schuller group - electrical and computer...
TRANSCRIPT
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SCHULLER GROUP Nanoscience: Thin Film, Lithography
Magnetism: Exchange Bias, Tunneling, Transport
Superconductivity: Pinning,Photoinduced,Search
Superlattices: Metal, Organic, Oxides, Semicond.
Organics: Metallo-Phthalocyanines
Oxides: Transition Metals, Perovskites,
Applications: Sensors, Storage, Magnetic devices
Movies and Plays
http://ischuller.ucsd.edu
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Enjoy the Process
•Caminante no hay camino, se hace el camino al andar.
Antonio Cipriano José María y Francisco de Santa Ana Machado y Ruiz
(26 July 1875 – 22 February 1939)
•Wanderer, there is no road,the road is made by walking.
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VERY INTERESTING
50 100 150
-1.0
-0.5
0.0
0.5
1.0
M /
MS
Temperature (K)TN
AFFM
H HFC=1kOe
Proximity Between Dissimilar Magnets
Anomalous Spontaneous Reversal in Magnetic Heterostructures, Z.-P. Li, J. Eisenmenger, C. W. Miller and Ivan K. Schuller, Phys. Rev. Lett. 96, 137201 (2006).
UNDERSTANDING CRUCIAL
TN<< TC
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PLEASE ASK QUESTIONSWhy ?
• Keeps you focused• Keeps you awake• You learn more• Develop interest
Feed Back Please
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35 Years of
Metallic Superlattices
DOENSF, AFOSR, ONR
IVAN K. SCHULLER
IEEE Distinguished Lecturer
IEEE Magnetics Society Home Page: www.ieeemagnetics.org– 3000 full members– 300 student members
The Society– Conference organization (INTERMAG, MMM, TMRC, etc.)– Student support for conferences– Large conference discounts for members– Graduate Student Summer Schools– Local chapter activities– Distinguished lectures
IEEE Transactions on Magnetics– ~2000 peer reviewed pages each year– Electronic access to all IEEE Transactions on Magnetics papers
Online applications for IEEE membership: www.ieee.org/join– 360,000 members – IEEE student membership IEEE full membership
The Journal of Your Field
On line at ieeexplore.ieee.orgSubmit manuscripts at mc.manuscriptcentral.com/maglet‐ieee
Peer reviewed
Rapid publication
Worldwide circulation
IEEE Xplore archive
Four‐page articles
No page charges
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L. Esaki and R.Tsu, IBM J. Res. Dev. 14,61(1970)
35 years
of
Metallic Superlattices
(Fe/Cr)N Nb SiO2
I I
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JUNIOR
UCSD ARGONNE LABS BELGIUMJose Colino Cornell Chun Kristian TemstKai Liu Hitoshi Homma Hans VanderstraetenMarie-Claire Cyrille Indrajit Banerjee M. GijsArjang Fartash M.R. Khan J.-P. LocquetIatneng Chan Yves Lepetre W. SevenhansAlberto Fernandes J. MurduckEric Fullerton T.R. WernerJosé M. Gallego Q.S. YangDoris Girata G.-G. ZhengElvira Gonzalez Jia-Qi ZhengJulio Guimpel Eric ZieglerSihong KimDavid LedermanChris LeightonJosé I. MartínTim MoranOsamu NakamuraMaría VélezJosep Nogués
LONG TERM
Yvan BruynseraedeRicardo RamirezMiguel KiwiJose VicentK.V. Rao
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U C T )
T E
AP
PL
ICA
TIO
NS
Hard disk drives
MRAM
Sensors
SC
IEN
CE
Co
Cu
I
State: +1
State: 0
State: -1
-4 -3 -2 -1 0 1 2 3 4
-1
0
1 HFC (kOe) 0.5 2.0 5.0
M /
MS
H (kOe)
GMR SPIN TORQUE
EXCHANGEBIAS
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Increased Exchange Anisotropy due to Interface Disorder in Permalloy/CoO, T.J. Moran, J.M. Gallego, and Ivan K. Schuller,
Jour. Appl. Phys. 78, 1887 (1995).
15Source: ISI Web of Knowledge, July 8, 2011
1960 1970 1980 1990 2000 20100
300
600
900
Total # of records: 7174
After 2000: 6062
Rec
ord
Cou
nt
Publication Year
"Exchange Bias" in topic
In 2050 everybodyWill be workingOn exchange bias
Unemployment Solved
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PLAN• Introduction and History
• Characterization
• Interface Effects:
Structural length scale different from magnetic• Long Length Scales- Superlattice Effect:
Collective Magnons in M/N • Short Length Scales- Superlattice effects:
Oscillations in Resistivity• Future
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One layer
Two layers
Three layers
Many layers, N
DisorderConfinementLower dimensionality
InterfacesElectron transferStrainsProximity effects
CouplingDimensional transitionsSpin Transmission
Superlattice effects
WHY DO ALL THIS ?
320 340 360101
102
103
104
105
106
107 100 nm VO2
film
Cooling
R(
)
Temperature (K)
Heating
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VO2
~ 0.32% Volume Change
V2O3
100 120 140 160 180 200102
103
104
105
106
107
108
Cooling
R (
)
Temperature (K)
Heating
100 nm V2O3 film
1.4% Volume Change
Dimers to Single AFM to Para
Peierls Slater
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DICTIONARY• Heterostructure(incoherent)
• Multilayer(long wavelength coherence)
• Superlattice(atomic scale coherence)
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ATOMSSOLIDS
DUE TO THE ADDED PERIODICITYNEW EFFECTS APPEAR IN THE
ELECTRONIC PROPERTIES
FILMS SUPERLATTICES
SUPERLATTICE EFFECTS!
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STRUCTURE vs. PROPERTIES
• POSTULATEProperties of a solid are given by the atomic locations
• SMALL STRUCTURAL CHANGESLarge effects on Physical Properties
•EXAMPLE2% expansion in lattice 100% change in elastic constant
CHARACTERIZE QUANTITATIVELY AT THE ATOMIC SCALE
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MAGNETISM
MgOFeFFeAl
2
glass
Untwinned TwinnedIn-plane
polycrystalline
FeF2
FeAl
ZnF2
bulk FeF2
MgOFeFFeAg
2
ALL 110 FeF2
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STRUCTURE
“DETERMINE THE POSITIONS OF ALL THEATOMS IN THE MATERIAL”
Find out: - Expansions- Interdiffusion- Roughness- etc.
• ELECTRON MICROSCOPY• DIFFRACTION
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Z
X-Y
1Å 10Å 100Å 1000Å 1m 10m
1Å 10Å 100Å 1000Å 1m 10m
Magnetism
Transport
Superconductivity
exchange
screeningRKKY dipolar
spin diffusionmean free path
coherencepenetration depth
ion mill surface analysis
x-ray diffractionneutron diffraction
transmission electron microscopy
x-ray diffractionneutron diffraction
transmission electron microscopyscanning electron microscopy
scanning probe microscopy
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WHY CAREABOUT
STRUCTURE ?•Nothing is Perfect nor As Expected
•Small structural changes give BIG effects in
the Physical Properties
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-3000 -2000 -1000 0 1000 2000 3000
-0.0005
0.0000
0.0005
150 K
Long
Mom
ent (
emu)
Field (Oe)
-3000 -2000 -1000 0 1000 2000 3000
-0.0005
0.0000
0.0005
120 K
Long
Mom
ent (
emu)
Field (Oe)-3000 -2000 -1000 0 1000 2000 3000
-0.0005
0.0000
0.0005
110 K
Long
Mom
ent (
emu)
Field (Oe)-3000 -2000 -1000 0 1000 2000 3000
-0.0005
0.0000
0.0005
100 K
Long
Mom
ent (
emu)
Field (Oe)-3000 -2000 -1000 0 1000 2000 3000
-0.0005
0.0000
0.0005
80 K
Long
Mom
ent (
emu)
Field (Oe)-3000 -2000 -1000 0 1000 2000 3000
-0.0005
0.0000
0.0005
40 K
Long
Mom
ent (
emu)
Field (Oe)-3000 -2000 -1000 0 1000 2000 3000
-0.0005
0.0000
0.0005
10 K
Long
Mom
ent (
emu)
Field (Oe)
Field Cooling 1000 Oe
Py-V2O3 Bilayer
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-3000 -2000 -1000 0 1000 2000 3000
-0.0005
0.0000
0.0005
10 K 40 K 60 K 70 K 80 K 90 K 100 K 110 K 120 K 150 K
Long
Mom
ent (
emu)
Field (Oe)
Field Cooling 1000 Oe
J. De la Venta, M. Erehkinsky, R. Morales, IKS, Phys. Rev. 2013
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-800 -400 0 400 800
MO
KE (a
rb. u
nits
)
H (Oe)-400 -200 0 200 400
MO
KE (a
rb. u
nits
)
H (Oe)
Py (30 nm)
Py (30 nm)V2O3 (100 nm)
Kerr Effect
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10 20 30 40 50 60 70 80 90 100
2 degrees)
* V2O3
▼FM (Py or Ni)
● New Phase●●
▼
▼●*
Py (30nm) /V2O3(100 nm)
Ni (30nm) /V2O3(100 nm)X-
Ray
Int
ensi
ty
Unexpected FeO phase
STRUCTURE IS IMPORTANT
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Capability Neutrons Synchrotron Electron Micr Scanning Probe
Magnetic structure ☺☺☺ ☺☺ ☺☺☺Element specificity ☺☺☺ ☺☺ ☺☺Isotope sensitivity ☺☺☺ ☺Energy tuning ☺☺☺ ☺☺Inelastic ☺☺☺ ☺ ☺Intensity ☺ ☺☺☺ ☺☺Time dependence ☺ ☺☺☺ ☺
TECHNIQUES & CAPABILITIES
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Sample Neutrons Synchrotron E- microscopy Scanning Probe
Destructive ☺☺☺ ☺☺ ☺☺☺Smallest size ☺ ☺☺☺ ☺☺ ☺☺☺Homogeneity ☺ ☺☺☺ ☺☺Environment ☺☺☺ ☺☺☺ ☺
Heating ☺ ☺ ☺Interfaces ☺☺☺ ☺ ☺
SAMPLE VIEWPOINT
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How well do we need to know the structure ???
Compare to Physical Length Scaleand ……….
Always remember limitations
PHILOSOPHYEffects are interesting either if they:
Cannot be explained as disorderOr
Connected quantitatively to the structure
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Physics Driving Force
• Surfaces• Quantization
NANO, Nano, nano, nano
Proximity• Extension of
• Extension of M
STRUCTURAL DETERMINATION
QuantitativeAppropriate Length Scale
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SMALL CHANGES IN THE STRUCTURECAN PRODUCE
LARGE EFFECTS IN THE PHYSICS
Remember limitations of techniques
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Magnetic & Nonmagnetic Roughness
Mo/Ni SuperlatticesCollaborators
J. Cable, ORNLM. Khan, G. Felcher, ANL
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Polarized Neutron ScatteringMo/Ni Superlattices
SquareModulation
ExperimentalFlippingRatio
All possiblemodels
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Mo/Ni Superlattices
J. W. Cable, M.R. Khan, G. Felcher, I. K. Schuller, Phys. Rev. B34, 1643(1986)
“A comparison of X-ray and neutron diffraction implies that the magnetic profile in the superlattice is more perfect than the chemical profile.”
Mo
Ni
Mo
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So six blind men of Hindustan disputed loud and long,Each in his own opinion exceeding stiff and strong;
Though each was partly in the right,
they all were in the wrong!
Syādvāda (Devanagari:
यादवाद)Jain Philosphy
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SYSTEMATIC STUDIES ESSENTIAL
• Quantitative (Structure,….. )• Systematic (One parameter at a time)• Different measurements on same samples• Reevaluate (Even well accepted “facts”)
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One layer
Two layers
Three layers
Many layers, N
DisorderConfinementLower dimensionality
InterfacesElectron transferStrainsProximity effects
CouplingDimensional transitionsSpin Transmission
Superlattice effects
WHY DO ALL THIS ?
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Exchange Bias
FM
Free FMExchange field HE=0Small coercivity HCSymmetricUniform
FMAF
Pinned FMLarge HELarge HC
HE
2HC
H
M
H
M
60
200 nm
20 40 60 80 100
T (K)
FM/AF/FMParallel
PyFeF2
Ni
PyFeF2
Ni
Anti-parallel
20 40 60 80 100
0
100
200
300
400
HE
B (O
e)
T (K)
Ni
-2 -1 0 1 2
-1.0
-0.5
0.0
0.5
1.0
HvEB=66.5mT
HbEB=40.9mT
M/M
sMagnetic Field (kOe)
T=10K
Radiation Damage
320 340 360101
102
103
104
105
106
107 100 nm VO2
film
Cooling
R(
)
Temperature (K)
Heating
63
VO2
~ 0.32% Volume Change
V2O3
100 120 140 160 180 200102
103
104
105
106
107
108
Cooling
R (
)
Temperature (K)
Heating
100 nm V2O3 film
1.4% Volume Change
-300 -200 -100 0 100 200 300
-400
-200
0
200
400
180 K 190 K 200 KM
agne
tizat
ion
(em
u cm
-3)
Magnetic Field (Oe)
100 150 200 250406080
100120140160180200220
Coe
rciv
ity (O
e)
Temperature (K)
Heating Cooling
Metal Insulator Transition + Structural Phase TransitionInterface Coupling in Ni/V2O3
Change of M and Hc at MIT and SPT
V2O3 (100 nm)
Ni (10 nm)
Al2O3 Substrate
-300 -200 -100 0 100 200 300
-400
-200
0
200
400
165 K 170 K 175 K 180 K 190 K 200 K
100 K 120 K 140 K 150 K 155 K 160 K
Mag
netiz
atio
n (e
mu
cm-3)
Magnetic Field (Oe)
100 150 200 250406080
100120140160180200220
Coe
rciv
ity (O
e)
Temperature (K)
Heating Cooling
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-300 -200 -100 0 100 200 300
-400
-200
0
200
400
165 K 170 K 175 K 180 K 190 K 200 K
150 K 155 K 160 K
Mag
netiz
atio
n (e
mu
cm-3)
Magnetic Field (Oe)
100 150 200 250406080
100120140160180200220
Coe
rciv
ity (O
e)
Temperature (K)
Heating Cooling
-300 -200 -100 0 100 200 300
-400
-200
0
200
400
165 K 170 K 175 K 180 K 190 K 200 KM
agne
tizat
ion
(em
u cm
-3)
Magnetic Field (Oe)
100 150 200 250406080
100120140160180200220
Coe
rciv
ity (O
e)
Temperature (K)
Heating Cooling
65
One layer
Two layers
Three layers
Many layers, N
DisorderConfinementLower dimensionality
InterfacesElectron transferStrainsProximity effects
CouplingDimensional transitionsSpin Transmission
Superlattice effects
WHY DO ALL THIS ?
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Magnetotransport in Superlattices
CollaboratorsC. Falco, ANL
J. Hilliard, J. Ketterson, B. Thaler, NorthwesternR. Lacoe, R. Dee, UCLA
69
e e-GMR in Fe/Cr superlattices
-1.5 -1.0 -0.5 0.0 0.5 1.0 1.5
0
2
4
6
8
10
RP
RAP
BS
R/R
P[%
]
B [T]
M. N. Baibich et al Phys. Rev. Lett.61, 2472 (1988)
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DON’T LET YOUR ELDERS DEPRESS YOU !!!!
•Pushing the Limits is Important•Make New Materials
•Something will happen
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One layer
Two layers
Three layers
Many layers, N
DisorderConfinementLower dimensionality
InterfacesElectron transferStrainsProximity effects
CouplingDimensional transitionsSpin Transmission
Superlattice effects
WHY DO ALL THIS ?
73
PROPERTIES WHICH DEPENDON THE SUPERLATTICE NATURE ?
Relevant Length scale?
1. X-rays Sensitive to disorder !
2. Magnons Long length scaleDipolar ~ 200 Å
M. Grimsditch, M. Khan, A. Kueny, IKS, Phys.Rev.Lett. 51, 498(1983)
3. Resistivity Very high compared to bulkMonotonic vs. Periodicity (
RESISTORS IN PARALLEL
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SUPERLATTICE EFFECTS IN THETRANSPORT PROPERTIES
COLLABORATORSSihong KimJ.M. GallegoD. Lederman
UCSD
Work supported byDOE
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ATOMSSOLIDS
DUE TO THE ADDED PERIODICITYNEW EFFECTS APPEAR IN THE
ELECTRONIC PROPERTIES
FILMS SUPERLATTICES
SUPERLATTICE EFFECTS!
79
One layer
Two layers
Three layers
Many layers, N
DisorderConfinementLower dimensionality
InterfacesElectron transferStrainsProximity effects
CouplingDimensional transitionsSpin Transmission
Superlattice effects
WHY DO ALL THIS ?
80
INTERESTING QUESTIONS1. Extended Electronic States?
• Signature
2. Interaction Effects?• Phase in Ferromagnetic/Superconducting
3. Confinement of Collective Excitations?• Magnons, Phonons, etc.
4. Proximity Effects?• Magnetism
5. Growth• Kinetics vs. Thermodynamics
6. Pinning
7. Spin Transport