new p. vavassori - magnetism.eumagnetism.eu/esm/2018/slides/vavassori-slides2.pdf · 2018. 9....
TRANSCRIPT
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
FT-2: Magneto-optics and Magneto-plasmonics Part 1
P. Vavassori
-Ikerbasque, Basque Fundation for Science and CIC nanoGUNE Consolider, San Sebastian, Spain.
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
Outline
Magneto-optics
Brief overview of the Magneto-optical Kerr effects (MOKE)
Advanced MOKE: vector magnetometry
Magnetic nanostructures
micro-MOKE
Approach 1: focused beam
Approach 2: microscopy
MOKE from diffracted beams:
simple theory of diffracted MOKE
in conjunction with micromagnetics and MFM
from magnetometry to magnetic imaging
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
John Kerr1824 - 1907
Michael Faraday1791 - 1867
s
p
s
p
s
p
Reflected Light
z
θ
x
Transmitted Light
Polarization Plane
Sample
The MagnetoOptical Effect
x
z
y
p
s
ps
θ θ
x
z
y
p
s
ps
θ θ
But, what happens if we applied a magnetic field??
→ →
→ →
=
s s p s
s p p p
r rR
r r
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
The Magneto-Optical Effect
→ →
→ →
=
s s p s
s p p p
r rR
r r
xx xy xz
yx yy yz
zx zy zz
x
z
yHy
p
s
ps
θ θ
x
z
y
Hx
p
s
ps
θ θ
Hz
Polar and Longitudinal Configuration Transverse Configuration
Reflectivity matrixDielectric Tensor
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
MOKE
The magneto-optic Kerr effect (MOKE) is widely
used in studying technologically relevant
magnetic materials.
It relies on small, magnetization induced changes
in the optical properties which modify the
polarization or the intensity of the reflected light.
Macroscopically, magneto-optic effects arise from
the antisymmetric, off-diagonal elements in the
dielectric tensor.
sssp
pspp
rr
rrSample
rpp = r0
pp+ rppM my
rps - mx - mzrsp mx-mz
Fresnell reflection coefficients
iTM
rTMpp
E
Er =
iTE
rTMps
E
Er =
iTM
rTEsp
E
Er =
iTE
rTEss
E
Er =
−
−
−
=
0
0
0
ˆ
xy
xz
yz
ii
ii
ii
=
0
0
0
00
00
00
ˆ
x = 0 Q mx; y = 0 Q my; z = 0 Q mz;
• Non-destructive;
• High sensitivity;
• Finite penetration depth (~ 10 nm);
• Fast (time resolved measurements);
• Laterally resolved (microscopy);
• Can be easily used in vacuum and
cryogenic systems;
J. Kerr, Philosophical Magazine 3 321 (1877)Z. Q. Qui and S. D. Bader, Rev. Sci. Instrum. 71, 1243 (2000) P. Vavassori, APL 77 1605 (2000)
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
MOKE origin: classical picture Lorentz force
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
Here, x (r) is the spin-orbit parameter or coupling constant, which depends on the gradient of the electrostatic potential of the nuclear charges.
Its values are of the order of 10-100meV and, thus, the spin-orbit interaction is much weaker than the exchange interaction (≈ 1eV).
Electron theory of Magneto-Optics
Microscopically, the coupling between the electric field of the propagating light and the
electron spin in a magnetic medium occurs through the spin-orbit interaction splitting of
optical absorption lines (Zeeman effect).
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
Electron theory of Magneto-Optics
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
Microscopic origin of Magneto-Optics
s+ and s- Selection rules
Optical transitions between the d-orbitals and the p-orbitals
Only transition from m = 1 to m = 0 are considered for simplicity
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
Microscopic origin of Magneto-Optics
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
Microscopic origin of Magneto-Optics
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
Microscopic origin of Magneto-Optics
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
Microscopic origin of Magneto-Optics
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
Microscopic origin of Magneto-Optics
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
Electron theory of Magneto-Optics
• Magnetization→Splitting of spin-states (Exchange)
– No direct cause of difference of optical response between LCP and RCP
• Spin-orbit interaction→Splitting of orbital states
– Absorption of circular polarization→Induction of circular motion of electrons
• Condition for large magneto-optical response
– Presence of strong (allowed) transitions
– Involving elements with large spin-orbit interaction
– Not directly related with Magnetization
MOKE results from a lifting of orbital degeneracy due to spin-orbit interaction (SOI) in the presence of spontaneous spin polarization.
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
−=
xx
xxxy
xyxx
00
0
0~ xy = i0 Q mz;
( )( )
( ) 0~
2
2
2=
+ E
tcErotrot
0
00
0
0
2
2
=
−
−
−−
z
y
x
zz
xxxy
xyxx
E
E
E
n
n
xyxx in =2
Maxwell Equation
Eigenequation
Eigenvalue Eigenmodes:LCP and RCP
Without off-diagonal terms:No difference between LCP & RCP
( ) ( )tznkieEE −= 00 ( ) 0ˆ2 =−− EEnnE n
A simple case: M || z
Different modes :different speed and attenuation
Therefore, incidentlight becomeselliptically polarizedafter propagation in a MO activematerial
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
Phenomenology of MO effect
Linearly polarized light can be decomposed to LCP and RCP
Difference in phase causes rotation ofthe direction of Linear polarization
Difference in amplitudes makes Elliptically polarized light
In general, elliptically polarized lightWith the principal axis rotated
Different speed(phase lag)
Different attenuation
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
1
220
212
21
20
12
1
sinsin1sin1cos
n
nn
n
n
−=−=−=
rpp = r0
pp+ rppM my
rps - mx - mzrsp mx-mz
xy = i1Q mz; xz = -i1Q my; yz = i1 Q mx; xy = -yx; zx = -xz; zy = -yz;
sssp
pspp
rr
rr
General case: Oblique incidence and arbitrary direction of M
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
Polarization conversion
Summary of phenomenology
Ei Er Ei Er
M
M = 0
pxpx
py( )0
−=
xx
yx
yppx
py
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
( )
+=
=
= sincos
11~
ir
re
r
rr
rE
pp
spi
pp
sp
sp
pp
r
K K
pp
sp
r
rRe
ss
ps
r
rRe
pp
sp
r
rIm
ss
ps
r
rIm
rsp
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
x
y
x’
y’
l/4plate
h
E0
E0sinh
E0cosh
E E i i j= +0(cos sin )h h
Opticaxis
( )
E E i i e j
E i j
E i
i
' (cos sin )
cos sin
'
= +
= +
=
−
02
0
0
h h
h h
x
y
h
E’
E
Measurement of ellipticity
E0 Er
E’rM
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
l/4
l/2
45°
22.5°
p
sp
s p
s
p
s
wollastone
45°p
s
wollastone
Measurement of ellipticity & rotation: high sensitivity
+M
-M
+M
-M
=0
+M
-M
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
Measurement of ellipticity & rotation: high sensitivity
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 201824
Measuring K and K
Modulation polarization technique for recording the longitudinal and polar Kerr effects, which are proportional to the magnetization components mx mz..
POLARIZER Glan-Thompson
PHOTOELASTIC MODULATOR (50kHz)
ORIGINAL ELLIPTICTY
MODULATED ELLIPTICTYPREAMPLIFIED PHOTODIODE
POLARIZER
HeNe LASER
p-polarized beams-p polarized reflected
beam (elliptical polarization)
y
x
Lock-in
Electromagnet
E
More details in: P. Vavassori, Appl. Phys. Lett. 77, 1605 (2000)
K Kspol - mx – mzppol mx- mz
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
Io
Transverse Kerr effect
Laser
Polarizer
Detector
p-polarized light (TM)M
Er = rpp Eo
rpp = ro
pp + rm
ppmy
Ir = Er (Er)*
Ir = Io+ DIm DIm/Io a my
The reflected beam is p-polarized.Variation of intensity and phase.
y
Y. Souche et al.JMMM 226-230, 1686 (2001);JMMM 242-245, 964 (2002).
M fm
Dfm a my
E
E
Polarizer
l/4
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
Supplementary information
Examples of application of MOKE for magnetic characterization of materials and nanosctructures
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
Vector analysis of reversal
H
MMyMx
x
y
My Mx-1.0
-0.5
0.0
0.5
1.0
-1.0
-0.5
0.0
0.5
1.0
-10000 -5000 0 5000 10000
-1.0
-0.5
0.0
0.5
1.0
my
mx
Fig. 2
mz
Field (Oe)
MgO
Fe(300 nm)
NiO(1.4 nm)Fe(7 nm) 180-nm-thick CoNiO
-10000 -5000 0 5000 10000
0
30
60
90
120
150
180
210
240
10000 5000 0 -5000 -10000
180
210
240
270
300
330
360
390
420
-10000 0 10000
0.5
1.0
10000 0 -10000
0.5
1.0
Branch up
out
in
Ro
tatio
n a
ng
le (
de
g.)
out
in
Branch down
Ro
tatio
n a
ng
le (
de
g.)
Field (Oe)
m
Field (Oe)
m
Field (Oe)
- F. Carace, P. Vavassori, G. Gubbiotti, S. Tacchi, M. Madami, G. Carlotti, and T. Okuno, Thin Solid Films 515/2, 727 (2006).- A. Brambilla, P. Biagioni, M. Portalupi, P. Vavassori, M. Zani, M. Finazzi, R. Bertacco, L. Duò, and F. Ciccacci, Phys. Rev. B. 72, 174402 (2005).- P. Vavassori, Appl. Phys. Lett. 77, 1605 (2000) .
Reconstruction of the magnetization vector during the reversal
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
Element sensitivity (and layer sensitivity)
XMCD x-ray magnetic circular dichroism (FeL3 Py hysteresis loop and CoL3 thresholds), → chemical and magnetic sensitivity
PyCuCo
230 nm
10 nm
-1000 -500 0 500 1000
0.1725
0.1730
0.1735
0.1740
0.1745
0.1750
Rotation
MO
KE
sig
nal (a
rb. units)
Field (Oe)
-1000 -500 0 500 10000.065
0.066
0.067
0.068
0.069
0.070
0.071
0.072
0.073
0.074
0.075Ellipticity
MO
KE
sig
nal (a
rb. units)
Field (Oe)
MOKE XMCD
-1000 -500 0 500 1000-5.4
-5.2
-5.0
-4.8
-4.6
-4.4
-4.2
-4.0
Fe
Sig
na
l
Field (Oe)
-1000 -500 0 500 1000-2.0
-1.5
-1.0
-0.5
0.0
0.5
1.0
1.5
2.0
Co
Sig
na
l
Field (Oe)
Simulations
-1000 -500 0 500 1000-0.006
-0.004
-0.002
0.000
0.002
0.004
0.006
Permalloy
MO
KE
sig
nal (a
rb. units)
Field (Oe)
-1000 -500 0 500 1000-0.004
-0.003
-0.002
-0.001
0.000
0.001
0.002
0.003
0.004
Cobalt
MO
KE
sig
na
l (a
rb.
un
its)
Field (Oe)
JOURNAL OF PHYSICS D-APPLIED PHYSICS 41, 134014 (2008)
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
0 20 40 60 80 100
-0,010
-0,005
0,000
0,005
0,010
0,015 Py S Rotation P Rotation
s Ellipticity
P Ellipticity
Radia
nts
Incidence Angle (degrees)
0 20 40 60 80 100
-0,04
-0,02
0,00
0,02
0,04
0,06 Co S Rotation P Rotation
s Ellipticity
P Ellipticity
deg
rees
Incidence Angle (degrees)
0 1 2 3 4 5 6
-0,015
-0,010
-0,005
0,000
0,005
0,010
0,015
0,020
Py S Rotation
P Rotation
s Ellipticity
P Ellipticity
deg
rees
Photon energy (eV)
0 1 2 3 4 5 6
-0,030
-0,025
-0,020
-0,015
-0,010
-0,005
0,000
0,005
0,010
0,015
0,020
0,025
0,030
0,035
0,040
0,045
Co S Rotation
P Rotation
s Ellipticity
P Ellipticity
de
gre
es
Photon energy (eV)
Element sensitivity (thin layer regime)
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
Layer sensitivity
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 201831
Ht = Ht0 Sin(2ft)
H
Lock-in 1: Ref.
freq. 50-100kHz
Lock-in 2:Ref
freq. f
mx0 mx = mx0 Sin (2ft)
MOKE transverse susceptibility: anisotropy
The quantity measured with the Lock-in2 is proportional to the transverse
suceptibility ct = D0 / Ht0.
It can be shown that : 1/ct = (Eo''(eq)/ eq) where Eo(eq) is the total free energy and eq is the
average magnetization, which makes an angle eq with the EA.
H = 700 OeHt = 35 Oef = 156 Hz
0.0
0.4
0.8
1.2
0
30
6090
120
150
180
210
240270
300
330
0.0
0.4
0.8
1.2
1/c
M
t (O
e
Vo
lt-1)
ea
ea ea
ea
1/c
Mt (
arb
. u
nit
s)
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 201832
Configurational anisotropy
Flower state: higher energy
Leaf state: lower energy
Even small perturbations from uniform magnetization which must exist in anynonellipsoidal magnet give rise to a (strong) angular dependence of magnetostaticdipolar energy in symmetric squared particles, which should be magnetically isotropicin the approximation of M uniform. This anisotropy is called configurational anisotropy
Py squares 150 x 150 x 15 nm3
H
fourfold symmetry, at first order, eightfold symmetry at second order
R. P. Cowburn et al. Phys. Rev. Lett. 81, 5414 (1998)
H = 0
P. Vavassori, et al., Phys. Rev. B 72, 054405 (2005)
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 201833
Kerr microscopy: focused laser beam
Laser
Detector
CCD
PHYSICAL REVIEW 72, 224413 (2005)
D. A. Allwood, et al., J. Phys. D: Appl. Phys. 36, 2175 (2003)
Py wires 175 nm wideMicro-MOKE
Py wire 200 nm wideSingle loop
Py wire 100 nm wide1000 loops
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
Polar
Longitudinal and transverse
Kerr microscopy: imaging
M
M
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
Magnetometry of ultra-small nanostructure
EBIDelectron beam induced deposition
Scanning electron microscopy image of the set of EBID cobalt structures
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
APPLIED PHYSICS LETTERS 100, 142401 (2012)
t = 20 nm
single sweep measurement sensitivity of approximately 1 x10-15 Am2
sensitivity of 10-12 to 10-13 Am2 for the latest generation of SQUID magnetometer
t = 5 nm
9 averagesSingle sweep
Magnetometry of ultra-small nanostructure
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
Diffraction of light by an array
"Diffracted-MOKE: What does it tell you?",
M. Grimsditch and P. Vavassori J. Phys.: Condensed Matter 16, R275 - R294 (2004).
As is well known for optical gratings, when a beam of light is incident upon a sample that has a structure comparable to the wavelength of radiation, the beam is not only reflected but is also diffracted. If the material is magnetic, one may ask whether the diffracted beams also carry information about the magnetic structure.
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
Examples of D-MOKE loops
Peculiar structures due to- Collective properties- Interference effects
P. Vavassori, et al., J Appl. Phys. 99, 053902 (2006)
M. Grimsditch, P. Vavassori, et al., Phys. Rev. B 65, 172419 (2002)
P. Vavassori, et al., Phys. Rev. B 67, 134429 (2003)
P. Vavassori, et al., J. Appl. Phys. 101, 023902 (2007)
P. Vavassori, et al.,Phys. Rev. B 59 6337 (1999)
P. Vavassori, et al., Phys. Rev. B 69, 214404 (2004)
P. Vavassori, et al., Phys. Rev. B 78, 174403 (2008)
-2000 -1500 -1000 -500 0 500 1000 1500 2000
-1,0
-0,5
0,0
0,5
1,0
1,5
Rflected
No
rm.
Sig
na
l-2000 -1500 -1000 -500 0 500 1000 1500 2000
-1,0
-0,5
0,0
0,5
1,0
1,5
1st order
No
rm.
Sig
na
l
-2000 -1500 -1000 -500 0 500 1000 1500 2000-3,0
-2,5
-2,0
-1,5
-1,0
-0,5
0,0
0,5
1,0
1,5
2,0
2,5
3,0
Field (Oe) Field (Oe)
Field (Oe)
2nd
order
No
rm.
Sig
na
l
-2000 -1500 -1000 -500 0 500 1000 1500 2000
-2,5
-2,0
-1,5
-1,0
-0,5
0,0
0,5
1,0
1,5
2,0
2,5
3,0
No
rm.
Sig
na
l
3rd order
-2000 -1500 -1000 -500 0 500 1000 1500 2000-1,5
-1,0
-0,5
0,0
0,5
1,0
No
rm.
Sig
na
l
4th order
-600 -400 -200 0 200 400 600
-0.274
-0.273
-0.272
-0.271
-0.270
-0.269
-0.268
Reflected
D-M
OK
E I
nte
nsi
ty (
arb
. u
nits
)
Field (Oe)
H
-2000 -1500 -1000 -500 0 500 1000 1500 2000
-1,0
-0,5
0,0
0,5
1,0
1,5
Rflected
No
rm.
Sig
na
l
-2000 -1500 -1000 -500 0 500 1000 1500 2000
-1,0
-0,5
0,0
0,5
1,0
1,5
1st order
No
rm.
Sig
na
l
-2000 -1500 -1000 -500 0 500 1000 1500 2000-3,0
-2,5
-2,0
-1,5
-1,0
-0,5
0,0
0,5
1,0
1,5
2,0
2,5
3,0
Field (Oe) Field (Oe)
Field (Oe)
2nd
order
No
rm.
Sig
na
l
-2000 -1500 -1000 -500 0 500 1000 1500 2000
-2,5
-2,0
-1,5
-1,0
-0,5
0,0
0,5
1,0
1,5
2,0
2,5
3,0
No
rm.
Sig
na
l
3rd order
-2000 -1500 -1000 -500 0 500 1000 1500 2000-1,5
-1,0
-0,5
0,0
0,5
1,0
No
rm.
Sig
na
l
4th order
Inte
nsity (
norm
. sig
nal)
-600 -400 -200 0 200 400 6000.838
0.840
0.842
0.844
0.846
0.848
0.850
0.852
0.854
0.856
Field (Oe)
D-M
OK
E In
tensi
ty (
arb
. u
nits
)
2nd
order
H
Reflected
Reflected
2nd order
2nd order
-600 -400 -200 0 200 400 600 -600 -400 -200 0 200 400 600 Field (Oe) Field (Oe)
3.0
2.0
1.0
0.0
-1.0
-2.0
-3.0
1.0
0.5
0.0
-0.5
-1.0
1.0
0.5
0.0
-0.5
-1.0
1.0
0.5
0.0
-0.5
-1.0
-2000 -1000 0 1000 2000
Inte
nsity (
norm
. sig
nal)
-2000 -1000 0 1000 2000
IncidencePlane (xz)
H
Laser532 nm50 mW
E
Diffraction
pattern
coil
coil
Photo
dete
cto
r
IncidencePlane (xz)
H
Laser532 nm50 mW
E
IncidencePlane (xz)
H
Laser532 nm50 mW
IncidencePlane (xz)
H
Laser532 nm50 mW
E
Diffraction
pattern
coil
coil
Photo
dete
cto
r
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
Intuitive explanation of D-MOKE loops
Peculiar structures due to- Interference effects- Collective propertiesO. Geoffroy et al., J. Magn. Magn. Mat. 121 (1993) 516
Y. Souche et al., J. Magn. Magn. Mat., 140-144 (1995) 2179
H
rpp = ro
pp + rm
ppmy(x,y)
M M
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
Physical-optics approximation provides a very simple and physically transparent
description.
The electric field in the nth order diffracted beam, due to the periodic modulation of
the “effective” reflectivity r’pp is:
End = Eo fnfn = S r’pp exp{i n G•r} dS where n integer, G reciprocal lattice vector
and S is the unit cell.
r’pp = ropp + rmpp my(x,y,H)
End = Eo (r
opp fn
nm + rmpp fnm ) with ropp(i, n, dots, subst), rmpp(i, n, dots, Q)
fnnm = S exp{i n G•r} dxdy non-magnetic form factor
fnm (H)= Dot my(x,y,H) exp{i n G•r}dxdy magnetic form factor
Ind = En
d (End)* DIn
m (my) = AnRe[fnm]+Bn Im[fnm]
Simple theory of diffracted-MOKE
-
P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
DInm a An Re[fn
m] + Bn Im[fnm]
Re[fnm]= Dot my cos(n Gx x) dS
Im[fnm]= Dot my sin(n Gx x) dS
Im[f1m] = 0
Saturated state Re[f1
m] > 0
What are the differences due to?
y
x
period L
Unit cell
Gx = 2/L reciprocal lattice vector
Diffracted spots in the scattering planey
x
y
x
1st order
Im[f1m] < 0
Re[f1m] = 0
Im[f1m] > 0
Re[f1m] = 0
2nd order
Im[f2m] < 0 large
Re[f2m] = 0
y
x
y
x
3rd order
Im[f2m] < 0 very large
Re[f2m] = 0
Two-domain state: asymmetric M distribution
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
y
x
Tuning the sensitivity to selected portions of the dot!
Immaginary contribution:highlight any asymmetric (y-mirror symmetry breaking) magnetic (my) behaviour
Real contribution:y-mirror symmetry my
y
x
period L
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
Asymmetry to induce the desired vortex rotation
Narrow channel pins
the magnetization2 m
-600 -400 -200 0 200 400 600
-0.274
-0.273
-0.272
-0.271
-0.270
-0.269
-0.268
Reflected
D-M
OK
E Inte
nsity (
arb
. units)
Field (Oe)
3
1
2
-600 -400 -200 0 200 400 6000.838
0.840
0.842
0.844
0.846
0.848
0.850
0.852
0.854
0.856
Field (Oe)
D-M
OK
E In
tensity (
arb
. u
nits)
2nd
order
-600 -400 -200 0 200 400 600-0.46
-0.44
-0.42
-0.40
-0.38
-0.36
-0.34
1st order
D-M
OK
E Inte
nsity (
arb
. units)
-600 -400 -200 0 200 400 600-0.285
-0.280
-0.275
-0.270
-0.265
-0.260
-0.255
1st order
-600 -400 -200 0 200 400 600-0.231
-0.230
-0.229
-0.228
-0.227
-0.226
-0.225
-0.224
Field (Oe)
2nd
order
H
H
H
H
H
-600 -400 -200 0 200 400 600
-3
-2
-1
0
1
2
3
Field (Oe)
2nd
order (Re[fd
m] + 0.65 * Im[f
d
m])
-600 -400 -200 0 200 400 600-1.5
-1.0
-0.5
0.0
0.5
1.0
1.5
No
rma
lize
d D
-MO
KE
sig
na
l
Reflected
Field (Oe)
H
H H
H H
-600 -400 -200 0 200 400 600-1.5
-1.0
-0.5
0.0
0.5
1.0
1.5
1st order (Re[f
d
m] + 0.8 * Im[f
d
m])
No
rma
lize
d D
-MO
KE
sig
na
l
-600 -400 -200 0 200 400 600-1.5
-1.0
-0.5
0.0
0.5
1.0
1.5
1st order (Re[f
d
m] + 0.8 * Im[f
d
m])
-600 -400 -200 0 200 400 600-1.5
-1.0
-0.5
0.0
0.5
1.0
1.5
No
rma
lize
d D
-MO
KE
sig
na
l
Field (Oe)
2nd
order (Re[fd
m] + 0.65 * Im[f
d
m])
P. Vavassori, R. Bovolenta, V. Metlushko, and B. Ilic, J Appl. Phys. 99, 053902 (2006)
Measured Calculated
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
Measured D-MOKE loops from square rings
-2000 -1000 0 1000 2000
-1.0
-0.5
0.0
0.5
1.0
Norm
alize
d Kerr
sign
al
0th order
-2000 -1000 0 1000 2000
-1.0
-0.5
0.0
0.5
1.00
th order
-2000 -1000 0 1000 2000
-15
-10
-5
0
5
10
15
1st order
Field (Oe)
-2000 -1000 0 1000 2000
-3
-2
-1
0
1
2
3
1st order
Norm
alize
d Kerr
sign
al
Field (Oe)
(a) (b)
Reflected
1st order 1st order
Reflected
H H
Square lattice (4.1x4.1 m2) of
Permalloy square rings (2.1 m
side). Nominal width 250 nm.
Thickness 30 nm.
Note intense peaks in the diffracted loopsP. Vavassori, et al., Phys. Rev. B 67, 134429 (2003)
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
Square ring structures
1 saturated state
2 onion state 4 reversed onion state 5 saturated state
1 saturated state 4 reversed onion state 5 saturated state
2 onion state
-2000 -1000 0 1000 2000
-8
-4
0
4
8
Norm
alize
d sign
al 1st order
Field (Oe)
-2000 -1000 0 1000 2000-2
-1
0
1
2
Field (Oe)
1st order
Norm
alize
d sign
al
3 horseshoe state
3 vortex state
H
H
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
Quenching structures in intermediate states
and image them with MFM
-1000 -500 0 500 1000-3
-2
-1
0
1
2
3
Norm
alize
d Kerr
sign
al
Field (Oe)
H
-1000 -500 0 500 1000
-15
-10
-5
0
5
10
15
Norm
alize
d Kerr
sign
al
Field (Oe)
H
(c)
(b)
P. Vavassori, M. Grimsditch, V. Novosad, V. Metlushko, B. Ilic, P. Neuzil, and R. Kumar, Phys. Rev. B 67, 134429 (2003)
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
Y. Suzuki, C. Chappert, P. Bruno, and P. Veillet, J. Magn. Magn. Mater. 165 516 (1997) only for size >> l
“effective” reflectivity
An = Re[ro
pp* rmpp]
Bn = Im[ro
pp* rmpp]
An and Bn (i, n, dots, sub, Q)
r’pp = ropp + rmpp
For inhomogeneous gratings ropp = ropp, dot + ropp, sub
DInm (my) = 2 fn
nm { AnRe[fnm]+Bn Im[fn
m] }
About An and Bn
An interesting characteristic of D-MOKE related to this : the absolute value of (DI/Io)n is increased up to several times the specular value. Effect due to the compensation of the non-magnetic component of the light diffracted by the magnetic dots and the light diffracted by the (non-magnetic) complementary part of the substrate.
Io,n = |ro
pp, dot|2 fnnm + | ropp, sub |2 f’n
nm = ( |ropp, dot|2 - | ropp, sub |2 )fnnm
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
532 n
m la
ser
Different approach: towards Fourier imaging? 1st step
H(1,0)(-1,0)
(0,1)
(0,-1)(-1,-1) (1,-1)
(1,1)(-1,1)
Normal incidence: the scattering plane is defined by the selected spot
y
x
Sensitivity to (mx , my)
Sensitivity to mx
-2000 -1000 0 1000 2000
-0.0465
-0.0460
-0.0455
-0.0450
-0.0445
-0.0440
-0.0435
-0.0430
-0.04252
nd order m
x
MO
KE
in
ten
sity (
arb
. u
nits)
Field (Oe)
Vectorial D-MOKE
(DInm)norm = An Re[fn
m]- Bn Im[fnm]
(DI-nm)norm = −An Re[fn
m]- Bn Im[fnm]
Sensitivity to my
-2000 -1000 0 1000 2000-16.55
-16.50
-16.45
-16.40
-16.35
-16.30 2nd
order my
MO
KE
in
ten
sity (
arb
. u
nits)
Field (Oe)
-2000 -1000 0 1000 2000
-1.0
-0.5
0.0
0.5
1.0
Norm
alize
d Kerr
sign
al
0th order
-2000 -1000 0 1000 2000
-1.0
-0.5
0.0
0.5
1.00
th order
-2000 -1000 0 1000 2000
-15
-10
-5
0
5
10
15
1st order
Field (Oe)
-2000 -1000 0 1000 2000
-3
-2
-1
0
1
2
3
1st order
Norm
alize
d Kerr
sign
al
Field (Oe)
(a) (b)
-2000 -1000 0 1000 2000
-1.0
-0.5
0.0
0.5
1.0
Norm
alize
d Kerr
sign
al
0th order
-2000 -1000 0 1000 2000
-1.0
-0.5
0.0
0.5
1.00
th order
-2000 -1000 0 1000 2000
-15
-10
-5
0
5
10
15
1st order
Field (Oe)
-2000 -1000 0 1000 2000
-3
-2
-1
0
1
2
3
1st order
Norm
alize
d Kerr
sign
al
Field (Oe)
(a) (b)
Im
Re
Mz
x
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
K. Postava et al. “Null ellipsometer with phase modulation,” Opt. Express 12, 6040 (2004)
compensator
analyzer
photodetector
photoelasticmodulator
polarizer
laserrLock-inI
I2Lock-in Re[Drm/r0] = DIm/I0
Im[Drm/r0] = Dfm/f0
Dfnm/fn
o = Bn Re[fnm]−An Im[fn
m]
DInm/In
o = An Re[fnm]−Bn Im[fn
m] DI−nm/I−n
o = −An Re[fnm] − Bn Im[fn
m]
Df−nm/f−n
o = −Bn Re[fnm] − An Im[fn
m]
Re[fnm]
Im[fnm]
D-MOKE problem fully solved
M fm
Dfm a my
E
E
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
Samples: arrays of NiFe triangular rings
Triangular rings (2.1 m side).
Nominal width 250 nm.
Nominal thickness 30 nm.
ZEP 520 Resist (0.3 m)
PMGI Resist (0.3 m)
Exposed Areas
Double Layer Resist Spin-coating
EB Patterning Si substrate
Resist Development
EB Deposition
(FeNi target)
Lift-off process nanoelement
Electron beam lithography
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
+1
-1
-2000 -1000 0 1000 2000
-0,002
-0,001
0,000
0,001
0,002
-2000 -1000 0 1000 2000
-0,003
-0,002
-0,001
0,000
0,001
0,002
0,003
Am
plit
ude(m
V)
Field(Oe)
-1 order Re(Drpp/rpp)
-1 order Im(Drpp/rpp)
Am
plit
ude(m
V)
Field(Oe)
-2000 -1000 0 1000 2000
-0,001
0,000
0,001
-2000 -1000 0 1000 2000
-0,002
-0,001
0,000
0,001
0,002
Am
plit
ude(m
V)
Field(Oe)
+1 order Re(Drpp/rpp)
Am
plit
ude(m
V)
Field(Oe)
+1 order Im(Drpp/rpp)
Normal incidence: extraction of magnetic form factors
Dfnm/fn
o = Bn Re[fnm]−An Im[fn
m]
DInm/In
o = An Re[fnm]−Bn Im[fn
m] DI−nm/I−n
o = −An Re[fnm] − Bn Im[fn
m]
Df−nm/f−n
o = −Bn Re[fnm] −An Im[fn
m]
Re[fnm]
Im[fnm]
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
Fig. 2
nmf nmf
-0.10
-0.05
0.00
0.05
-0.02
0.00
0.02
-2 -1 0 1 2
-0.12
-0.06
0.00
0.06
-2 -1 0 1 2
-0.08
-0.04
0.00
0.04
-0.05
0.00
0.05
0.10
-0.03
0.00
0.03
2nd
order horizontal
2nd
order vertical
3rd
order horizontal
CalculatedExperimental
1st
order horizontal
Form
fact
orField (kOe)
3rd
order vertical
1st
order vertical
Exp and calculated Re[fm] and Im[fm] – horizontal and vertical plane
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
-2000 -1000 0 1000 2000-0,14
-0,12
-0,10
-0,08
-0,06
-0,04
-0,02
0,00
0,02
0,04
0,06
0,08
0,10
Re
Im
Am
plit
ud
e
Field (Oe)
-2000 -1000 0 1000 2000-0,06
-0,04
-0,02
0,00
0,02
0,04
0,06
Re
Im
Am
plit
ud
e
Field (Oe)-2000 -1000 0 1000 2000
-0,020
-0,015
-0,010
-0,005
0,000
0,005
0,010
0,015
0,020 Re
Im
Am
plit
ude
Field (Oe)
-2000 -1000 0 1000 2000
-0,10
-0,08
-0,06
-0,04
-0,02
0,00
0,02
0,04
0,06 Re
Im
Am
plit
ud
e
Field (Oe)
-2000 -1000 0 1000 2000-0,08
-0,06
-0,04
-0,02
0,00
0,02
0,04 Re
Im
Am
plit
ud
e
Field (Oe)
-2000 -1000 0 1000 2000
-0,06
-0,04
-0,02
0,00
0,02
0,04
0,06
0,08
0,10
0,12
Re
Im
Am
plit
ude
Field (Oe)
1st - h 2nd - h 3rd - h
1st - v 2nd - v 3rd - v
Re and Im parts of the magnetic form factors
-
P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
0 50 100 150 200
0
50
100
150
200
0 50 100 150 200
0
50
100
150
200
Saturated state
0 50 100 150 200
0
50
100
150
200
0 50 100 150 200
0
50
100
150
200
0 50 100 150 200
0
50
100
150
200
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
“Peak” state
0 50 100 150 200
0
50
100
150
200
0 50 100 150 200
0
50
100
150
200
0 50 100 150 200
0
50
100
150
200
0 50 100 150 200
0
50
100
150
200
0 50 100 150 200
0
50
100
150
200
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
0 50 100 150 200
0
50
100
150
200
0 50 100 150 200
0
50
100
150
200
0 50 100 150 200
0
50
100
150
200
0 50 100 150 200
0
50
100
150
200
0 50 100 150 200
0
50
100
150
200
After “peak”
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
0 50 100 150 200
0
50
100
150
200
0 50 100 150 200
0
50
100
150
200
0 50 100 150 200
0
50
100
150
200
0 50 100 150 200
0
50
100
150
200
0 50 100 150 200
0
50
100
150
200
Towards negative saturation
-
P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
-2000 -1000 0 1000 2000
-0,12
-0,09
-0,06
-0,03
0,00
0,03
0,06
0,09 Re
Im
Am
plit
ud
e
Field (Oe)
-2000 -1000 0 1000 2000-0,06
-0,04
-0,02
0,00
0,02
0,04
0,06
Re
Im
Am
plit
ude
Field (Oe)
-2000 -1000 0 1000 2000
-0,020
-0,015
-0,010
-0,005
0,000
0,005
0,010
0,015
0,020
Re
Im
Am
plit
ude
Field (Oe)
-2000 -1000 0 1000 2000-0,14
-0,12
-0,10
-0,08
-0,06
-0,04
-0,02
0,00
0,02
0,04
0,06
0,08
0,10
Re
Im
Am
plit
ude
Field (Oe)
-2000 -1000 0 1000 2000-0,06
-0,04
-0,02
0,00
0,02
0,04
0,06
Re
Im
Am
plit
ude
Field (Oe)
-2000 -1000 0 1000 2000
-0,020
-0,015
-0,010
-0,005
0,000
0,005
0,010
0,015
0,020 Re
Im
Am
plit
ud
e
Field (Oe)
Exp and calculated Re[fm] and Im[fm] – horizontal plane
1st - h 2nd - h 3rd - h
-
P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
-2000 -1000 0 1000 2000-0,08
-0,06
-0,04
-0,02
0,00
0,02
0,04
0,06
0,08
0,10
0,12 Re
Im
Am
plit
ude
Field (Oe)
-2000 -1000 0 1000 2000-0,10
-0,08
-0,06
-0,04
-0,02
0,00
0,02
0,04
0,06
0,08
Re
Im
Am
plit
ude
Field (Oe)
-2000 -1000 0 1000 2000
-0,08
-0,06
-0,04
-0,02
0,00
0,02
0,04
0,06 Re
Im
Am
plit
ude
Field (Oe)
-2000 -1000 0 1000 2000
-0,10
-0,08
-0,06
-0,04
-0,02
0,00
0,02
0,04
0,06 Re
Im
Am
plit
ud
e
Field (Oe)
-2000 -1000 0 1000 2000-0,08
-0,06
-0,04
-0,02
0,00
0,02
0,04 Re
Im
Am
plit
ude
Field (Oe)
-2000 -1000 0 1000 2000
-0,06
-0,04
-0,02
0,00
0,02
0,04
0,06
0,08
0,10
0,12
Re
Im
Am
plit
ude
Field (Oe)
1st - v 2nd - v 3rd - v
Exp and calculated Re[fm] and Im[fm] – vertical plane
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P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
Micromagneticsimulations
D-MOKE
MFM(quenchedTo 0 field)
Magnetic imaging proved
APPLIED PHYSICS LETTERS 99, 092501 (2011)
-
P. VAVASSORI European School on Magnetism (ESM-2018), Krakow 17-28 September 2018
MOKE is a powerful technique for studying technologically relevant magneticmaterials.
MOKE magnetometry based on microscopy provides a noninvasive probeof magnetization reversal for individual ultra-small nano-structures.
Concluding remarks
Next lecture:
Interplay between plasma excitations and MO-activity (magnetoplasmonics).
D-MOKE is a powerful technique to investigate the collective behavior of
magnetic nano-arrays.