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A typical image from a digital camera for x rays
(CCD) showing a soft x-ray speckle pattern. The close-up structure
shows the large intensity variation due to interference of scattered
x rays from different domains.
One conundrum involving the manganites is colossal magnetoresistance,
a hot topic in correlated electron physics with promising applications
in electronics, energy conservation, and nanodevice switching.
Scientifically, this family of materials is also exciting because
of the enormous range of phenomena it exhibits. Charge, orbital,
lattice, and magnetic order are all intertwined to create an array
of patterns, all interrelated in a nontrivial way. Orbital ordering
occurs when specific electron wave functions self-organize.
Interactions between these electron shells determine the patterns
formed by the orbitals and, among other things, will even affect
the system's magnetism.

A cartoon diagram of the orbital ordering is
shown in purple and red, emphasizing the anti-phase domain wall.
Any points where the wave functions are out of phase with each
other can act as an orbital domain boundary.
To perform this study, the researchers used the coherent magnetic
scattering endstation at ALS Beamline
12.0.2, which is specifically designed to deliver "laser-like" x
rays that propagate in unison, like musicians in a marching band.
It includes an 11-flanged vacuum chamber (dubbed the "flangosaurus" after
its resemblance to a prehistoric creature) that allows signal detection
over a broad range of scattering angles.
These coherent x rays are also resonant. This means they
are tuned precisely to a specific absorption edge of a particular
atomic species in the crystal to enhance the sensitivity to the
local environment. In other words, by changing the energy of the
x rays to particular values, they can "see" things that
are invisible at all other energies.
The researchers measured a diffraction peak that is due solely
to the orbital ordering of the d-electron shells in a single crystal
of half-doped manganite, Pr0.5Ca0.5MnO3.
Because of the coherent illumination, constructive and deconstructive
interference occurs between waves scattered from different domains,
and the peak exhibits a "speckle" pattern, a unique characteristic pattern that acts as a fingerprint of the
microscopic domain structure. Just as it is not easy to directly connect
the fingerprint of a person to the face, extracting the domain
structure from the speckle pattern is not straightforward. However,
to better understand the orbital domain physics, one can measure
the dynamics of the domains by noting that any small changes in
this unique speckle pattern indicate changes in the domain configuration,
the same way that a different fingerprint uniquely correlates to
a different person.
Overall, the speckle patterns did not change significantly over time. However, near a transition temperature of about 232 K, small-amplitude fluctuations "turned on" before the domains completely melted. The domain walls are pinned except for close to the transition, where they execute small-amplitude motion. This behavior contrasts with that of most systems, where things usually behave in one of two ways: fluid-like, where everything is dynamic, or solid-like, where everything is static. Here a mixture of the two was found. Another surprising finding was that the fraction of the sample that was dynamic moved quite slowly, slower than typical electron domain behavior in other types of systems. The cause is unclear, but something is impeding the motion of the domain walls, up to a time scale on the order of several minutes. These slow dynamics may even be the reason the manganites form these disordered states in the first place.

Comparisons of adjacent speckle patterns for
different temperatures. Yellow is attributed to speckle patterns
that have not changed, while the other colors indicate that the
speckle—and hence the domain configuration—is changing in time,
with blue the most drastic. Time is represented on the vertical
axis while momentum is on the horizontal.
Research conducted by J.J. Turner (University of Oregon
and ALS), K.J. Thomas and J.P. Hill (Brookhaven National Laboratory),
M.A. Pfeifer (La Trobe University, Australia), K. Chesnel (National
Pulsed Magnetic Field Laboratory [LNCMP], France), Y. Tomioka and
Y. Tokura (National Institute of Advanced Industrial Science and
Technology, Japan), and S.D. Kevan (University of Oregon).
Research funding: U.S. Department of Energy, Office of Basic Energy
Sciences (BES), and the National Science Foundation. Operation
of the ALS is supported by BES.
Publication about this research: J.J. Turner, K.J. Thomas, J.P.
Hill, M.A. Pfeifer, K. Chesnel, Y. Tomioka, Y. Tokura, and S.D.
Kevan, "Orbital
domain dynamics in a doped manganite," New J. Phys. 10,
053023 (2008).
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