ctem/sem principles - cime | epfl · advantages and disadvantages of scanning beam microscopy tem ...
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MSE-603 Autumn 2013 STEM Marco Cantoni
15/16. STEM, EDX & HAADF
Scanning Transmission Electron Microscopy
a) STEM, principle, basics,TEM / STEM with the same instrument
Transmission Electron Microscopya Textbook for Materials ScienceDavid B. Williams and Barry Carter
ISBN 0-306-45247-2
b) Analytical Electron Microscopy (AEM)Practical Analytical Electron Microscopy in Materials Science
David B. WilliamsISBN 0-9612934-0-3
c) High angle annular dark-field, HAADFZ-contrast
Handbook of Microscopy, Methods IIS. Amelinckx, D. van Dyck, J. van Landuyt, G. van Tendeloo
ISBN 3-527-27920-2
MSE-603 Autumn 2013 STEM Marco Cantoni
CTEM/SEM principles
Conventional TransmissionElectron Microscope
ScanningElectron Microscope
Slide Projector TV
What you see is what
the detector sees !!!
MSE-603 Autumn 2013 STEM Marco Cantoni
TEM-SEMinteraction of electrons with the sample
Specimen
Inci
dent
bea
m
Auger electrons
Backscattered electronsBSE
secondary electronsSE Characteristic
X-rays
visible light
“absorbed” electrons electron-hole pairs
elastically scatteredelectrons
direct beam inelasticallyscattered electrons
BremsstrahlungX-rays
1-100nm
MSE-603 Autumn 2013 STEM Marco Cantoni
Detectorsin S(T)EM
• Secondary Electrons
• Backscattered Electrons
• X-rays
• EELS
• Bright field
• Dark field
• (Absorbed current)
MSE-603 Autumn 2013 STEM Marco Cantoni
Advantages and disadvantages of Scanning Beam Microscopy
TEM <-> STEM (SEM)
Advantages
• Parallel detection of different signals
• Easy positioning of the beam (EDX, EELS)
• Small interaction volume, High energy (EDX)
Disadvantages
• Longer acquisition times(line by line)
• Image distortions (deflection coils)
• More complicated alignment procedure
• More expensive…
MSE-603 Autumn 2013 STEM Marco Cantoni
a) Principle
MSE-603 Autumn 2013 STEM Marco Cantoni
STEM <-> (C)TEM
MSE-603 Autumn 2013 STEM Marco Cantoni
Reciprocity
A B
Sou
rce
Det
ecto
r
Spe
cim
en
Lens
A B
CTEM
Cowley (1969): for the same lenses, apertures and system dimension the image contrast must be the same for CTEM and STEM
2STEM = 2CTEM
2STEM = 2 CTEM
STEM
Lens
22
22
Cowley, 1989
MSE-603 Autumn 2013 STEM Marco Cantoni
Illumination / opticsTEM / STEM with the same instrument
MSE-603 Autumn 2013 STEM Marco Cantoni
Source
Illumination
Scanning
“descanning” / Detection
MSE-603 Autumn 2013 STEM Marco Cantoni
Beam current versus probe size
100keV electron beam: beam current:1nA, probe size: 1nm
150MW/mm2 !!!
Field emission guns• provide high emission current• from a small source (~1nm)• require small demagnification
->small probe size
MSE-603 Autumn 2013 STEM Marco Cantoni
Diffraction pattern = stationary patternBF/DF detectors
MSE-603 Autumn 2013 STEM Marco Cantoni
MSE-603 Autumn 2013 STEM Marco Cantoni
Au particles on a C filmSTEM BF:
Detection of transmitted electrons:
contrast similar to
CTEM BF image (objective aperture
selects only transmitted electrons)
STEM ADF:
Detection of diffracted electrons on the annular
DF detector:
(integration of multiple CTEM DF images)
Diffraction pattern
MSE-603 Autumn 2013 STEM Marco Cantoni
Bright field/ AnnularDark field detectorinfluence of camera length and convergence angle
The selected camera-length (magnification of the diffraction pattern) determines what the detectors “sees”
Big camera length small camera length
ADF
BF
MSE-603 Autumn 2013 STEM Marco Cantoni
Bright field TEM <->STEM
MSE-603 Autumn 2013 STEM Marco Cantoni
Bright field TEM STEM
CTEMCTEM
Effect of increasing detection angle (decreasing camera length)on STEM BF image contrast: Loss of dynamical diffraction contrast
STEM
STEM
STEM
MSE-603 Autumn 2013 STEM Marco Cantoni
ADF STEM
• The ADF image provides a signal which depends strongly on the bragg scattering (Al2O3).
• Single atoms scatter electrons incoherently to higher angles~ “z-contrast”
Single atoms (or small groups of atoms) of Pt on
crystalline Al2O3
MSE-603 Autumn 2013 STEM Marco Cantoni
b) Analytical Electron Microscopy(EDS)
• Thin samples -> correction factors weak (A and F can be neglected), quantification “easy”
• Very weak beam broadening -> high spatial resolution ~ beam diameter (~nm)
• STEM: beam control and positioning
MSE-603 Autumn 2013 STEM Marco Cantoni
Interaction volumeSEM (30KeV), bulk
versusTEM (300KeV), thin film
PZT ceramics
bulk
20nm thick PZT
Small interaction volume -> high spatial resolution for EDX Analysis!
TEM
MSE-603 Autumn 2013 STEM Marco Cantoni
STEM point analysisPbMg1/3Nb2/3O3 (bulk)
Processing option : Oxygen by stoichiometry (Normalised)
Spectrum Mg Si Nb Pb O Total Spectrum 1 30.02 13.32 56.66 100.00 Spectrum 2 19.15 7.96 4.11 11.72 57.06 100.00 Spectrum 3 6.01 12.49 22.13 59.37 100.00 Spectrum 4 5.65 12.39 22.67 59.29 100.00 Spectrum 5 5.63 12.48 22.52 59.36 100.00 Spectrum 6 5.98 13.66 20.11 60.25 100.00 Spectrum 7 5.55 12.45 22.66 59.34 100.00 Spectrum 8 5.49 12.96 21.84 59.72 100.00 Spectrum 9 5.63 12.19 23.04 59.14 100.00 Max. 30.02 13.32 13.66 23.04 60.25 Min. 5.49 7.96 4.11 11.72 56.66
All results in Atomic Percent
MSE-603 Autumn 2013 STEM Marco Cantoni
Pb(Zr,Ti)O3 Thick films for MEMS
SEM image of a wet etched (in HF/HCl solution) side-wall of 2 µm PZT film. All the 8 interfaces corresponding to the intermediate crystallization steps became visible indicating a compositional gradient (preferential etching) across the PZT layers.
MSE-603 Autumn 2013 STEM Marco Cantoni
CTEM dark field image STEM dark field
STEM dark field images. The ramps in the gray level indicate changes of density or chemical composition (~atomic number).
TEM dark field images. Strong diffraction contrast
MSE-603 Autumn 2013 STEM Marco Cantoni
EDX Line-scan
MSE-603 Autumn 2013 STEM Marco Cantoni
EDX point analysis
Quantitative EDX Analysis of the points indicated in the imageProcessing options : Oxygen by stoichiometry (normalised)results a Percent
SpectrumZr Ti Pb O Total Zr/Ti
1 8.43 12.60 18.45 60.52 100.0 40/60
2 9.92 9.98 20.15 59.95 100.0 49/51
3 12.07 7.61 20.49 59.84 100.0 61/39
MSE-603 Autumn 2013 STEM Marco Cantoni
STEM Element MappingPMN/PT 90/10 (bulk)
MSE-603 Autumn 2013 STEM Marco Cantoni
Artifactshow to recognize/minimize them
MSE-603 Autumn 2013 STEM Marco Cantoni
Analytical TEM of multifilamentNb3Sn superconducting wires
Prof. R. Flükiger, V. Abächerli, D. Uglietti, B. SeeberDept. Condensed Matter Physics (DPMC),University of Geneva
Typical cable:1 x 1.5mm cross-section121x121 filaments of Nb3Snin a bronze (Cu/Sn) matrix
0.5 mm
Superconducting Nb3Sn cables for high magnetic fields 10-20T:increase current density, lower costPotential Applications:NMR, Tokamak fusion reactorsLarge Hadron Collider (LHC), CERN
MSE-603 Autumn 2013 STEM Marco Cantoni
Processing„bronze route“
Nb3Sn
Nb
Cu,Sn
Nb
Cu,Snbronze
Hea
t tre
atm
ent
SEM: reacted filament (1 out of 14‘000)
Ti
Ti
Ta
“Nano”-engineering: controlled creation of “imperfections” of nm scale (coherence length)
Cu and Ti are believed to play an important role at the grain boundaries: „dirty“ grain boundaries = pinning
• Is it possible to detect Cu and Ti at the grain boundaries ?• What is the difference between the grain boundaries
depending on where the additives are added to the unreacted material ?
MSE-603 Autumn 2013 STEM Marco Cantoni
Typical problems:thinning of heterogeneous specimens:
selective thinning
Cross-section, polished mechanicallyto 30 um, ion milled until perforation
STEM, Dark field:core of filament too thick, preferential etching of bronze matrix
Nb3Sn filament
bronze
MSE-603 Autumn 2013 STEM Marco Cantoni
Specimen preparation by focused Ion Beam (FIB):large areas with uniform thickness ideally for EDX Analysis
in the TEM (STEM mode)
SEM (FIB)
STEM, Bright field
Ion milling
FIB
ED
S, e
lem
ent
map
s
STEM-DF
Sample #21
15um
thickness:40-50nm
MSE-603 Autumn 2013 STEM Marco Cantoni
Spot analysisLine profile
Point Ti%at
Nb%at
Sn %at Ta%at
1 0.1 79.7 17.1 2.9
2 0.4 79.2 17.8 2.4
3 0.8 77.8 18.5 2.7
4 1.8 75.1 20.8 2.1
5 0.5 76.5 20.9 1.9
6 0.2 74.3 23.1 2.2
7 1.6 73.1 23.4 1.7
8 1.2 73.7 22.8 2.1
9 0.9 70.4 26.4 2.1
Sample #21
Tc/Jc„useful“
bronzeNb
Sn
„Nb3Sn“
MSE-603 Autumn 2013 STEM Marco Cantoni
grain boundaries ? Ti/Cu
Sample #21
Cu
Sn
TaTi
Nb
Cu and Ti at the grain boundaries:
width ~ coherence lenght (4nm)
possible pinning centers !!
EDX line-scan
MSE-603 Autumn 2013 STEM Marco Cantoni
grain boundary without Ti
Sample #24
Cu
Sn
TiTa
Nb
Quantitative Line-scan
MSE-603 Autumn 2013 STEM Marco Cantoni
New possibilities due toSDD (silicon drift detector) technology
X-rays
SDD Si(Li)Thickness 300-400µm 3mm
Area 30,50,80mm2 30mm2
Det. Interval 4-10µsec. 50-100µsec.Speed: 100’000cps 10’000cps
Cooling Peltier Liq. N
SDD
MSE-603 Autumn 2013 STEM Marco Cantoni
TECNAI OSIRISAnalytical TEM2012 @ CIME 5x
10x
electrons
Det. area
MSE-603 Autumn 2013 STEM Marco Cantoni
400x400 pixels (5umx5um)160’000 spectra4msec., (10min.)
2.5nA
Nb
Cu
Sn
MSE-603 Autumn 2013 STEM Marco Cantoni
• 400x400 pixels (500nmx500nm)
• 160’000 spectra
• 4msec., (10min.), 2.5nA
CuSTEM DF Sn
MSE-603 Autumn 2013 STEM Marco Cantoni
Synthetic sapphire: Al2O3
Al2O3with La (250ppm) in the grain boundaries
Paul Bowen, M. StuerEPFL-LPT
MSE-603 Autumn 2013 STEM Marco Cantoni
HAADF STEM
La at grain boundaries
Cl (from synthesis)
MSE-603 Autumn 2013 STEM Marco Cantoni
QUALITATIVE EDX Mapping:
GREAT!
MSE-603 Autumn 2013 STEM Marco Cantoni
c) High Angle Annular Dark Fieldz-contrast
(atomic resolution)
Ultramicroscopy 30 (1989) 58-69North-Holland, AmsterdamZ-CONTRAST STEM FOR MATERIALS SCIENCES.J. PENNYCOOK
Ultramicroscopy 37 (1991) 14-38;North-HollandHigh-resolution Z-contrast imaging of crystalsS.J. Pennycook and D.E. Jesson
MSE-603 Autumn 2013 STEM Marco Cantoni
MSE-603 Autumn 2013 STEM Marco Cantoni
High Angle Annular Dark field detector
Big camera length small camera length
ADF
BF
HAADF
MSE-603 Autumn 2013 STEM Marco Cantoni
High angle incoherent scattering
The annular DF detector is placed beyond the bragg-scattered electrons…
Small camera length and large diameter of the detectors inner diameter
The image is formed by high angle incoherently
scattered electrons-> Rutherford scattering at
the nucleus of the atoms
z2
Z-Contrast Si nano-crystals in SiO2 formed by implantation
MSE-603 Autumn 2013 STEM Marco Cantoni
HAADF <-> HRTEM
Pt catalyst on Al2O3
Pt particles become visible in the HAADF image
HAADF BF
MSE-603 Autumn 2013 STEM Marco Cantoni
HRTEM STEM-HAADF
HRTEM <-> STEM HAADF
MSE-603 Autumn 2013 STEM Marco Cantoni
Defocus…?
Also for High Resolution STEM-HAADF there is a
defocus value which gives the highest resolution ( =
sharpest peak of maximum intensity).
MSE-603 Autumn 2013 STEM Marco Cantoni
No contrast reversal as in CTEM HRTEM images !!!!no repeated contrast patterns at different defocus settings
MSE-603 Autumn 2013 STEM Marco Cantoni
HAADF-STEM study of β′-type precipitates inan over-aged Al–Mg–Si–Ag alloy
MSE-603 Autumn 2013 STEM Marco Cantoni
MSE-603 Autumn 2013 STEM Marco Cantoni
Chemical analysis on atom columns
MSE-603 Autumn 2013 STEM Marco Cantoni
Cs-corrected STEM
ADF images of Si[112]recorded with
aberration corrected STEMProbe size = 60pm (0.06nm)
Resolution 78pm
Atomic resolutionEELS analysisof defects and interfacesR.F. Klie*, Y. ZhuMicron 36 (2005) 219–231
EELS spectrum ofsingle atom columns
Ti-L edgein SrTiO3 8° grain
boundary