Title: Recent Advances in Magneto-Optics
1Recent Advances in Magneto-Optics
- Katsuaki Sato
- Department of Applied Physics
- Tokyo University of Agriculture Technology
2CONTENTS
- Introduction
- Fundamentals of Magneto-Optics
- Magneto-Optical Spectra
- Experiments and theory
- Recent Advances in Magneto-Optics
- Magneto-optics in nano-structures
- Nonlinear magneto-optical effect
- Scanning near-field magneto-optical microscope
- Current Status in Magneto-Optical Devices
- Magneto-optical disk storages
- Magneto-optical isolators for optical
communication - Other applications
- Summary
31. Introduction
- Magneto-Optical EffectDiscovered by Faraday on
1845 - PhenomenonChange of Linear Polarization to
Elliptically Polarized Light Accompanied by
Rotation of Principal Axis - CauseDifference of Optical Response between LCP
and RCP - Application
- Magneto-Optical Disk
- Optical Isolator
- Current Sensors
- Observation Technique
42.Fundamentals of Magneto-Optics
- MO Effect in Wide Meaning
- Any change of optical response induced by
magnetization - MO Effect in Narrow Meaning
- Change of intensity or polarization induced by
magentization - Faraday effect
- MOKE(Magneto-optical Kerr effect)
- Cotton-Mouton effect
52.1 Faraday Effect
- (a) Faraday Configuration
- Magnetization // Light Vector
- (b)Voigt Configuration
- Magnetization ? Light Vector
6Faraday Effect
- MO effect for optical transmission
- Magnetic rotation(Faraday rotation)?F
- Magnetic Circular Dichroism(Faraday
Ellipticity)??F - Comparison to Natural Optical Rotation
- Faraday Effect is Nonreciprocal (Double rotation
for round trip) - Natural rotation is Reciprocal (Zero for round
trip) - Verdet Constant
- ?FVlH (For paramagnetic and diamagnetic
materials)
7Illustration of Faraday Effect
Rotation of Principal axis
- For linearly polarized light incidence,
- Elliptically polarized light goes out (MCD)
- With the principal axis rotated (Magnetic
rotation)
Elliptically Polarized light
Linearly polarized light
8Faraday rotation of magnetic materials
92.2 Magneto-Optical Kerr Effect
- Three kinds of MO Kerr effects
- Polar Kerr(Magnetization is oriented
perpendicular to the suraface) - Longitudinal Kerr(Magnetization is in plane and
is parallel to the plane of incidence) - Transverse Kerr (Magnetization is in plane and is
perpendicular to the plane of incidence)
10Magneto-optical Kerr effect
M
M
M
- Polar Longitudinal Transverse
11 MO Kerr rotation of magnetic materials
"a-" means "amorphous".
122.3 Electromagnetism and Magnetooptics
- Light is the electromagnetic wave.
- Transmission of EM waveMaxwell equation
- Medium is regareded as continuum?dielectric
permeability tensor - Effect of Magnetic field?mainly to off-diagonal
element - Eigenequation
- ?Complex refractive indextwo eigenvalues
- eigenfunctionsright and left circularpolarizatio
n - Phase difference between RCP and LCP?rotation
- Amplitude difference ?circular dichroism
13Dielectric tensor
Isotromic mediaM//z Invariant C4 for 90rotation
around z-axis
14MO Equations (1)
Maxwell Equation
Eigenequation
Eigenvalue
EigenfunctionLCP and RCP
Without off-diagonal termsNo difference between
LCP RCP
No magnetooptical effect
15MO Equations (2)
Both diagonal and off-diagonal terms contribute
to Magneto-optical effect
16 Phenomenology of MO effect
Linearly polarized light can be decomposed to LCP
and RCP
Difference in phase causes rotation of the
direction of Linear polarization
Difference in amplitudes makes Elliptically
polarized light
In general, elliptically polarized light With the
principal axis rotated
172.4 Electronic theory of Magneto-Optics
- Magnetization?Splitting of spin-states
- 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
18Dielectric functions derived from Kubo formula
where
19Microscopic concepts of electronic polarization
Expansion by unperturbed orbitals
20Orbital angular momentum-selection rules and
circular dichroism
py-orbital
px-orbital
ppxipy
Lz1
Lz-1
p-px-ipy
Lz0
s-like
21Role of Spin-Orbit Interaction
Jz-3/2
Jz-1/2
L1
Jz1/2
LZ1,0,-1
Jz3/2
Jz-1/2
L0
Jz1/2
LZ0
Exchange spin-orbit
Exchange splitting
Without magnetization
22 MO lineshapes (1)
23MO lineshapes (2)
2.Paramagnetic lineshape
243. Magneto-Optical Spectra
- Measurement technique
- Magnetic garnets
- Metallic ferromagnetFe, Co, Ni
- Intermetallic compounds and alloysPtMnSb etc.
- Magnetic semiconductorCdMnTe etc.
- SuperlatticesPt/Co, Fe/Au etc.
- AmorphousTbFeCo, GdFeCo etc.
25Measurement of magneto-optical spectra using
retardation modulation technique
Light source
chopper
filter
ellipsoidal mirror
monochromator
polarizer
eletromagnet
sample
sample
analyzer
detector
computer
26Magnetic garnets
- One of the most intensively investigated
magneto-optical materials - Three different cation sites octahedral,
tetrahedral and dodecahedral sites - Ferrimagnetic
- Large magneto-optical effect due to strong
charge-transfer transition - Enhancement of magneto-optical effect by
Bi-substitution at the dodecahedral site
27Electronic level diagram of Fe3 in magnetic
garnets
28Experimental and calculated magneto-optical
spectra of Y3Fe5O12
29Electronic states and optical transitions of Co2
and Co3 in Y3Fe5O12
30Theoretical and experimental magneto-optical
spectra of Co-doped Y3Fe5O12
31Theoretical and experimental MO spectra of bcc Fe
Katayama
Krinchik
theory
32MO spectra of PtMnSb
Magneto-optical Kerr rotation ?K and ellipticity
?K
Off-diagonal Dielectric function
Diagonal dielectric functions
(a)
(b)
(c)
33Comparison of theoretical and experimental
spectraof half-metallic PtMnSb
After Oppeneer
34Magneto-optical spectra of CdMnTe
35Pt/Co superlattices
36MO spectra in RE-TM (1)
37MO spectra in R-Co
38MO spectra of Fe/Au superlattice
39Calculated MO spectra of Fe/Au superlattice
By M.Yamaguchi et al.
40Au/Fe/Au sandwich structure
By Y.Suzuki et al.
414. Recent Advances in Magneto-Optics
- Nonlinear magneto-optics
- Scanning near-field magneto-optical microscope
(MO-SNOM) - X-ray magneto-optical Imaging
42NOMOKE(Nonlinear magneto-optical Kerr effect)
- Why SHG is sensitive to surfaces?
- Large nonlinear magneto-optical effect
- Experimental results on Fe/Au superlattice
- Theoretical analysis
- Future perspective
43MSHG Measurement System
44Optical arrangements
Sample
????
Sample stage
w (810nm)
Pole piece
P-polarized or S-polarized light
45
Rotating analyzer
w (810nm)
Analyzer
Filter
2w (405nm)
45Azimuthal dependence of
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
MSHG
linear
45?
SHG intensity (counts/10sec.)
SHG intensity (counts/10sec.)
(a) Linear (810nm)
(b) SHG (405nm)
Fe(3.75ML)/Au(3.75ML) ???? (Pin
Pout)??????????????????
46Calculated and experimental patterns x3.5
Dotsexp. Solid curvecalc.
47Nonlinear Kerr Effect
Df 31.1
The curves show a shift for two opposite
directions of magnetic field
Fe(1.75ML)/Au(1.75ML) Sin
48Nonlinear Magneto-optical Microscope
49MO-SNOM(Scanning near-field magneto-optical
microscope)
- Near-field optics
- Optical fiber probe
- Optical retardation modulation technique
- Stokes parameter of fiber probe
- Observation of recorded bits on MO disk
50Near-field
Scattered wave by a small sphere placed in the
evanescent field produced by another sphere
Total reflection and near field
51Levitation control methods
Shear force type
Canti-lever type
52 Collection mode(a) and illumination mode(b)
53SNOM/AFM System
54Recorded marks on MO diskobserved by MO-SNOM
MO image
topography
55MO-SNOM image of 0.2?m recorded marks on Pt/Co MO
disk
Resolution ?
MO image
Line profile
Topographic image
56Reflection type SNOM
P. Fumagalli, A. Rosenberger, G. Eggers, A.
Münnemann, N. Held, G. Güntherodt Appl. Phys.
Lett. 72, 2803 (1998)
57XMCD (X-ray magnetic circular dichroism)
58Magnetic circular dichroism of L-edge
(b)
59Domain image of MO media observed using XMCD of
Fe L3-edge
SiN(70nm)/ TbFeCo(50nm)/SiN(20nm)/ Al(30nm)/SiN(20
nm) MO ??
N. Takagi, H. Ishida, A. Yamaguchi, H. Noguchi,
M. Kume, S. Tsunashima, M. Kumazawa, and P.
Fischer Digest Joint MORIS/APDSC2000, Nagoya,
October 30-November 2, 2000, WeG-05, p.114.
60Spin dynamics in nanoscale region
GaAs high speed optical switch
Th. Gerrits, H. van den Berg, O. Gielkens, K.J.
Veenstra and Th. Rasing Digest Joint
MORIS/APDSC2000, Nagoya, October 30-November 2,
2000, TuC-05, p.24.
61Further Prospects-For wider range of researches-
- Time (t)Ultra-short pulse?Spectroscopy using ps,
fs-lasers, Pump-probe technique - Frequency (?)Broad band width, Synchrotron
radiation - Wavevector (k)Diffraction, scattering,
magneto-optical diffraction - Length (x)Observation of nanoscale magetism,
Appertureless SNOM, Spin-polarized STM, Xray
microscope - Phase (?)Sagnac interferrometer
625. Magneto-optical Application
- Magneto-optical disk for high density storage
- Optical isolators for optical communication
- Other applications
63Magneto-optical (MO) Recording
- RecordingThermomagnetic recording
- Magnetic recording using laser irradiation
- Reading out Magneto-optical effect
- Magnetically induced polarization state
- MO disk, MD(Minidisk)
- High rewritabilitymore than 107 times
- Complex polarization optics
- New magnetic concepts MSR, MAMMOS
64History of MO recording
- 1962 Conger,Tomlinson Proposal for MO memory
- 1967 Mee Fan Proposal of beam-addressable MO
recording - 1971 Argard (Honeywel) MO disk using MnBi films
- 1972 Suits(IBM) MO disk using EuO films
- 1973 Chaudhari(IBM) Compensation point recording
to a-GdCo film - 1976 Sakurai(Osaka U) Curie point recording on
a-TbFe films1980 Imamura(KDD) Code-file MO memory
using a-TbFe films - 1981 Togami(NHK) TV picture recording using
a-GdCo MO disk - 1988 Commercial appearance of 5MO disk (650MB)
- 1889 Commercial appearance of 3.5 MO
disk(128MB) - 1991 Aratani(Sony) MSR
- 1992 Sony MD
- 1997 Sanyo ASMO(5 6GBL/G, MFM/MSR) standard
- 1998 Fujitsu GIGAMO(3.5 1.3GB)
- 2000 Sanyo, Maxell iD-Photo(5cmf730MB)
65Structure of MO disk media
Polycarbonate substrate
SiNx layer for protection and MO-enhancement
Al reflection layer
MO-recording layer (amorphous TbFeCo)
Land
Groove
Resin
66MO recording How to record(1)
- Temperature increase by focused laser beam
- Magnetization is reduced when T exceeds Tc
- Record bits by external field when cooling
M Tc
Temp
Tc
Laser spot
MO media
External field
Coil
67MO recording How to record(2)
- Use of compensation point
- writing
- Amorphous TbFeCo
- Ferrimagnet with Tcomp
- HC takes maximum at Tcomp
- Stability of small recorded marks
Hc
M
Tb
FeCo
Mtotal
Fe,Co
T
Tcomp
Tc
Tb
RT
68??????TbFeCo??
69Two recording modes
- Light intensity modulation (LIM) present MO
- Laser light is modulated by electrical signal
- Constant magnetic field
- Elliptical marks
- Magnetic field modulation (MFM)MD, ASMO
- Field modulation by electrical signal
- Constant laser intensity
- Crescent-shaped marks
70Shape of Recorded Marks
71MO recording How to read
- Magneto-optical conversion of magnetic signal to
electric signal
D1
-
LD
D2
Differential detection
Polarized Beam Splitter
72Structure of MO Head
73Advances in MO recording
- Super resolution
- MSR
- MAMMOS/DWDD
- Use of Blue Lasers
- Near field
- SIL
- Super-RENS (AgOx)
74MSR(Magnetically induced super-resolution)
- Resolution is determined by diffraction limit
- d0.6?/NA, where NAn sin a
- Marks smaller than wavelength cannot
- be resolved
- Separation of recording and reading layers
- Light intensity distribution is utilized
- Magnetization is transferred only at the heated
region
d
75Illustration of 3 kinds of MSR
76AS-MO standard
77iD-Photo specification
78MAMMOS(magnetic amplification MO system)
79Super-RENSsuper-resolution near-field system
- AgOx filmdecomposition and precipitation of Ag
- Scattering center?near field
- Ag plasmon?enhancement
- reversible
- Applicable to both phase-change and MO recording
??????
?????
80To shorter wavelengths
- DVD-ROM Using 405nm laser, successful play back
of marks was attained with track pitch
0.26?m?mark length 213?m (capacity 25GB) using
NA0.85 lens i? - i M. Katsumura, et al. Digest ISOM2000, Sept.
5-9, 2000, Chitose, p. 18. - DVD-RW Using 405nm laser, read / write of
recorded marks of track pitch0.34?m and mark
length0.29?m in 35?m two-layered
disk(capacity27GB) was succeeded using NA0.65
lens, achieving 33Mbps transfer rate ii ?ii
T. Akiyama, M. Uno, H. Kitaura, K. Narumi, K.
Nishiuchi and N. Yamada Digest ISOM2000, Sept.
5-9, 2000, Chitose, p. 116.
81Read/Write using Blue-violet LD and SIL (solid
immersion lens)
NA1.5 405nm 80nm mark 40GB
SILhead
405nm LD
I. Ichimura et. al. (Sony), ISOM2000 FrM01
82SIL (solid immersion lens)
83Optical recording using SIL
84Hybrid Recording
405nm LD
Recording head (SIL)
Readout MR head
Achieved 60Gbit/in2
H. Saga et al. Digest MORIS/APDSC2000, TuE-05,
p.92.
TbFeCo disk
85 Optical elements for fiber communication
- Necessity of optical isolators
- Principles of optical isolators
- Structure of optical isolators
- Polarization-independent type
- Polarization-dependent type
- Optical multiplexing and needs of optical
isolators
86Optical circuit elements proposed by Dillon
87Optical isolator for Laser diode module
88Optical fiber amplifier and optical isolator
89Optical Circulator
90Optical add-drop and circulator
91Polarization dependent isolator
92Polarization independent isolator
93Magneto-optical circulator
94Optical absorption in YIG
95Waveguide type isolators
96Mach-Zehnder type isolator
97Current-field sensor
98Current sensors used by power engineers
99Field sensor using optical fibers
100SUMMARY
- Basic concepts of magneto-optics are described.
- Macroscopic and microscopic origins of
magneto-optics are described. - Some of the recent development of magneto-optics
are also given. - Some of the recent application are summarized.