The magnetic anisotropy of 3d-TM clusters is studied in the framework
of a d-electron tight-binding Hamiltonian including hopping, Coulomb,
and spin-orbit interactions on the same electronic level. Results for
the magnetic anisotropy energy and spin-polarized DOS are given as a f
unction of the bond length for the Fe, cluster. In particular it is sh
own that the MAE may be qualitatively related to the projections of th
e orbital moment along the magnetization directions, and that the ''in
-plane'' anisotropy can be of the same order of magnitude as the ''per
pendicular'' anisotropy. Using the same Hamiltonian, the problem of th
e convergence of the magnetic anisotropy energy of very thin films is
revisited. By the choice of a basis which mixes spherical harmonics, i
t is shown that the irregular oscillations of the MAE versus the band
filling disappear. For Co(111) excellent stability of the in-plane ani
sotropy as observed experimentally was found. Finally, the crystal-fie
ld effects are also discussed.