The connection between granular gases and sticky gases has recently been co
nsidered, leading to the conjecture that inelastic collapse is avoided for
space dimensions higher than 4. We report Molecular Dynamics simulations of
hard inelastic spheres in dimensions 4, 5 and 6. The evolution of the gran
ular medium is monitored throughout, the cooling process. The behaviour is
found to be very similar to that of a two-dimensional system, with a sheari
ng-like instability of the velocity field and inelastic collapse when colli
sions are inelastic enough, showing that the connection with sticky gases n
eeds to be revised.