Probing the structural, electronic and magnetic properties of AgnSc (n = 1-16) clusters
The structural, electronic and magnetic properties of Ag n Sc ( n = 1-16) clusters have been studied on the basis of density functional theory and the CALYPSO structure prediction method. The optimized geometry exhibits that the growth process of Sc-doped silver clusters have a periodic structural c...
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Published in | Physical chemistry chemical physics : PCCP Vol. 2; no. 23; pp. 15824 - 15834 |
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Main Authors | , , , , |
Format | Journal Article |
Language | English |
Published |
Cambridge
Royal Society of Chemistry
01.01.2018
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Subjects | |
Online Access | Get full text |
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Summary: | The structural, electronic and magnetic properties of Ag
n
Sc (
n
= 1-16) clusters have been studied on the basis of density functional theory and the CALYPSO structure prediction method. The optimized geometry exhibits that the growth process of Sc-doped silver clusters have a periodic structural change. The Ag atom grows around a basically invariant cluster core in each growth cycle. The Sc atom has a tendency to occupy the most highly coordinated position in the ground state. The infrared spectra, Raman spectra and photoelectron spectra of Ag
n
Sc clusters are forecasted and can be used to identify the structures of these clusters from experiments. The global maxima of the dissociation energy, the averaged binding energy and the gap of the energy level occur at
n
= 15 for the most stable Ag
n
Sc clusters, implying that the Ag
15
Sc can be perceived as a superatom. The magnetism analysis indicates that the magnetic moment of the Sc atom in Ag
n
Sc clusters decreases with the increase of the cluster. The change of the magnetic moment is proportional to the charge transfer between the Sc and Ag atoms.
The structural, electronic and magnetic properties of Ag
n
Sc (
n
= 1-16) clusters have been studied on the basis of density functional theory and the CALYPSO structure prediction method. |
---|---|
Bibliography: | ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 23 |
ISSN: | 1463-9076 1463-9084 |
DOI: | 10.1039/c8cp02605j |