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Volumn 120, Issue 19, 2004, Pages 9286-9296

High density gradients in the (√3 × √3)R30°-CO layer on Ru(0001)

Author keywords

[No Author keywords available]

Indexed keywords

ABSORPTION SPECTROSCOPY; ADSORPTION; BONDING; CARBON MONOXIDE; COMPOSITION; DESORPTION; ELECTRON ENERGY LOSS SPECTROSCOPY; FREQUENCIES; HIGH RESOLUTION ELECTRON MICROSCOPY; INFRARED SPECTROSCOPY; LOW ENERGY ELECTRON DIFFRACTION; MIXTURES; NUCLEAR MAGNETIC RESONANCE; PHASE TRANSITIONS; POINT DEFECTS;

EID: 2942525464     PISSN: 00219606     EISSN: None     Source Type: Journal    
DOI: 10.1063/1.1710852     Document Type: Article
Times cited : (14)

References (45)
  • 24
    • 2942620948 scopus 로고    scopus 로고
    • CO has been kept low in order to stay in the linear regime of spectral changes
    • CO has been kept low in order to stay in the linear regime of spectral changes.
  • 36
    • 2942583546 scopus 로고    scopus 로고
    • note
    • C-O line positions of both isotopic species overlap within about one wave number.
  • 37
    • 2942583437 scopus 로고    scopus 로고
    • note
    • 16O layer, e.g., in Fig. 4(f).
  • 38
    • 2942613546 scopus 로고    scopus 로고
    • note
    • -1) as well as the associated "intensity transfer" will be relatively weak.
  • 43
    • 2942553323 scopus 로고    scopus 로고
    • M. Gsell and P. Jakob (unpublished results)
    • M. Gsell and P. Jakob (unpublished results).
  • 45
    • 2942613547 scopus 로고    scopus 로고
    • note
    • Our IR data related to saturated CO/Ru(0001) layers now exist for about 9 years. So far we restrained from publishing them because there still existed some open questions regarding the structural arrangement of the various species and details of their binding geometry. In order to avoid confusion in the literature and to straighten up a few points related to these layers, we decided to publish them along with a less detailed interpretation of our observations.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.