X-ray scattering as a probe of magnetic order in rare-earth

X-ray scattering as a probe of magnetic order in rare-earth compounds k′ εσ ε1 επ θf ε2 επ ε3 θi k εσ The Advanced Photon Source You are here 6...
Author: Edwina French
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X-ray scattering as a probe of magnetic order in rare-earth compounds k′ εσ ε1

επ θf

ε2

επ ε3 θi

k εσ

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6-ID-A

6-ID-D

6-ID-B

6-ID-C

MUCAT Main Undulator Line

Outline • Resonant and nonresonant magnetic scattering • Polarization dependence – Magnetic moment directions

• An example: GdNi2Ge2 – Magnetic structure and transitions – AFM domain imaging – Magnetic powder diffraction

• Summary

k′ εσ ε1

επ θf

ε2

επ ε3 θi

k εσ

Solving magnetic structures • Determine the magnetic wavevector (what is the “magnetic unit cell”) • Determine the magnetic moment directions • Determine the magnitude of the ordered magnetic moment.

Long-range order

Bragg peaks QBragg=2π/d τ = 2π/2d

I 1

τ

τ 10-6

2d d 2π/d

Q

X-ray Magnetic Scattering For nonresonant scattering we directly probe the “magnetic electrons

L3 - edge

For resonant scattering:

EF

•(L2, L3)-edge for rare-earths (610KeV) •Electric multipole transition (E1: 2p – 5d, E2: 2p – 4f) • 4f : magnetic properties 5d : exchange splitting by 4f outgoing photon

Incoming photon

P3/2 P1/2

f

res el

=



λ

∑ [εˆ′ L

*

M =− L

() () ]

* ⋅ YLM kˆ′ YLM kˆ′ ⋅ εˆ FLM (ω )

TbNi2B2C

Nonresonant scattering ……. Scattering from the unpaired magnetic electrons (e.g. 4f electrons for rare earth elements)

f

res el

=



λ

∑ [εˆ′ L

*

M =− L

() () ]

* ⋅ YLM kˆ′ YLM kˆ′ ⋅ εˆ FLM (ω )

analyzer

Angular dependence and polarization properties

sample

k′ εσ ε1

επ ε 3 θf

ε2

επ θi

k εσ

σ→σ σ→π π→σ π→π

fe1res = 0 ^ fe1res ~ k′ ·M ^ fe1res ~ -k ·M ^ fe1res ~ (k′ X k)·M

Magnetic moment direction Discrimination of charge scattering

Resonant scattering amplitude Relating the magnitude of the resonant scattering to the details of the resonant processes • Atomic models vs. solid state effects • SOC in 5d bands • CEF effects

We still have a lot of work to do!!

FIG. 1 Schematic view of scattering geometries (a) σ to π geometry (b) π to σ geometry

We can do this by plotting the q-dependence of integrated intensities (a la neutrons) Angular dependence of the scattering at (0 0 L ± τ) of GdCo2Ge2 measured by resonant and nonresonant diffraction

Gd L3 edge

X-ray resonant magnetic scattering azimuth scans

Q Gd5Ge4 θ

θ

f

i

k

Gd5Ge4 (0 3 0) at T = 8 K

Orthorhombic structure with moments along the b-axis

Integrated Intensity (arb. unit.)

k '

Intensity ∝ |k' • M|2

1.0

0.5

bc in scattering plane 0.0

0

30

ab in scattering plane 60

90

120

Azimuth Ψ (deg.)

bc in scattering plane 150

180

GdNi2Ge2 – An Example Crystal structure

Magnetization measurement Tt

TN

Gd Ni Ge

S.L. Bud’ko, Z. Islam, T.A. Wiener, I.R. Fisher, A.H. Lancerda, P.C. Canfield Journal of Magnetic Materials 205, 53 (1999)

Magnetic and charge satellite peaks

Second transition β=~0.409 (0 0 6+τ)

A(1-T/ TN)2β

(0 0 4+2τ)

B(1-T/ TN)4β

(0 0 8+3τ)

C(1-T/ TN)6β

Modulation vector τ Lattice parameter c

But… fitting the angular and azimuth dependence of the scattering to extract the moment direction never quite worked! Issue: We presume that our samples consist of small multiple domains Let’s shrink the incident beam size and look again.

One single magnetic domain T < Tt

Tt < T < TN

Q

Q

T < Tt

15 K Tt < T < TN

17 K

Q : magnetic modulation vector direction

Imaging Antiferromagnetic domains of GdNi2Ge2 by X-ray resonant magnetic scattering

How to get the images Scattered X-ray

Sample Beam Size

0.1 mm

0.1 mm

Incoming X-ray

0.1 mm

0.05 mm

How to get the images Scattered X-ray Beam Size Incoming X-ray

0.1 mm

0.05 mm

How to get the images Scattered X-ray Beam Size Incoming X-ray

0.1 mm

0.05 mm

How to get the images Scattered X-ray Beam Size Incoming X-ray

0.1 mm

0.05 mm

(a)

0.2mm

10K

Beam direction

(b) 3.5 2.8 2.1 1.4 7.0 0

17K

Beam direction

(c)

3

1

17K

Beam direction

(d)

2

Beam direction

(e)

(f) Normalized Intensity

17K

4 3 2 1 0 4 3 2 1 0 4 3 2 1 0 0

1 2 3 45 90 135 180 225 270 315 360

Azimuth angle ψ (degree)

What happens if you don’t have the slightest idea where to look for the magnetic peak, or if there can be more than one magnetic wavevector? • Powder Diffraction! – Problem is that the resonant scattering crosssection is still tiny w.r.t. charge and fluorescence scattering.

Magnetic powder diffraction from UO2 • Resonant scattering length at the U M4 edge is a significant fraction (0.2%) of charge scattering. • U-edge energies don’t allow a broad coverage of reciprocal space. • Resonant scattering at the R L-edges is a thousand times smaller! not possible!

The Challenge • Signal-to-Noise – Scattering from the sample – Fluorescence from the sample – General background (scattering from everything else) For Si (333) at the Gd L2-edge: analyzer

sample

cos2 2θanalyzer = 9 x 10-4 ΔE/E ~ 10-4 Reduce background and fluorescence to ~ 1ct /sec

The Result

Good agreement between measured peak integrated intensities and the magnetic structure determined from single crystal studies

Why Bother? •

Many of the technologically important RE compounds contain neutron opaque elements. • Superior reciprocal space (Q) resolution allows more detailed study … reinvestigation of “solved” structures. • Can be used for investigations of submillimeter-sized single crystals. • Resonant magnetic scattering occurs at well-defined energies specific to elements of interest -- probe local magnetism. • Studies of magnetic surfaces and interfaces.

Harmonics for collinear and spiral structures Diffraction Pattern ≈ Fourier transform of the charge (magnetic) distribution

Collinear structure

Spiral structure

“A limited menu of choices”

1.5

1.5

1

1

0.5

0.5

0

0 0

5

10

15

0

-0.5

-0.5

-1

-1

-1.5

-1.5

5

10

15

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