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Surface entropy of rare-gas clusters
Abundances of Ar N + and Xe N + clusters produced in a supersonic expansion source are inverted to find relative dissociation energies. The values around the shell and subshell closings at N = 55 , 71, and 147 differ from theoretical values derived from ground-state energies of Lennard-Jones cluster...
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Published in: | The Journal of chemical physics 2005-08, Vol.123 (8), p.084317-084317-10 |
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Main Authors: | , , , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | Abundances of
Ar
N
+
and
Xe
N
+
clusters produced in a supersonic expansion source are inverted to find relative dissociation energies. The values around the shell and subshell closings at
N
=
55
, 71, and 147 differ from theoretical values derived from ground-state energies of Lennard-Jones clusters. A significant part of the difference can be accounted for by the conformational entropies of surface atoms and vacancies. |
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ISSN: | 0021-9606 1089-7690 |
DOI: | 10.1063/1.2008948 |