TY - JOUR
T1 - Perpendicular magnetic anisotropy of multilayers
T2 - recent insights
AU - Johnson, M. T.
AU - Jungblut, R.
AU - Kelly, P. J.
AU - den Broeder, F. J.A.
PY - 1995/7/1
Y1 - 1995/7/1
N2 - Extending our understanding of perpendicular magnetic anisotropy (PMA) beyond the phenomenological approach of volume (KV) and interface anisotropies (KS) requires caution. Experimentally, many factors such as roughness, formation of interface alloys, or patchiness of ultrathin layers may cause a reduction in PMA. Where stresses are present in multilayer growth, these may, under particular circumstances, contribute to both KV and KS, as demonstrated for the Cu/Ni/Cu system. Theoretically, the difficulty in modelling incoherently grown materials prevents a detailed quantitative comparison with most experimental systems, so that an evaluation of the underlying approximations common to all of the quantitative theoretical studies becomes very difficult.
AB - Extending our understanding of perpendicular magnetic anisotropy (PMA) beyond the phenomenological approach of volume (KV) and interface anisotropies (KS) requires caution. Experimentally, many factors such as roughness, formation of interface alloys, or patchiness of ultrathin layers may cause a reduction in PMA. Where stresses are present in multilayer growth, these may, under particular circumstances, contribute to both KV and KS, as demonstrated for the Cu/Ni/Cu system. Theoretically, the difficulty in modelling incoherently grown materials prevents a detailed quantitative comparison with most experimental systems, so that an evaluation of the underlying approximations common to all of the quantitative theoretical studies becomes very difficult.
UR - http://www.scopus.com/inward/record.url?scp=0029341761&partnerID=8YFLogxK
U2 - 10.1016/0304-8853(95)00174-3
DO - 10.1016/0304-8853(95)00174-3
M3 - Article
AN - SCOPUS:0029341761
SN - 0304-8853
VL - 148
SP - 118
EP - 124
JO - Journal of magnetism and magnetic materials
JF - Journal of magnetism and magnetic materials
IS - 1-2
ER -