Exchange bias can be understood qualitatively by
a simple model. In an external field and above the Néel temperature
(TN), antiferromagnetic spins located at the interface with the
ferromagnet are aligned, like the ferromagnet, with the field. Once
cooled below TN, these interface spins thereafter keep their orientation
and appear "pinned" because they are tightly locked to
the spin lattice in the bulk of the antiferromagnet, which is not
sensitive to external fields. Consequently these pinned spins produce
a constant magnetic field at the interface that causes the hysteresis
loop of the ferromagnet to shift. However, this intuitive picture
overestimates the magnitude of the loop shift by orders of magnitude.
Exchange bias. The hysteresis loop of a ferromagnet in contact
with an antiferromagnet shifts after cooling in an external field
to a temperature below the Néel temperature (field-cooling),
so that one magnetization direction becomes preferred.
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Numerous efforts have been made to explain the difference,
but the problem has been the missing knowledge about the actual
spin structure at the interface, which need not be the same as in
the bulk. The goal of the collaboration was to detect pinned interfacial
spins and use the information to find a direct correlation between
their number and the size of the loop shift. The unique ability
of x-ray magnetic circular dichroism (XMCD) to probe magnetic properties
of individual elements in thin-film samples was the key to success.
Hysteresis loops of cobalt (top) and manganese (bottom)
in an exchange-biased layer of ferromagnetic cobalt on antiferromagnetic
iridium/manganese. The loops for both elements shift, with the
direction (red and blue) of the shift depending on the
sample geometry. In addition, there is a vertical shift between
the manganese loops. Both shifts are due to a small fraction of
pinned spins at the interface.
For this purpose, the researchers used elliptically polarizing
undulator (EPU) Beamline 4.0.2 at the ALS to measure hysteresis
loops of interfacial spins in samples comprising thin layers of
exchange-biased ferromagnetic cobalt or cobalt–iron on thicker
layers of antiferromagnetic iridium–manganese, platinum–manganese,
or nickel oxide, all on silicon substrates. In each case, they measured
hysteresis loops in two sample orientations that gave loop shifts
parallel and anti-parallel to the positive field direction, respectively.
By tuning the photon energy to the manganese or nickel absorption
edges, they detected the extremely small XMCD signal arising only
from the interfacial spins in the antiferromagnet (there is no signal
from the antiferromagnet itself). These hysteresis loops exhibit
a vertical shift in addition to the horizontal shift. Like the preferred
magnetization direction, the vertical shift reverses if the sample
geometry is reversed.
Left, in an ideal, single-crystal antiferromagnet (green),
all spins at the smooth interface (red arrows) are pinned
and contribute in the same way to the internal field acting on
the top ferromagnetic layer (blue).
Right, in a real sample with a rough interface (horizontal
gray) and grain boundaries (vertical gray), most
spins at the interface (white arrows) are not pinned
and follow the magnetization of the ferromagnet. The small number
of pinned spins (red arrows) causes exchange bias.
Two important conclusions follow from the interface hysteresis
loops. First of all, most of the interfacial spins couple strongly
to the ferromagnet on top and follow its magnetization, thereby
exhibiting the same hysteretic behavior. Second, only a small fraction
(5%) of interfacial spins is actually pinned, and these cause the
horizontal hysteresis loop shifts. In addition, the vertical shift
is caused by these pinned interfacial spins, which were aligned
by the cooling field and remain pointing in a fixed direction. The
very small number of pinned spins observed explains why it was not
possible to detect these spins with conventional magnetometry techniques.
Furthermore, it shows that the simple model for exchange bias is
correct in principle, if one assumes "mixed coupling"
across an imperfect antiferromagnetic/ferromagnetic interface instead
of ideal interfaces. A next-generation photoemission electron microscope
(PEEM-3) coming to the ALS will clarify the origin of the pinning.
Research conducted by H. Ohldag (Stanford Synchrotron Radiation
Laboratory, ALS, and Universität Düsseldorf); A. Scholl,
E. Arenholz, and A.T. Young (ALS); F. Nolting (Swiss Light Source);
S. Maat and M. Carey (Hitachi Global Storage Technologies); and
J. Stöhr (Stanford Synchrotron Radiation Laboratory).
Research funding: U.S. Department of Energy, Office of Basic Energy
Sciences (BES). Operation of the ALS is supported by BES.
Publication about this research: H. Ohldag, A. Scholl, F. Nolting,
E. Arenholz, S. Maat, A.T. Young, M. Carey, and J. Stöhr, "Correlation
between exchange bias and pinned interfacial spins," Phys.
Rev. Lett. 91, 017203 (2003).
ALSNews
Vol. 240, April 28, 2004 |