Since carbon molecules with geodesic structures have been detected, the que
stion for potential silicon-based analogues of these species has been raise
d. The existence of these hypothetical 'silicon balls', however, has not be
en ascertained so far in spite of several theoretical as well as experiment
al attempts to do so. Several theoretical approaches have been put forward
in the past to explain the experimentally observed features of Si-N cluster
s and thus to account for the obvious dissimilarity between finite systems
based on the isovalent elements silicon and carbon, but no comprehensive gr
owth sequence model has been generally accepted for Si-N so far.
The present work is aimed at an exploration of closed-shell Si-N systems, d
erived from highly symmetric cage-like geometries, in the size range N less
than or equal to 26 by means of Hartree-Fock and post-Hartree-Fock procedu
res. Particular emphasis is placed on the question of the stabilities of th
ese isomers as compared to the corresponding ground states, wherever availa
ble. Cohesive energy calculations suggest a tendency towards an increase of
cluster stability with the number of constituents for cage-like Si-N isome
rs up to N = 10, while a trend towards destabilization with growing size is
found for larger clusters. (C) 1998 Elsevier Science B.V. All rights reser
ved.