66
Transmission Electron Microscopy -TEM- Scanning Electron Microscopy – SEM - The first electron microscope was built 1932 by the German physicist Ernst Ruska, who was awarded the Nobel Prize in 1986 for its invention. He knew that electrons possess a wave aspect, so he believed he could treat them as light waves. Ruska was aware that magnetic fields affect electron trajectories, possibly focusing them as optical lenses do to light. After confirming these principles he set out to design the electron microscope, which he knew would be much more powerful than an ordinary optical microscope since electron waves were shorter than ordinary light waves. Electrons would therefore allow for greater magnification and to visualize much smaller structures. The first practical electron microscope was built by in 1938 and had 10 nm resolution. Although modern electron microscopes can magnify an object 2 million times, they are still based upon Ruska's prototype. The electron microscope is now an integral part of many laboratories. Researchers use it to examine biological materials (such as microorganisms and cells), a variety of large molecules, medical biopsy samples, metals and crystalline structures, and the characteristics of surfaces.

(Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

  • Upload
    vuduong

  • View
    231

  • Download
    3

Embed Size (px)

Citation preview

Page 1: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Transmission Electron Microscopy -TEM-

Scanning Electron Microscopy – SEM -

The first electron microscope was built 1932 by the German physicist Ernst Ruska, who

was awarded the Nobel Prize in 1986 for its invention.

He knew that electrons possess a wave aspect, so he believed he could treat them as light

waves. Ruska was aware that magnetic fields affect electron trajectories, possibly focusing

them as optical lenses do to light. After confirming these principles he set out to design the

electron microscope, which he knew would be much more powerful than an ordinary

optical microscope since electron waves were shorter than ordinary light waves. Electrons

would therefore allow for greater magnification and to visualize much smaller structures.

The first practical electron microscope was built by in 1938 and had 10 nm resolution.

Although modern electron microscopes can magnify an object 2 million times, they are still

based upon Ruska's prototype.

The electron microscope is now an integral part of many laboratories. Researchers use it to

examine biological materials (such as microorganisms and cells), a variety of large

molecules, medical biopsy samples, metals and crystalline structures, and the

characteristics of surfaces.

Page 2: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Aim of the lecture

Electron Microscopy is a very large and specialist field

Just a few information on

Electron Microscopy

•What is it possible to do •How do instruments work

Page 3: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

HISTORY OF THE TRANSMISSION ELECTRON MICROSCOPE

(TEM)

•1897 J. J. Thompson Discovers the electron

•1924 Louis de Broglie identifies the wavelength for electrons as λ=h/mv

•1926 H. Busch Magnetic or electric fields act as lenses for electrons

History of TEM

•1926 H. Busch Magnetic or electric fields act as lenses for electrons

•1929 E. Ruska Ph.D thesis on magnetic lenses

•1931 Knoll & Ruska 1st electron microscope (EM) built

•1931 Davisson & Calbrick Properties of electrostatic lenses

•1934 Driest & Muller Surpass resolution of the Light Microscope

•1938 von Borries & Ruska First practical EM (Siemens) - 10 nm resolution

•1940 RCA Commercial EM with 2.4 nm resolution

• 2000 new developments, cryomicroscopes, primary energies up to 1 MeV

Page 4: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Scheme of TEM

0.00251

Resolution

(nm)

Wavelength

(nm)

Electrons at 200kV

~0.2

Page 5: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

TEM lens system

Page 6: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Application of magnetic Lenses: Transmission Electron Microscope (Ruska and Knoll 1931)1945 - 1nm resolution

Page 7: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

vm

h

0

2

02

1vmeV =

2

1

2

0

02

12

+

=

cm

eVeVm

−=

2

2

0 1c

vmm

Basis of the transmission electron microscopy

Attention

relativistic

electrons!

Accelerating voltage

(kV)

Nonrelativistic λλλλ

(nm)

Relativistic λλλλ

(nm)

Velocity

(×108 m/s)

100 0.00386 0.00370 1.644

200 0.00273 0.00251 2.086

400 0.00193 0.00164 2.484

1000 0.00122 0.00087 2.823

Page 8: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

βλ

61.0=thr

0.00251~550

Electrons at 200kVGreen light

Wavelength (nm)

Resolution

The resolution of the transmission electron

β= semi-collection angle of magnifying lens

λ= electron wavelength

4

1

4

3

67.0 sCr λ= Best attained resolution ~0.07 nm

Nature (2006)

The resolution of the transmission electron

microscope is strongly reduced by lens aberration

(mainly spherical aberration Cs )

Page 9: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Emitters

tungsten Lanthanum Field emitters: single oriented crystal of thungsten

tungsten Lanthanum hexaboride

crystal of thungstenetched to a fine tip

Page 10: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Thermoionic emitters

=J

Heating current

Emitter

Wehnelt

A virtual probe of size d can beassumed to be present at the

first cross-over

=J

kTc eATd

iJ

Φ−

== 2

2

0

4

π

Brightness: density per unit solid angle

E

x

Anode

0.2 eV

Ω=

πβ

2

0

4

d

ic

4A Area Emitting

2

0dπ=

Page 11: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Schottky and Field emission guns

+

++

Φ−

Φ+Φ= E

eE

J

5.14x108.62

6x102.6µ

µ

Emission occurs by tunnel effect

E=electric field

Φ=work function

µ=Fermi level

•High brilliance •Little cross over•Little integrated current

Page 12: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

CoherenceCoherence: a prerequisite for interference is a superposition of wave systems whose phase difference remains constant in time. Two beams are coherent if, when combined, they produce an interference pattern.

Two beams of light from self luminous sources are incoherent.In practice an emitting source has finite extent and each point of the source can be considered to generate light. Each source gives rise to a source can be considered to generate light. Each source gives rise to a system of Fresnel fringes at the edge. The superposition of these fringe systems is fairly good for the first maxima and minima but farther away from the edge shadow the overlap of the fringe patterns becomes sufficiently random to make the fringes disappear.

The smaller is the source the larger is coherence

Using a beam with more than one single wave vector k (polychromatic beam)

reduces the coherence

Page 13: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

B

Magnetic lenses

B

( )

∞+

∞−

∞+

∞−

=

=

dxxBV

dxxBVf

)(8

8

1 2

ηθ

ηlens with focal length f but with a rotation θ

V acceleration voltage of the electrons

η charge to mass ratio of the electron

Page 14: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Magnetic lenses: bell shaped field(((( ))))2

0

/1 az

BBz

++++====

z

BrB

zr

∂∂∂∂∂∂∂∂

−−−−====2

Newton’s law

3)

2ϕ&&& mrFrm r +=

( ) ϕϕ rFmrdt

d=&

2

zFzm =&&

2ϕϕ && mrreB z +−=

= zBre

dt

d 2

2

ϕ&reB r=

1)

2)

CBre

mr z += 22

2ϕ&from 2): with C=0 for per trajectories

in meridian planes

zBm

e

2====ϕϕϕϕ&

Br is small for paraxial trajectories, eq. 3) gives vz=const, while the coordinate r oscillates with frequency ω=√(1+k2)

rBm

eB

m

emrB

m

ereBrm zzzz

222

422−=

+−=&&

ary /=azx /=

*0

2202

8 Um

aeBk ==== y

x

k

dx

yd22

2

2

2

)1( ++++−−−−====

from 1):

in meridian planes

Page 15: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Aberrations

Spherical aberration 3αδ ss C=

Defocus

αδ ff =

Scherzer: in a lens system with

Chromatic aberration

∆+

∆=

I

I

E

ECCC 2δ

Scherzer: in a lens system with radial symmetry the spherical

aberration can never be completely corrected

Page 16: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Astigmatism

different gradients of the field:different focalization in the two directions

It can be corrected

Other aberrations exist like threefold astigmatism ComaAbut can be corrected or are negligible

Page 17: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Deflection coils

At least two series of coils are necessary to decouple the shift of the beam from its tilt its tilt

Position remains in pwhile different tilts are possible

Position is shifted without changing the incidence angles

Page 18: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Revelators

Scintillator: emits photons when hit by high-energy electrons. The emitted photons are collected by a lightguide and transported to a photomultiplier for detection.

phosphor screen: the electron excites phosphors that phosphor screen: the electron excites phosphors that emit the characteristic green light

CCD conversion of charge into tension. Initially, a small capacity is charged with respect a reference

level. The load is eventually discharged. Each load corresponds to a pixel. The discharge current is proportional

to the number of electrons contained in the package.

Page 19: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Trajectories of 10KeV electrons in matter

GaAs bulk

http://www.gel.usherbrooke.ca/casino/download2.html

Energy released in the matrix

Page 20: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Trajectories of 100KeV electron in a thin

specimen

GaAs thin film

Page 21: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Interaction electronic beam – sample: electron diffraction

backscattering

forwardforward

scattering

Electrons can be focused by electromagnetic lenses

The diffracted beams can be recombined to form an image

Page 22: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Electron diffraction - 1

Diffraction occurs when the Ewald’s sphere cuts a point of the reciprocal lattice

λθ =sin2dBragg’s Law

Page 23: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Electron diffraction - 2

λ1

1 d

L

R=

R

Ld

λ=

Recorded spots correspond mainly to one plane in reciprocal space

Page 24: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Scattering

Fast electrons are scattered by the protons in

the nuclei, as well as by the electrons of the

atoms

X-rays are scattered only by the electrons of

the atoms

Diffracted intensity is concentrated in the forward direction.

Coherence is lost with growing scattering angle.

Page 25: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Electrons (200 kV)

λ = 2.51 pm

r = 2.0·1011 m

Comparison between high energy electron diffraction

and X-ray diffraction

X-ray (Cu Kα)

λ = 154 pm

rE = 3.25·109 m

rE = 2.0·1011 m

Page 26: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Objective lens

The magnetic pre-field of the

objective lens can also be used to

Objective is the most important lens in a TEM, it has a very high field (up to 2 T)

The Specimen is completely immersed in its field so that pre-field and post field can be distinguished

The post field is used to create

image or diffraction from diffracted also be used to

obtain a parallel illumination on the

specimen

from diffracted beams

Page 27: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Diffraction mode

Different directions correspond to different points in the back focal

plane

f

Page 28: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Imaging mode

Different point correspond to different points.

All diffraction from the same point in the sample converge to the same

image in the image plane

Page 29: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Contrast enhancement by single diffraction mode

f

Bright field Dark field

Objective aperture

Page 30: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Dark/bright field images

Dark field Bright field

0.5 m0.5 m

Using 200 Using 022

Page 31: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Diffraction contrast

Suppose only two beams are on

Page 32: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Imaging

Lattice Fringe Image High Resolution Image

Phase contrastAmplitude contrast

Bright Field Image Dark Field Image

Perfect imaging would require the interference of all difffraction

channels. Contrast may however be more important.

Page 33: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Amplitude contrast - 1

Page 34: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Amplitude contrast - 2

Page 35: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Phase contrast in electron microscopy

Fringes indicate two Dim. periodicity

Page 36: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Phase contrast in electron microscopy

What happens if we consider all beams impinging on the same point ? Interference !!!

~

~

FFT

2

2

∑∑∑∑ ΨΨΨΨ====BEAMS

giφφφφ

g a vector of the reciprocal latticeiφ iΦ

gΨΨΨΨ s the component beam scattered by a vector g

But notice that gΨΨΨΨ is the Fourier component of the exit wavefunction 1

2====ΨΨΨΨ∑∑∑∑

BEAMS

g

Indeed each electron has a certain probability to go in the transmitted or diffracted beam. For an amorphous material all Fourier components are possible but in a crystal

only beams with the lattice periodicity are allowed, these are the diffracted beams.

NOTE: the diffraction pattern is just the Fourier transform of the exit wave

Page 37: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Effect of the sample potential V

Phase shift

Amplitude variation

θθθθφφφφ it e====

tt e

µµµµφφφφ −−−−====

Vie Vi

t σφ σ +≈≈ 1

t eφφφφ ====

Example of exit wave function (simulation)

Real part Modulus phase

Page 38: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

(useful for biological specimen which absorb little

radiation but have different diffraction index with

respect to surrounding medium, thus inducing a

phase shift)

Optical Phase Contrast microscope

Image for regular brightfield

objectives. Notice the air bubbles

at three locations, some cells are

visible at the left side

Same image with phase contrast objectives.

White dots inside each cell are the nuclei.

Page 39: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

To build an ideal phase microscope we must dephase (by π/2) all diffracted beams while leaving the transmitted unchanged

Phase adjustment device

Phase contrast in electron microscopy

The device is ~150 µ wide and 30 µ thick. The

unscattered electron beam passes through a drift

tube A and is phase-shifted by the electrostatic

potential on tube/support B. Scattered electrons

passing through space D are protected from the

voltage by grounded tube C.

Page 40: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

An alternative use of the electron microscope is to concentrate the electron beam onto a small area and scan it over the sample. Initially it was developed to gain local chemical information. Actually structural information can be gained, too, since the beam spot can be as small as 1.3 Å.

STEM

Diffraction mode

While scanning the beam over the different part of the sample we integrate over different diffraction patterns. If the transmitted beam is included the method is called STEM-BF otherwise STEM-DF

The dark field image corresponds

to less coherent electrons and

allows therefore for a more

accurate reconstruction

Page 41: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

STEM probe

It depends on aperture , Cs , defocus

2

0

2)()(2max

),0,( ∫=

−−=∆−K

K

rrkiki

probe kdeerrP probe

r

r

rrrr rrr χ

0=K

It is the sum of the waves at different angles, each with its own phase factor.

If there is no aberration the larger is the convergence, the smaller is the probe.

The presence of aberrations limits the maximum value of the convergence angle up to 14 mrad

The different wavevectors contributing to the incoming wave

blur up the diffraction pattern, causing superposition of the spots.

Interference effects are unwanted and smallest at the largest angles

Page 42: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Convergent beam electron diffraction - CBED

The

diffracting

area is <1 nm

in diameter

Page 43: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Chemical analysis: energy dispersive spectrometry

SEM TEM

The electron beam can be focused to obtain a spot less than 500 nm

Page 44: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

EELSUsed to collect spectra and images

Usable in both scanning and tem

mode

Each edge is characteristic for each material

The fine structures of the edge reveal the characteristics of the local environment of the species. If the relevant inelastic event corresponds to a localized interatomic transition, the information is local, too

Page 45: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

EELS analysis

Page 46: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

TomographyBy observing at different angle it it is possible to reconstruct the

3D image

Page 47: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Drawback of TEM: necessity of sample preparation

Ion milling

Milling

Hand milling

Powders

Page 48: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

TEM DEVELOPMENTS

• An additional class of these instruments is the electron cryomicroscope, which includes a specimen stage capable of maintaining the specimen at liquid nitrogen or liquid helium temperatures. This allows imaging specimens prepared in vitreous ice, the preferred preparation technique for imaging individual molecules or macromolecular assemblies.

• In analytical TEMs the elemental composition of the specimen can be • In analytical TEMs the elemental composition of the specimen can be determined by analysing its X-ray spectrum or the energy-loss spectrum of the transmitted electrons.

• Modern research TEMs may include aberration correctors, to reduce the amount of distortion in the image, allowing information on features on the scale of 0.1 nm to be obtained (resolutions down to 0.08 nm have been demonstrated, so far). Monochromators may also be used which reduce the energy spread of the incident electron beam to less than 0.15 eV.

Page 49: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

TEM : transmission electron microscope

SEM : scanning electron microscope

STEM: scanning

Other Electron Microscopes

STEM: scanning transmission electron

microscope

Page 50: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

SEM

The signal arises from secondary electrons ejected by the sample and captured by the field of the detector

It is equivalent to the first part of the TEM but It is equivalent to the first part of the TEM but there is are important differences:a) The sample is outside the objective lens. b) The signal recorded corresponds to reflected

or to secondary electrons. c) No necessity for difficult sample preparationd) Max resolution 2 nm

The distance of the sample is called working distance WD

WD

Page 51: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

SEM

Page 52: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Range vs accelerating voltage

+

−+=32

69.54.1221.66.01

)(R

z

R

z

R

z

Rzg

( ) 75.1/052.0 beamER ρ= Range of electrons in a material

Page 53: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Accelerating voltage

Higher voltage -> smaller probeBut larger generation pear

Higher voltage -> more backscattering

Low energy-> surface effects

Low energy (for bulk) -> lower charging

High energy (for thin sample) -> less charging

Page 54: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Effect of apertures

Larger aperture means in the case of SEM worse resolution (larger probe) but higher current

Page 55: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Strength of Condenser Lens

The effect is similar to that of changing the aperture

Page 56: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Effect of the working distance

Page 57: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Depth of fieldD

D

WD

WD

Page 58: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

La divergenza del fascio provoca un allargamento del suo diametro sopra e sotto il punto di fuoco ottimale. In prima approssimazione, a una distanza D/2 dal punto di fuoco il diametro del fascio aumenta di ∆r ≈αD/2.

E’ possibile intervenire sulla profondità di campo aumentando la distanza di lavoro e diminuendo il diametro dell’apertura finale

Page 59: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Profondità di campo

Page 60: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Minore e’ l’apertura della lente obiettivo e maggiore e’ la distanza di lavoro WD, maggiore e’ la profondità di fuoco.

Page 61: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

SECONDARY electrons

A large number of electrons of low energy <30-50eV produced by the

passage of the primary beam electrons.

they are mainly created in a they are mainly created in a narrow area of radius λSE (few nm) = the SE creation mean

free path

The Everhart-Thornley detectors are suited to detect these electron by means of a gate with a positive

bias.

Page 62: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

BACKSCATTERING

NtEE

EE

E

Ze2

0

0

22

0

24

216

++

=πε

η

Backscattering coefficient=fraction of the incident beam making backscattering

Characterised by a quite large energy

Page 63: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Imaging with BS and SE

Page 64: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

Shadow effect

detector

by reciprocity it is almost by reciprocity it is almost equivalent to light : most

of time intuitive interpretation

Page 65: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

channeling BSE

Page 66: (Microsoft PowerPoint - 14 TEM - Sci Mat [modalit\340 compatibilit

BSDE Backscattering electron diffraction