THICKNESS DEPENDENCE OF THE TOTAL MAGNETIC-MOMENT PER ATOM IN THE CU NI/CU/SI(001) SYSTEM/

Citation
S. Hope et al., THICKNESS DEPENDENCE OF THE TOTAL MAGNETIC-MOMENT PER ATOM IN THE CU NI/CU/SI(001) SYSTEM/, Physical review. B, Condensed matter, 55(17), 1997, pp. 11422-11431
Citations number
40
Categorie Soggetti
Physics, Condensed Matter
ISSN journal
01631829
Volume
55
Issue
17
Year of publication
1997
Pages
11422 - 11431
Database
ISI
SICI code
0163-1829(1997)55:17<11422:TDOTTM>2.0.ZU;2-U
Abstract
Systematic measurements of the magnetic moment per Ni atom in Cu/Ni/Cu /Si(001) structures have been made using polarized neutron reflection (PNR) for Ni thicknesses in the range 30 Angstrom < t < 400 Angstrom a t room temperature. We find a dramatic reduction in the magnetic momen t per atom for t < 100 Angstrom and near bulk values above 100 Angstro m. These results are corroborated by alternating gradient magnetometer measurements on the same samples. A Cu/Ni-wedge/Cu/Si(001) structure with 30 Angstrom < t < 150 Angstrom was studied using magnetic circula r x-ray dichroism (MCXD), polar magneto-optical Kerr effect (MOKE), an d reflection high-energy electron diffraction (RHEED) in order to esti mate the variation in the values of (L-z), (S-z), perpendicular anisot ropy strength, and surface in-plane Ni lattice constant, respectively, during epitaxial growth. RHEED measurements show that the in-plane la ttice constant falls by 1.7% in the Ni thickness range 30 Angstrom < t < 90 Angstrom. The MCXD measurements reveal the same trend for (L-z), (S-z), and total moment per atom versus Ni thickness as found for the total moment by PNR. Polar MOKE measurements confirmed the transition from a perpendicular easy axis towards an in-plane magnetic easy axis as has already been extensively studied in the literature. Comparison of the PNR results with RHEED measurements reveal a striking correlat ion between the increase of in-plane strain and reduction in magnetic moment per atom with decreasing Ni thickness. While a direct strain-in duced variation of the moment based on bulk phase calculations cannot account for the magnitude of the moment variations we observe, we show that the results cannot be attributed to sample contamination, interd iffusion, or a reduction of the Curie temperature with decreasing Ni t hickness. Furthermore, the presence of a magnetically dead layer in th e samples is not consistent with the PNR results. The strong moment va riation partially explains the large thickness range for which perpend icular anisotropy is observed in this system.