Gas-phase copper/selenium and silver/selenium clusters

Binary clusters Cu sub n Se sub m exp + and Ag sub n Se sub m exp + are produced by a gas aggregation source and investigated by time-of-flight mass spectrometry following ionization with a KrF excimer laser. Dominant species in the mass spectra are assigned as (M sub 2 Se) sub n exp + and M(M sub 2...

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Published inChemistry of materials Vol. 5; no. 8; pp. 1085 - 1088
Main Authors Yamada, Y, Deng, H. T, Castleman, A. W
Format Journal Article
LanguageEnglish
Published Washington, DC American Chemical Society 01.08.1993
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Summary:Binary clusters Cu sub n Se sub m exp + and Ag sub n Se sub m exp + are produced by a gas aggregation source and investigated by time-of-flight mass spectrometry following ionization with a KrF excimer laser. Dominant species in the mass spectra are assigned as (M sub 2 Se) sub n exp + and M(M sub 2 Se) sub n exp + (M = copper or silver), which reflect stable compositions of neutral precursors and charged clusters. In these series, magic numbers appear at n = 6. Additionally, especially prominent peaks are observed for M sub n Se sub m exp + ; (n,m) = (7,4), (9,5), and (11,6). From an investigation of the magic numbers and prominent abundances of various species, it is suggested that these binary clusters have structures related to an antifluorite structure.
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ark:/67375/TPS-D7J9G57S-4
ObjectType-Article-2
SourceType-Scholarly Journals-1
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content type line 23
FG02-92ER14258
ISSN:0897-4756
1520-5002
DOI:10.1021/cm00032a010