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ALS EXPERIMENTAL SYSTEMS GROUP : : THE EXCHANGE BIAS STORY The Exchange Bias Story Introduction X-ray Dichroism LaFeO 3 NiO

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ALS EXPERIMENTAL SYSTEMS GROUP : : THE EXCHANGE BIAS STORY

The Exchange Bias Story

Introduction

X-ray Dichroism

LaFeO3

NiO

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ALS EXPERIMENTAL SYSTEMS GROUP : : THE EXCHANGE BIAS STORY

Magnetic Materials in Information Technology

Magnetic thin films are key components of non-volatile storage technologies:

• Magnetic Random Acess Memory (MRAM)

• Magnetic Hard Disk

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ALS EXPERIMENTAL SYSTEMS GROUP : : THE EXCHANGE BIAS STORY

Cut Through A GMR Read Head

Cut through a modern G(iant)-M(agneto)-R(esistence) read sensor used in disk drives. The sensor consists of two ferromagnetic layers, separated by a non-magnetic spacer. One of the ferromagnets is “exchange-biased” or “pinned” by an antiferromagnet.

10 nm

120 nm

AntiferromagnetPinned Ferromagnet

Non-Magnetic SpacerSoft Ferromagnet

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ALS EXPERIMENTAL SYSTEMS GROUP : : THE EXCHANGE BIAS STORY

Cut Through A GMR Read Head

10 nm

120 nm

Antiferromagnet Non-Magnetic Spacer

I

The resistance of the multilayer to the flow of an electrical current is used to read magnetic information on the disk.

Pinned Ferromagnet Soft Ferromagnet

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ALS EXPERIMENTAL SYSTEMS GROUP : : THE EXCHANGE BIAS STORY

The Giant-Magneto-Resistance Effect (GMR)

High ResistanceLow Resistance

The magnetic stray field of opposing bits when the read head flies over the hard disk changes the magnetization in the free layer (purple). The red layer is pinned by the antiferromagnet and serves as a magnetic reference. The according change in resistance because of the Giant-Magneto-Resistance Effect (GMR) is electronically measured.

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ALS EXPERIMENTAL SYSTEMS GROUP : : THE EXCHANGE BIAS STORY

Antiferromagnets & Exchange Bias

[1 0 0 ]

[0 0 1 ]

[0 1 0 ]

Meiklejohn & Bean, Phys. Rev. 102, 1956

Antiferromagnets have no macroscopic magnetization and are therefore not sensitive to magnetic fields. Spins are magnetically ordered on two or more sub-lattices (red and blue dots), which exactly compensate each other magnetically.

The magnetic structure of NiO

When a ferromagnet is brought in contact with an antiferromagnet, a peculiar effect occurs after heating the structure in a magnetic field. The magnetization of the ferromagnet is held by the antiferromagnet, it is pinned, usually in the direction of the field applied during the heating procedure. This effect is called exchange bias.

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ALS EXPERIMENTAL SYSTEMS GROUP : : THE EXCHANGE BIAS STORY

Exchange Bias—An Interface Effect

ideal AFM poly AFM

Assume that the antiferromagnet grows in layers which have opposite magnetization (left). The exchange coupling between the surface layer of the antiferromagnet (red arrows) and the ferromagnet would create a large pinning field: exchange bias.

In reality the interface is less ideal (right), the surface of the antiferromagnet is usually compensated, steps, grain boundaries and domain walls interrupt the smooth surface.

In these more complex systems exchange bias is believed to be a consequence of uncompensated spins that occur at these defects of the ideal surface.

To understand the origin of exchange bias, the microscopic structure of the ferromagnet and the antiferromagnet at the interface have to be known. This requires a technique, which is sensitive to ferromagnets and antiferromagnets and reaches very high spatial resolution, sufficient to resolve the surface domain structure of the antiferromagnet. X-ray spectromicroscopy techniques like PEEM are ideal for this task.

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ALS EXPERIMENTAL SYSTEMS GROUP : : THE EXCHANGE BIAS STORY

X-ray Absorption Spectroscopy (XAS)

Energy

EF

~~hν X rays

core level

valenceband

2p 3/2

2p1/2

I

X-ray transmission

Electron yield

Sample current

500 600 700 800 900NiFeMnO

Inte

nsity

(a.u

.)Photon energy (eV)

640 645 650 655

710 715 720 725

The absorption spectrum shows distinct edges for each element in the sample and a fine structure near the edge (NEXAFS—Near Edge X-ray Absorption Fine Structure), which contains information about the chemical state of the atom.

Absorbed x rays transfer their energy and momentum to core electrons, which are lifted into unoccupied valence or vacuum states. The new core hole decays in a cascade of secondary emission that is monitored by measuring the sample current or the electron yield, which are proportional to the absorption cross-section.

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ALS EXPERIMENTAL SYSTEMS GROUP : : THE EXCHANGE BIAS STORY

X-ray Magnetic Circular Dichroism

X-rays that are circularly polarized preferentially excite electrons of one spin in the presence of strong spin-orbit splitting. In magnetic materials these polarized electrons probe the occupation of the exchange split valence band. The absorption is higher when electrons are preferentially excited into minority states.

The XMCD spectrum of magnetic transition metals Fe, Co, Ni, which is the difference of two spectra acquired with left- and right-handed circular polarization, shows 2 peaks of opposite sign at the L3 (A) and the L2 (B) edge. The total area is proportional to the spin moment of the material, the difference is proportional to the orbital moment.

The strength of the dichroism is also dependent on the angle between the x-ray polarization and the magnetization:

XMCD spectrum

).,M(cosm ~ I σ∠rr

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ALS EXPERIMENTAL SYSTEMS GROUP : : THE EXCHANGE BIAS STORY

X-ray Magnetic Linear Dichroism

In antiferromagnets, the magnetization is compensated, the magnetic circular dichroism therefore vanishes. However, a magnetic axis is often determined by the orientation of the spins. Using linearly polarized x-rays the direction of this axis and the size of the magnetization per atom can be sensed in the near edge x-ray absorption fine structure, as demonstrated for NiO.

The strength of the dichroism is quadratic in the moment m and dependent on the angle between the linear x-ray polarization and the antiferromagnetic axis: ( ).)E,A(3cos-1m ~ I 22 rr

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X-ray Spectromicroscopy of Antiferromagnets

F. Nolting et al., Nature 2000

s

XMCDCoL3 /L2

775 780 785 790 795 800

L2

L3

Photon energy (eV)

TEY

(a.u

.)

Co

705 710 715 720 725 730

TEY

(a.u

.)

Photon energy (eV)

720 722 724 726

BA

LaFeO3

E

LaFeO3B/A

XMLD

Using a Photoemission Electron Microscope, X-ray Magnetic Circular and Linear Dichroism (XMCD & XMLD) allows us to image the microscopic domain structure of ferromagnets and antiferromagnets and to study the magnetic coupling between the materials.

Ferromagnet

Antiferromagnet

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Antiferromagnetic Structure of LaFeO3

c

11 μm

c

TEM XMLD

Bi-crystal

[100]

[010]

LaFeO3

45°

A

cc

A. Scholl et al., Science 2000

E

Domain imaging of an antiferromagnetic thin film was for the first time demonstrated on a LaFeO3 film grown by molecular beam epitaxy on a SrTiO3 (001) bi-crystal. Sub-micron-size domains are visible when the crystallographic axes, the antiferromagnetic axes and the linear polarization are aligned.

From domain images and spectroscopy a model of the structure was developed. Comparison with TEM images of the same sample (different area) suggest that the antiferromagnet domains coincide with crystallographic twin domains.

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Temperature Dependence of Domain Contrast

290K

565K

490K

290K

2 μm 300 400 500 600 7000.0

0.2

0.4

0.6

0.8

bulk

1st run back to RT 2nd run back to RT

Nor

mal

ized

XM

LD C

ontra

st

Temperature [K]

Fit: TN = 670 K

A. Scholl et al., Science 2000

The loss of magnetic order approaching the Néel temperature is visualized in temperature-dependent XMLD images. The contrast vanishes significantly below the Néel tenperature of the bulk material, extrapolated from the measured data by fitting a mean- field curve. This reduction is either a finite-size or a structural effect in a thin film.

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Co/LaFeO3 Exchange Coupling

LaFeO3

Co Co domain switching

LaFeO3Local loops

-223 Oe 92 Oe

103 Oe 223 Oe

XMCD

XMLD

[100]

[010]

10 mm-200 -100 0 100 200

Field (Oe)

1 2

12

F. Nolting et al., Nature 2000

In a Co/LaFeO3 bi-layer, the Co domains (top) are pinned by antiferromagnetic LaFeO3 domains (bottom). The coupling is parallel.

A horizontal loop shift in local Co hysteresis loops demonstrates a local exchange bias. The loops were measured by analyzing the domain switching in Co XMCD images after applying field pulses of increasing amplitude. A bias of random amplitude and direction is expected for a sample that was not field-annealed.

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Local Exchange Bias

+30 Oe

-30 Oe

-60 -40 -20 0 20 40 600

2

4

6

8

10 1st run 2nd run 3rd run

Dom

ain

area

[μm

2 ]

Bias field (Oe)

0 1 2 3 4 50

10

20

30

40

Domain Area (μm2)

()

0.5 1.0 1.5 2.0 2.5 3.0

8

10

12

14

Bia

s - σ

(Oe)

Diameter-1 (μm-1)

Bias field distribution

The domain area dependence of the local bias field of a large number of Co domains is shown. Bias and domain area were obtained by image analysis from bias field maps (top right). A color coding is used to show the local exchange bias.

The bias field increases inversely linearly with decreasing domain diameter, demonstrating a statistical origin of exchange bias.

Bias map

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NiO

NiO(001)

NiO(001)Co

E

[100][010]

Ohldag et al., PRL 2001

Ni XMLD

Co XMCDNi XMLD

Magnetic moments in NiO crystal are antiferromagnetically ordered with spin axes along <211> directions. The antiferromagnetic axes rotate into the sample plane along <110>, when Co is deposited onto a cleaved crystal..

NiO antiferromagnetic domain images and Co domain images show a parallel coupling of antiferromagnetic and ferromagnetic moments at the interface, similar to the system Co/LaFeO3 .

[1 0 0 ]

[0 0 1 ]

[0 1 0 ]

The magnetic structure of NiO

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Uncompensated Interface Spins

Coferromagnetic

NiO interfaceferromagnetic

NiOantiferromagnetic

XMCDXMCDXMLD

NiO Co

[010]

[100]

E σσ

Ohldag et al., PRL 2001

The Co and NiO domain images show identical ferromagnetic patterns. The uncompensated Ni spins, which amount to less than one monolayer, mediate the coupling between the ferromagnet and the antiferromagnet.

The NiO crystal was rotated such that all antiferromagnetic domains have the same angle to the linear polarization to suppress antiferromagnetic domain contrast. Using circular dichroism, the Co domain pattern and the ferromagnetic pattern of NiO were imaged.

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Hysteresis Loops of Interface Spins

Sample Pinned σE σE (ideal) Jinter

[fraction of layer] [erg/cm2] [erg/cm2] meV3 nm Co/Nio 0.04 0.052 1.3 1.42 nm Co/IrMn 0.041 0.168 4.1 0.51 nm CoFe/PtMn 0.032 0.124 3.9 0.52 nm CoFe/PtMn 0.04 0.193 4.8 0.63nm Co/Fe/PtMn 0.04 0.229 5.7 0.7

Co/NiO Co/IrMn CoFe/PtMn

poly AFM

Ohldag et al., PRL 2003

Using circular dichroism spectroscopy, hysteresis loops were measured of the uncompensated anti- ferromagnetic moments. Most of the uncompensated moments rotate freely with the ferromagnet and are only weakly bound to the antiferromagnet. Some, however, are strongly anchored and can only be rotated by rotation of the sample, giving rise to the observed vertical loop shift between the black and red loops. The density of uncompensated spins explains the observed bias field.