • ,
  • Sudipta Roy Barman

100
23
記述言語
英語
掲載種別
研究論文(学術雑誌)
DOI
10.1103/PhysRevB.100.235404
出版者・発行元
AMER PHYSICAL SOC

The electronic structure of Au-Sn intermetallic layers of different compositions grown on Au(111) to the thickness of several nanometers has been studied in this paper. The layer, the interface, and the substrate related components in the Au 4f and Sn 4d core-level spectra obtained using x-ray photoelectron spectroscopy (XPS) vary with deposition parameters to reveal the details of the Au-Sn formation. While AuSn is grown by deposition at room temperature, Au rich compounds form as a result of heat treatment through interdiffusion of Au and Sn. Deposition at high temperature forms more Au rich compositions compared to postannealing at the same temperature due to the kinetic energy of the impinging Sn atoms in the former case. Postannealing, on the other hand, stabilizes the bulk phases such as AuSn and Au5Sn and exhibits an activated behavior for transition from the former to the latter with increasing temperature. The XPS valence-band spectra of AuSn and Au5Sn layers show good agreement with the density functional theory calculation, indicating that these have the bulk structure reported in literature. However, the influence of antisite defects is observed in Au5Sn. Low-energy electron-diffraction study reveals that although the AuSn layer is ordered its top surface is disordered at room temperature. Surface order is obtained by annealing or deposition at elevated temperatures and dispersing bands are observed by angle-resolved photoemission spectroscopy. Both electronlike and holelike bands are evident for the (root 3 x root 3)R30 degrees phase, while a nearly free electronlike parabolic surface state is observed for the p(3 x 3)R15 degrees phase.

リンク情報
DOI
https://doi.org/10.1103/PhysRevB.100.235404
Web of Science
https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=JSTA_CEL&SrcApp=J_Gate_JST&DestLinkType=FullRecord&KeyUT=WOS:000500717500002&DestApp=WOS_CPL
ID情報
  • DOI : 10.1103/PhysRevB.100.235404
  • ISSN : 2469-9950
  • eISSN : 2469-9969
  • Web of Science ID : WOS:000500717500002

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