APS March Meeting 2010
Volume 55, Number 2
Monday–Friday, March 15–19, 2010;
Portland, Oregon
Session A33: Focus Session: Magnetization and Spin Dynamics I
8:00 AM–11:00 AM,
Monday, March 15, 2010
Room: E143
Sponsoring
Units:
GMAG DMP
Chair: Michael Flatté, University of Iowa
Abstract ID: BAPS.2010.MAR.A33.8
Abstract: A33.00008 : Ferromagnetic resonance linewidth and damping in perpendicular-anisotropy magnetic multilayers thin films
9:48 AM–10:24 AM
Preview Abstract
Abstract
Author:
Jean-Marc Beaujour
(Department of Physics, New York University)
Transition metal ferromagnetic films with perpendicular magnetic
anisotropy (PMA) have ferromagnetic resonance (FMR) linewidths
that are one order of magnitude larger than soft magnetic
materials, such as pure iron (Fe) and permalloy (NiFe) thin
films. We have conducted systematic studies of a variety of thin
film materials with perpendicular magnetic anisotropy to
investigate the origin of the enhanced FMR linewidths, including
Ni/Co and CoFeB/Co/Ni multilayers. In Ni/Co multilayers the PMA
was systematically reduced by irradiation with Helium ions,
leading to a transition from out-of-plane to in-plane easy axis
with increasing He ion fluence [1,2]. The FMR linewidth depends
linearly on frequency for perpendicular applied fields and
increases significantly when the magnetization is rotated into
the film plane with an applied in-plane magnetic field.
Irradiation of the film with Helium ions decreases the PMA and
the distribution of PMA parameters, leading to a large reduction
in the FMR linewidth for in-plane magnetization. These results
suggest that fluctuations in the PMA lead to a large two magnon
scattering contribution to the linewidth for in-plane
magnetization and establish that the Gilbert damping is enhanced
in such materials ($\alpha \simeq 0.04$, compared to $\alpha
\simeq 0.002$ for pure Fe) [2]. We compare these results to those
on CoFeB/Co/Ni and published results on other thin film materials
with PMA [e.g., Ref. 3].
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[1] D. Stanescu \textit{et al.}, J. Appl. Phys. \textbf{103},
07B529 (2008).
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[2] J-M. L. Beaujour, D. Ravelosona, I. Tudosa, E. Fullerton, and
A. D. Kent, Phys. Rev. B RC \textbf 80, 180415 (2009).
\newline
[3] N. Mo, J. Hohlfeld, M. ulIslam, C. S. Brown, E. Girt, P.
Krivosik, W. Tong, A. Rebel, and C. E. Patton, Appl. Phys. Lett.
\textbf{92}, 022506 (2008).
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*Research done in collaboration with: A. D. Kent, New York
University, D. Ravelosona, Institut d'Electronique Fondamentale,
UMR CNRS 8622, Universit\'{e} Paris Sud, E. E.
Fullerton, Center for Magnetic Recording Research, UCSD, and
supported by NSF-DMR-0706322.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2010.MAR.A33.8