A main ingredient to model the physics of metallic clusters is the kno
wledge of the spatial and energetic distribution of the atoms. Quenche
d molecular dynamics simulations with interatomic potentials derived f
rom the electronic structure (tight-binding approximation) show that P
d cubo-octahedral and icosahedral clusters undergo an inhomogeneous co
ntraction, restricted to the surface selvedge and, in the latter case,
to the inner core. This wrinkled profile leads to interatomic distanc
es which can be larger than the bulk Pd ones for icosahedral clusters,
whereas they all are smaller for cubo-octahedral clusters. Moreover i
t induces, for the icosahedral shape, the occurrence of a core energy
in the energy profile, which leads to a structural transition from ico
sahedron to cubo-octahedron when the cluster size reaches about 2000 a
toms.