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Spintronics
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A Different Spin on Future Data Storage
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| The
next generation of computers will be "instant-on,"
meaning they won't need to be booted up to move hard-drive
data into memory. They'll also store data in a smaller
space and access it faster, while consuming less power
than today's machines — thanks in part to the development
of magnetic random access memory chips, or MRAM. These
MRAM chips will store data through the spin of electrons,
giving them a distinct advantage over today's chips,
which utilize electron charge. |

MRAM computer chips use magnetization rather than
electric charges to store bits of data; they can
retain information even when electrical power is
turned off. The world's first 16-megabit MRAM chip
from Infineon Technologies and IBM research set
records for high-density data storage in 2004.
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| Before
the "spintronics" revolution can begin, however,
a much better scientific understanding is needed of
complex metal oxide materials that display the unique
phenomenon called colossal magnetoresistance (CMR),
including the materials known as manganites.
"With CMR manganites, the application
of a magnetic field can cause the material's electrical
resistance to change by as much as 1,000 percent,"
says Charles Fadley, a physicist affiliated with Berkeley
Lab's Materials Sciences Division and a professor
of physics at the University of California at Davis.
"Today's best data storage devices are based
on the GMR effect" — gigantic magnetoresistance
— "in which the field application reduces the
electrical resistance only 20 to 50 percent."
Fadley, working with his student Norman
Mannella, now at Stanford University, used the exceptionally
bright, soft x-ray beams (lower energy x-rays) and
sophisticated experimental facilities of Berkeley
Lab's Advanced Light Source (ALS) to shed new light
on what could prove to be a crucial element of the
CMR effect in manganites and other metal oxides. This
is the surprising formation of a type of polaron,
an electron that is somehow bound to a local distortion
of the atoms in the crystal.
The distortion creates a sort of energy
"well" that traps the electron, like a divot
on a fairway that traps a golf ball. The type of polaron
that Fadley and Mannella detected is called a Jahn-Teller
polaron, after Hans Jahn and Edward Teller (the same
Teller who later led development of the hydrogen bomb),
who predicted such polaron distortions in a famous
1937 paper. Fadley and Mannella found that Jahn-Teller
polaron formation took place in the CMR manganite
only after it was heated past its Curie temperature,
the point at which a material ceases to be magnetic.
"We've shown for the first time,
using a combination of all of the primary ALS spectroscopies,
that one of the most studied of the CMR manganites,
a mixture of lanthanum, strontium, manganese, and
oxygen, exhibits the formation of polarons above its
Curie temperature" of about 350 degrees Kelvin,
Fadley says. "The combination of ALS techniques
we used showed much more directly than any previous
measurements that one electron is localized to the
magnetic manganese atoms, thus altering the electrical
resistance of the entire material."
Manganites typically contain four
or more constituents; manganese is often the only
magnetic atom present. According to the findings of
Fadley and Mannella, as the CMR manganites cool to
below their Curie temperature, the Jahn-Teller polarons
disappear, releasing the trapped electrons. The ability
of the CMR manganites to conduct electricity is very
different depending on whether or not a polaron is
present.
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Watching
electrons move in a spintronic material; lanthanum
strontium manganese oxide:
(Left
panel) Two electrons in an inner shell of a manganese
atom have slightly different energies, resulting from
the interactions of their spins with the spin of the
atom as a whole. In this graph, made by plotting the
energy of electrons knocked out of the shell by photons
from the ALS beamline, their energy separation at
different temperatures (adjacent curves) appears as
a trench-like feature. The separation increases as
the temperature goes above the Curie point (blue line)
and keeps increasing until no more separation is apparent
(red line). When the temperature is decreased, the
process reverses. The energy separation of these electrons
is a direct measure of the atom's magnetic strength,
which increases markedly above the Curie point due
to the transfer of an electron to the manganese atom.
(Right panel) Meanwhile, the electrons in the innermost
orbital shell of oxygen atoms in the compound simultaneously
shift to a higher energy as temperature is raised,
confirming the transfer of charge to the manganese
atom above the Curie temperature. (Lanthanum and strontium
in the compound show graphs similar to oxygen.) These
results provide direct evidence of "polaron"
formation: a distortion in the lattice of atoms surrounding
the manganese atom, which traps an electron in its
vicinity.
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| As
Mannella explains, "Since the manganese atom and
its surrounding oxygen atoms are much more massive than
a bare electron, the polaron behaves as a negatively
charged particle with a larger mass and lower mobility
than an isolated electron."
Adds Fadley, "It seems clear
that to understand CMR in manganites, you will have
to take into account the effects of polarons. As for
the temperature dependence of the polaron formation,
it was much bigger than we ever imagined it would
be."
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4.0.2
of the Advanced Light Source, where they used multiple
spectroscopy techniques to detect the temperature-dependent
formation of Jahn-Teller polarons in manganites, linked
to colossal magnetoresistance (CMR) (Photo Roy Kaltschmidt)
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| The
spectroscopic experiments carried out by Fadley and
Mannella were performed using the multi-technique spectrometer/
diffractometer at ALS Beamline 4.0.2, which generates
circularly polarized soft x-ray beams. A beam of light
is circularly polarized when its electric-field component
rotates around the direction in which the beam is traveling.
The absorption of circularly polarized light by a magnetic
material reveals much about the magnetic moments of
its constituent atoms. Powered by one of the ALS's undulator
magnets, beamline 4.0.2 is ideal for studying manganites
and other materials of spintronic interest.
The CMR effect in manganites is an important subject
of study for reasons other than its potential impact
on high-density data storage devices. Some CMR materials
conduct electricity via electrons with only one direction
of spin (spin is a quantum-mechanical property, considered
to be up or down), rather than equal numbers of electrons
with either direction of spin, as in all of today's
typical electronic devices. This means that CMR manganites
can have nearly 100 percent spin polarization, making
them excellent candidates for lightning-fast new logic
devices, such as spin transistors and magnetic tunneling
transistors.
"Beyond spintronic applications, our results
could also have implications for the magnetic states
of atoms under high pressure, as in the earth's core,"
Mannella says.
Geophysical studies have shown that iron-containing
perovskites, metal-oxide materials with the same general
crystal structure as the CMR manganites, can exhibit
a marked reduction in the electron spin state of their
iron atoms as they move through the earth's mantle
toward conditions of extreme pressure at the earth's
core. From an initial high spin state, the iron atoms
drop to a low spin state as pressure increases. This
leads to a gradual loss of magnetic moment, which
has significant influence on the magnetic, thermoelastic
and transport properties of the deep mantle. It could
also affect the partitioning of iron between the upper
and lower mantle, and between the lower mantle and
core, with a possibility of iron enrichment in the
deep mantle.
"The relationship between
the perovskites in the mantle and pressure is based
on the same effects that we're studying to observe
changes in transition-metal spin [magnetic] states
as a function of pressure and temperature," said
Fadley. "Therefore, our results should be helpful
to those who are developing a model of what the mantle
really looks like."
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| Collaborating
with Fadley and Mannella on this research were Berkeley
Lab's Bongjin Mun, Corwin Booth, Stefano Marchesini,
and See-Hun Yang. The research was funded by the U.S.
Department of Energy, Office of Basic Energy Sciences
(BES), Materials Sciences and Engineering Division.
Contact:
Lynn Yarris, lcyarris@lbl.gov
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This
story has been adapted from a news release -
Diese Meldung basiert auf einer Pressemitteilung -
Deze
tekst is gebaseerd op een nieuwsbericht - |
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