The origin of the observed perpendicular magnetic anisotropy (PMA) in
Ni/Cu(001) for thick Ni layers is investigated using the ab initio ful
l potential linearized augmented plane wave method. With the aid of th
e state tracking and torque approaches, very stable results are obtain
ed for the magnetocrystalline anisotropy (MCA) energies for both the N
i/Cu(001) overlayer systems and the distorted bulk fct Ni. We find tha
t the PMA is due mainly to the strain induced bulk contribution rather
than to interfacial hybridization. The calculated value of the bulk M
CA energy, 65 mu eV/atom, is very close to recent experimental data ex
trapolated to zero temperature, 70 mu eV/atom. (C) 1997 American Insti
tute of Physics.