We have used the Stillinger-Weber potential to calculate the interacti
on energy between pairs of missing dimer vacancies (MDVs) on the Si(11
0) surface. We have found that there is a long-range repulsion between
two MDVs located in the same dimer row, and a slight attraction betwe
en MDVs in adjacent rows. The results have been used to model the coll
ective equilibrium properties of ensembles of vacancies. At low temper
ature and high concentration the vacancies self-organize into long wav
y lines perpendicular to the dimer rows. When heated, these lines brea
k up to form a ''gas'' of short nearly linear aggregates consisting of
several vacancies. At an even higher temperature the vacancies tend t
o form pairs which serve as nuclei for the formation of ''vacancy isla
nds''.