D.
Fenske, Paloma Sevillano, T. Langetepe, N. Zhu
There
are a number of metal chalcogenide ions known in the gas phase. Examples are
[Cu2n+1En]- (E: S, Se), [Ag2n+1Sn]-
and [NixSy]- clusters. Obviously it is
possible to stabilize these species with protecting PR3 ligands. Ab
initio calculations show that the influence of the tertiary PR3
ligands depends on the cluster size and type of the PR3 ligand used.
An easy route to such compounds is via the reaction of transition metal halides
with silylated derivatives of S and Se. Examples are [Cu12Se6(Pr3)8],
[Cu20Se10(PR3)8], [Cu26Se13(PR3)14],
[Cu30Se15(PR3)12], [Cu44Se22(PR3)12],
[Cu48Se22(PR3)20], [Cu59Se30(PR3)15],
[Ag112Se32(SeBu)48(PBu3)12],
[Ag172Se40(SeBu)92(dppp)4] and many
other clusters. During the last time we were also able to
synthesize Au Clusters with up to 90 Au atoms. Examples
are ionic clusters like: [Au10Se4(dppe)4Br2],
[Au18Se8(dppe)6Br2], [Au34Se14(tpep)6(tpepSe)2Cl6].
These compounds show interesting photophysical
properties. These materials may be regarded as sections cut out of the
structure of binary phases which are effectively shielded by an envelope of PR3
ligands. The structures, properties and results from ab initio calculations
will be reported. The conductivity is strongly dependent on the cluster size.
Under high vacuum conditions the PR3 ligands can be removed from the
cluster surface. This results in the formation of an amorphous nano composite
material. The size of the particles is between 3.0 to 5.0 nm with a very narrow
size.