Title: Nonlinear Magneto-Optical Studies in Magnetic Superlattices and Magnetic Nano Structures
1Nonlinear Magneto-Optical Studies in Magnetic
Superlattices and Magnetic Nano Structures
1st International Conference on Quantum Photonic
Science
- K. Sato, A. Kodama, M. Miyamoto, M. Tsuruga, T.
Matsumoto, T. Ishibashi Y. Morishita, Department
of Applied Physics, Tokyo University of
Agriculture and Technology, Koganei, Tokyo, Japan - K. Takanashi, S. Mitani, Institute of Materials
Science, Tohoku University, Sendai, Miyagi, Japan
TUAT COE Project Future Nano Materials
2Nonlinear Magneto-optics
- What is the nonlinear magneto-optical effect?
- Magnetization-induced nonlinear optics
- What is the nonlinear Kerr rotation?
- When P-polarized primary light is incident both
P- and S-polarized SH light emits which leads to
rotation of E vector from the plane of incidence. - In centrosymmetric materials such as Fe and Au no
SHG occurs due to cancellation of P and P.
3Azimuthal angle dependence of SHG from Si and
GaAs wafer
Si wafer (001) centrosymmetric
GaAs wafer (001) Non-centrosymmetric
4Theoretical prediction and experimental
verification
- Nonlinear magneto-optical Kerr rotation larger
than linear rotaion was theoretically
predicted1), and was experimentally proved2,3). - 1) W. Hübner and K.-H. Bennemann Phys. Rev. B40,
5973 (1989) - 2) Th. Rasing et al. J. Appl. Phys. 79, 6181
(1996) - 3) Th. Rasing J. Mag. Soc. Japan 20 (Suppl. S1),
13 (1996)
5Surface and interface sensitivity of MSHG
- Application of MSHG
- Sensitive to Evaluation of
- the break of Multilayers
- symmetry at surface Imaging of domains
- This effect cannot be expected to be applied to
some practical memory devices but is thought to
be useful for characterization of surfaces and
interfaces of materials.
6Nonlinear magneto-optical effect
linear response
For weak incident laser field E(w)
Nonlinear response
For strong incident laser field E(w)
Third rank tensor is not allowed in
centrosymmetric materials.
Nonlinear polarization P(2) for incident field
of EE0sinwt
Second harmonic generation (SHG)
7Nonlinear polarization of 2nd order
parametric process
SHG process
Light rectification
8Definition of nonlinear susceptibility
Centrosymmetric materials all the ?ijk(2)
components vanish. (from symmetry
operations) Surfaces and interfaces symmetry
breaks, leading to appreciable amount of
nonlinear magneto-optical effect even in the
centrosymmetric materials
9Wave equation of linear magneto-optical effect
YKfKihK (???????)
c1(1)eyz, c0(1)exx-1N2-1
10Wave equation of nonlinear magneto-optics.
Source term does not depend on optical constants
of materials, leading to special solution
associated with the second order susceptibility.
11Nonlinear Kerr roation
12Nonlinear Kerr rotaion
Different from the linear case ?(2)odd/?(2)even
contributes? This term is zero in centrosymmetric
materials And takes a finite value at
surfaces Surface sensitivity useful for
surface magnetism studies!
13Difference between linear and nonlinear Kerr
rotation
Linear factor reduces the
magnitude Also ?xy is order of magnitude smaller
that ?xx Nonlinearno such factor exists Also
?odd and ?even are of the same order ?
14Microscopic origin of MSHG
3 photon proicess
SHG
Here
k q//l gt?kq//lgt kq//lgt?k2q//l" gt
klgt ?k2q//lgt
w
w
2w
Intermediate state
Ground state
Excited state
15Illustration of microscopic process of MSHG
16Nonlinear Kerr rotation of Fe
17Nonlinear Kerr rotation of Fe/Cu
Nonlinaer Kerr effect
nolinear
18Cu cover layer-thickness dependence of Co/Cu
SH??
Cu???
19Superlattices ?Fe(xML)/Au(xML)?N
Integer x1, 2, 3, 4, 5, 6, 8, 10, 15
Non-integer x1.25, 1.5, 1.75, 2.25, 2.5, 2.75,
3.25, 3.5, 3.75
20Fe(1ML)/Au(1ML) superlattice
4.054Å
bcc-Fe (001)
Au
Fe
2.867Å
Schematic structure for the Fe/Au superlattice
L10
fcc-Au (001)
4.079Å
Atomic arrangement in a unit cell of Fe-Au with a
L10 suructure.
21MSHG Measureing System
22Laboratory
- Experimental setup for MSHG measurement
23Optical Setups(Longitudinal Kerr)
Sample
????
Sample stage
w (810nm)
P-polarized or S-polarized light
Pole piece
45
Rotating analyzer
w (810nm)
Analyzer
Filter
2w (405nm)
24Nonlinear Kerr Rotation and Kerr Ellipticity
Result
The curves show a shift for two opposite
directions of magnetic field
Analyzer angle-dependence for Fe(3.5ML)/Au(3.5ML)
(Sin)
Nonlinear Kerr rotation ellipticity ?K(2) 17.2
? hK(2)3
25Largest nonlinear Kerr rotationobserved in the
Fe/Au series
Df 31.1
Fe(1.75ML)/Au(1.75ML) Sin
26Azimuthal Angle Dependence
Linear optical response (?810nm) The
isotropic response for the azimuthal angle
Nonlinear optical response (?405nm) The
4-fold symmetry pattern Azimuthal pattern show
45?-rotation by reversing the magnetic field
nonlinear
linear
45?
SHG intensity (counts/10sec.)
SHG intensity (counts/10sec.)
(a) Linear (810nm)
(b) SHG (405nm)
Azimthal angle-dependence of MSHG intensity for
Fe(3.75ML)/Au(3.75ML) superlattice. (Pin Pout)
27Pin-Pout
Azimuthal Angle Dependence
Sin-Sout
28The equation of the azimuthal angle-dependence by
the theoretical analysis
Discussion
A Surface nonmagnetic term The
electric dipole origin give rise to isotropic
signal.
B Bulk nonmagnetic term The quadrupole
origin causes an anisotropic contribution for
four rank tensor.
C Surface magnetic term The time reversal
symmetry is lifted by magnetization Mirror
symmetry operations should be supplemented with
an additional reversion of M.
29Calculated azimuthal angle dependence of SHG and
MSHG signals
Kerr rotation calculated from parameters Axx,B,C
Sin
Pin
30 Surface non-magnetic term
SHG response causes an isotropic contribution
only.
Bulk non-magnetic term
For crystallographic contribution the electric
quadrupole should be introduced to get four rank
tensor.
SHG response causes an anisotropic contribution
(parameter B).
Surface magnetization induced term
The surface magnetic response comes from the
electric dipole term expanded by magnetization
and contributes to the parameter C.
31Calculated polar patterns of the azimuthal
angle-dependence (Sin-Pout)
Without nonlocality
The equation of the azimuthal angle-dependence by
theoretical analysis
(a) A5, B0, C0.85 For B much smaller than
C, the polar pattern shows 45? rotation for the
magnetization reversal.
With nonlocality
(b) A5, B0.85, C0.85 ?For B comparable C,
the polar pattern undergo a smaller rotation.
32Azimuthal angle-dependence of MSHG for a
Fe(3.5ML)/Au(3.5ML) superlattice(Sin-Pout,
Sin-Sout configuration)
The equation of the azimuthal angle-dependence by
theoretical analysis
Sin-Pout
Sin-Sout
ASP(surface nonmagnetic term) 460 ASS(surface
nonmagnetic term) 100 B(bulk nonmagnetic
term) 26 C(surface magnetic term) -88
33Calculated and experimental patterns x3.5
Dotsexp. Solid curvecalc.
34Calculated and experimental pattern of Nonlinear
Kerr rotation and ellipticity
(a) Experimental pattern (Sin)
The azimuthal angle-dependences of nonlinear
Kerr rotation angle and ellipticity in
Fe(3.75ML)Au(3.75ML)
(b) Calculated pattern (Sin)
35Experimental and calculated patterns of Kerr
rotation angle
(b) Calculation
(a) Experiment
(b) Calculation
(a) Experiment
Nonlinear Kerr rotation (deg.)
Fe(2.75ML)/Au(2.75ML)
Sin configuration (a) Experimental data,
(b) Calculated
using parameters determined by fitting to the
azimuth patterns
36Nonlinear Kerr rotation angle of
Fe(xML)/Au(xML) (1.25?x?3.75) superlattices
(Sin)
Calculation and experimental result
Calculated nonlinear Kerr rotation angle ?K(2)
using the fitting parameter ASP, ASS, B, C of the
azimuthal pattern (The maximum ?K(2) was
selected for azimuth angle)
? The experimental maximum ?K(2) for x1.75
superlattice was 31.1?. The calculated ?K(2)
reproduced the muximum ?K(2) for x1.75
superlattice.
The nonlinear Kerr rotation was explained by
theoretical analysis.
Fig. Nonlinear Kerr rotation angle of
Fe(xML)/Au(xML) (1.25?x?3.75) superlattices
(a)Calculation, (b)Experiment
37Summary MSHG of Fe/Au superlattice
The four-fold pattern clearly reflects the
symmetry of the MgO(100) substrate. This suggests
that the Fe/Au superlattice is perfectly
epitactic to the substrate.
The azimuthal angle dependence was analyzed in
terms of nonlinear electrical susceptibility
tensor taking into account the magnetic symmetry
of the superlattice.
?The azimuthal pattern was explained by symmetry
analysis, taking into account the surface
non-magnetic A, bulk non-magnetic B and surface
magnetic C contributions.
38Summary (contd)
MSHG was shown to lead to a nonlinear Kerr
rotation ?(2)K that can be orders of magnitude
larger than its linear equivalent (0.2?), e.g.,
?(2)K for x1.75 was 31.1?
- We observed azimuthal angle-dependence of the
nonlinear Kerr rotation for the first time.
The azimuthal angle-dependence of the nonlinear
Kerr rotation were explained using parameters
determined from azimuthal patterns of MSHG
response
- Modulation period dependence of parameters
- A (Surface nonmagnetic) is large for short period
- B (Bulk nonmagnetic) is nearly constant
- C (Surface magnetic) becomes larger with
modulation Period.
39Fabrication of permalloy nanostructure by
Damascene technique
- ?Preparation of substrate Spin-coating of ZEP
resist with high etching resistance - ?EB-exposition Write patterns by EB
- ?Development Formation of mask-pattern by
development - ?EtchingBy dry-etching process mask-pattern is
transferred to the substrate - ?Deposition of magnetic film Deposition of
magnetic films by sputter or evaporation - ?Polishing Obtain flat buried structure using
chemical-mechanical polishing - Process is simplified by abbreviation of lift-off
and repeated spin-coating
40EB-patterning process
Spin coating of resist
EB exposure
Development
Si substrate
- ?1?Dot size
- 100nm300nm rectangular dot with 300nm-spacing
- 100nm square dot with 300nm-spacing
- ?2?Patterned area 3mm3mm
- ?3?EB-resist thickness 300 nm
- by spin-coating with 5000 rpm rotation
- ?4?Baking 160? 20min
41Clean Room Laboratory
- Electron beam lithography
42Dry etching process
?1?Etching gas CF4 ?2?Vacuum 3.010-3Pa ?3?Gas
pressure 9.2Pa ?4?RF power 400W ?5?Etching
rate 0.1µm/min
Silicon surface after etching
43Dry-etching
44Laboratory
RF magnetron sputtering
45Embedding of permalloy
?1?material permalloy(Ni80Fe20) ?2?Vacuum
3.010-6Torr ?3?Accelerating voltage 4kV
?4?Deposition rate 1.0Å/sec
Embedding of permalloy film by electron beam
deposition
Chemical mechanical polishing
?1?Polishing chemicals Si wafer
grain-size20nm ?2?pH 11 ?3?polishing rate
60nm/min
flatting
46Observation
FE-SEM
47SEM observation
300nm100nmsquare dot, 300 nm space
48Cross sectional SEM observation
Dot depth?
49Cross section SEM image of Line and space pattern
(width 100nm)
0.3µm
50MFM observation of a permalloy film
51AFM and MFM observation
1µm
AFM Line scan Surface roughness10nm MFM image
magnetization axis along the longer side
direction
52Comparison between two scans after magnetization
in opposite direction
5kOe
5kOe
53MFM-image for different scanning direction
54Scan-direction dependence
55Pattern variation with scan direction
56VSM measurement
Perpendicular
57100nm circular dotswith 300 nm spacing
SEM
AFM
Surface roughness 10nm
58VSM measurement of circular dot array
Parallel to the plane
Perpendicular to the plane
59MFM measurement of circular dots
Magnetic field applied Perpendicular to the plane
Demagnetized
60Influence of stray field from the MFM probe tip
MFM measurenment
AFM sensing (2-3nmlevitation) MFM probe
80nm
A
B
A
B
Magnetization
Magnetization
Reading by second scan
Recording by first scan
61Models to explain MFM images
MFM image
Magnetization
621?m square dot array
MFM
AFM
63MFM image of 300nm x 100nm dot with a low-moment
probe tip
MFM
AFM
64300nm x 100nm dot (wide scan)with a low-moment
probe tip
AFM
MFM
65Simulation by Nakatani
66MSHG studies of Nano-structured magnetic patterns
67Azimuthal angle dependence of SHG from
unpatterned permalloy film
PinPout
Longitudinal
(counts/10sec)
Unstructured permalloy film H2.5kOe
68Azimuthal angle dependence of SHG from
unpatterned Si wafer
PinPout
(counts/10sec)
H2.5kOe
69Azimuthal angle dependence of SHG from GaAs wafer
70Azimuthal angle dependence of MSHG from 1?m
square dot array
PinPout
(counts/10sec)
Longitudinal Kerr configuration
H4kOe
71Azimuthal angle dependence of MSHG from 300nm x
100nm rectangular dot array (Longitudinal)
PinPout
SinPout
(counts/10sec)
(counts/10sec)
Longitudinal configuration
H4kOe
72Azimuthal angle dependence of MSHG from 300nm x
100nm rectangular dot array (Polar)
PinPout
(counts/10sec)
polar Kerr configuration
H6kOe
73?????
PinSout
PinPout
(counts/10sec)
(counts/10sec)
SinPout
SinSout
(counts/10sec)
(counts/10sec)
????(100nm)?????????4kOe
74???????? 6.00