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AP 5301/8301 Instrumental Methods of Analysis and Laboratory Lecture 4 Microscopy (III): Transmission Electron Microscopy (TEM) Prof YU Kin Man E-mail: [email protected] Tel: 3442-7813 Office: P6422 1

Instrumental Methods of Analysis and Laboratory · AP 5301/8301 Instrumental Methods of Analysis and Laboratory Lecture 4 Microscopy (III): Transmission Electron Microscopy (TEM)

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  • AP 5301/8301Instrumental Methods of Analysis

    and Laboratory

    Lecture 4

    Microscopy (III): Transmission Electron Microscopy (TEM)

    Prof YU Kin Man

    E-mail: [email protected]

    Tel: 3442-7813

    Office: P6422

    1

    mailto:[email protected]

  • Lecture 4: Outline Introduction:

    ─ Development of transmission electron microscope

    ─ Essential parts and functions

    ─ Operation principles

    TEM specimen preparation

    Imaging modes: brief field, dark field and high resolution

    TEM diffraction

    ─ Diffraction basics

    ─ TEM diffraction patterns

    ─ Selected area electron diffraction

    ─ Convergent beam electron diffraction

    Scanning transmission electron microscopy (STEM)

    ─ Z-contrast imaging

    Electron probe microanalysis

    ─ Electron energy loss spectroscopy

    ─ Energy dispersive and wavelength dispersive x-ray spectroscopy

    2

  • OM TEM SEM

    Magneticlenses

    detector

    CRTCathode Ray Tube

    Light sourceSource of electrons

    Condenser

    Specimen

    Objective

    Eyepiece

    Projector Specimen

    Optical and electron microscopes3

  • Transmission electron microscope4

  • TEM: an introduction

    E (keV) Wavelength (pm)

    50 5.36

    80 4.18

    100 3.70

    200 2.51

    300 1.97

    5

    Electrons at 300 keV have a 𝜆~2 𝑝𝑚 and a diffraction limited resolution ~1 pm

    In practice TEM resolution is far from these

    limits

    Imperfections (aberrations) of magnetic lenses

    are the limiting factor

    A short history:

    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

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

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

    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

  • Comparison: SEM and TEM

    TEM SEM

    Electron beam Broad, static beam Beam focused to fine point and

    scan over specimen

    Electron path passes through thin specimen. scans over surface of specimen

    Specimens Specially prepared thin

    specimens supported on TEM

    grids.

    Sample can be any thickness and is

    mounted on an aluminum stub.

    Specimen stage Located halfway down column. At the bottom of the column.

    Image formation Transmitted electrons collectively

    focused by the objective lens and

    magnified to create a real image

    Beam is scanned along the surface

    of the specimen to build up the

    image

    Image display On fluorescent screen. On TV monitor.

    Image nature Image is a two dimensional

    projection of the sample.

    Image is of the surface of the

    sample

    Magnification Up to 5,000,000x ~250,000x

    Resolution ~0.2 nm ~2-5 nm

    6

  • Advantages

    TEMs offer very powerful magnification and resolution.

    TEMs have a wide-range of applications and can be utilized in a variety of

    different scientific, educational and industrial fields

    TEMs provide information on element and compound structure.

    Images are high-quality and detailed.

    Chemical information with analytical attachments

    Disadvantages

    TEMs are large and very expensive (USD 300K to >1M)

    Laborious sample preparation.

    Operation and analysis requires special training.

    Samples are limited to small size (mm) and must be electron transparent.

    TEMs require special housing and maintenance.

    Images are black and white .

    TEM: advantages and disadvantages7

  • Transmission electron microscopy (TEM)8

    Two unique features of transmission electron microscopy (TEM) are its high

    lateral spatial resolution (better than 0.2 nm) and its capability to provide

    both image and diffraction information from a single sample.

    Hence TEM can be used to obtain full morphological, crystallographic,

    atomic structural and microanalytical such as chemical composition (at

    nm scale), bonding (distance and angle), electronic structure,

    coordination number data from the sample.

    Diffraction

    SpectroscopyImaging

  • TEM: operation principle Primary electrons generated by electron

    gun and focused by stages of condenser

    lenses into bundles

    Electrons illuminate the sample:

    ─ at low magnification, a spread beam is used

    to illuminate a large area

    ─ at high magnification, a strongly condensed

    beam is used

    The pattern of electrons leaving the object,

    reaches the objective lens forms the image.

    The image is greatly enlarged by a projector

    lens.

    The traversing electrons (transmission)

    reach the scintillator plate at the base of the

    column of the microscope.

    The scintillator contains phosphor

    compounds that can absorb the energy of

    the striking electrons and convert it to light

    flashes, forming an image

    9

  • Control brightness,

    convergence

    Control contrast

    A disc of metal

    TEM: operation principle10

  • TEM: essential parts and functions11

    Electron Gun

    EDS Detector

    Condenser

    LensSpecimen

    HolderObjective Lens

    Magnifying Lenses

    CM200 (200kV)

    SAD Aperture

    Fluorescenc

    e screen

    Cost: $4,000,000

    Column

    Binocular

    LN2

  • Specimen Holder

    a split polepiece objective lens

    holder

    beam

    Heating and strainingTwin specimen holder

    Double tilt heating

    Rotation, tilting, heating, cooling and straining

  • TEM: specimen preparationTEM is a microscopy technique whereby a beam of electrons is transmitted through an ultrathin specimen, interacting with the specimen as it passes through it. Materials for TEM must be specially prepared to thicknesses which allow electrons to transmit through the sample (~10-200 nm).

    13

    In addition to be thin, samples have to be:

    ─ Electrically conductive

    ─ Stable under vacuum

    ─ Free from hydrocarbon contaminants

    ─ No artefacts

    For nanoparticles or thin foils, e.g. graphene, disperse crystals or powders on

    a carbon film on a Cu grid

    Thin foil

  • TEM: specimen preparation

    For solid samples, there are different methods:

    Mechanical:─ Mechanical polishing down to electron

    transparency

    ─ Cleavage

    ─ Ultramicrotomy-using a (diamond) knife

    blade

    ─ Crushing

    Mechanical+ionic/chemical─ Grinding, dimpling, ion milling

    Using keV Ar ions focused on the sample to

    thin it down

    ─ Focused ion beam (FIB)

    ─ Electro-chemical polishing

    ─ Chemical polishing or etching

    14

    ion milling

    Focused ion beam

    (FIB)

  • TEM: Cross-section specimen preparation15

    Cross sectional TEM:

    characterization of multilayer materials

    layers thickness measurement

    layers and interfaces structure analysis

    Cross-sectional TEM image of a silicate-

    titanate film containing 10 nm gold particles

    http://www.nanoanalysis.co.jp/en/busin

    ess/case_example_49.html

  • TEM operation16

    TEM offers two methods of specimen observation, diffraction mode and image

    mode. The objective lens forms a diffraction pattern in the back focal plane with

    electrons scattered by the sample and combines them to generate an image in the

    image plane.

    Whether the diffraction pattern or the image

    appears on the viewing screen depends on

    the strength of the intermediate lens.

    The diffraction pattern is entirely equivalent

    to an X-ray diffraction pattern.

    The image mode produces an image of the

    illuminated sample area

    In image mode, the post-specimen lenses

    are set to examine the information in the

    transmitted signal at the image plane of the

    objective lens.

    There are three primary image modes that

    are used in conventional TEM work, bright-

    field microscopy, dark-field microscopy,

    and high-resolution electron microscopy.

  • Use of apertures Condenser aperture:

    ─ Limit the beam divergence (reducing the

    diameter of the discs in the convergent

    electron diffraction pattern).

    ─ Limit the number of electrons hitting the

    sample (reducing the intensity)

    Objective aperture:

    ─ Control the contrast in the image.

    ─ Allow certain reflections to contribute to the

    image.

    ─ Bright field imaging (central beam, 000),

    ─ Dark field imaging (one reflection, g),

    ─ High resolution Images (several reflections

    from a zone axis).

    Selected area aperture:

    ─ Select diffraction patterns from small (>

    1µm) areas of the specimen.

    ─ Allows only electrons going through an area

    on the sample that is limited by the SAD

    aperture to contribute to the diffraction

    pattern (SAD pattern).

  • TEM imaging: bright field

    Bright field (BF): a small objective aperture is used to block all diffracted beams and to pass only the transmitted(undiffracted) electron beam.

    ─ Contrast arises in a bright-field image when thickness or compositional variations or structural anomalies are present.

    ─ Regions in which intensity is scattered (defects) appear dark

    ─ High-Z material appear darker than the low-Z material

    ─ In crystalline materials, dark contrast regions in bright-field usually originate from areas that are aligned for Bragg diffraction

    18

    In image mode, the post-specimen lenses are set to examine the information in the

    transmitted signal at the image plane of the objective lens. The scattered electron

    waves finally recombine, forming an image with recognizable details related to the

    sample microstructure (or atomic structure). There are three primary image modes:

    TEM BF image of

    microcrystalline ZrO2.

    some crystals appear with

    dark contrast since they

    are oriented (almost)

    parallel to a zone axis

    (Bragg contrast).

  • TEM imaging: dark field Dark field (DF): a small objective aperture is

    used to select a diffracted beam and block all other beams.

    ─ Undistorted crystal lattice appears dark since little scattered intensity arises from these regions to contribute brightness.

    ─ dislocations (defects) appear as brightlines on a dark background

    19

    In the DF image (right), some

    of the microcrystals appear with

    bright contrast, namely such

    whose diffracted beams partly

    pass the objective aperture

    (a) Bright-field (BF) micrograph of

    multilayer cross-section sample Ni/Co

    multilayera; (b) Dark-field (DF) TEM

    image.

  • TEM imaging: high resolution Phase contrast or high resolution (HREM): use

    the non-diffracted and at least one diffracted

    beams by using a large (or none) objective

    aperture and add them back together, phase and

    intensity to form an image

    ─ When viewed at high-magnification, it is

    possible to see contrast in the image in the

    form of periodic fringes that represent direct

    resolution of the Bragg diffracting planes

    ─ The contrast is referred to as phase contrast

    20

    TDSi

    BN

    Objective

    aperture

    Electron diffraction pattern recorded from both BN film on Si substrate.

    High resolution TEM

    image of a RuO2

    nanorod

    High Resolution Transmission Electron

    Microscope (HRTEM) Image of a Grain

    Boundary Film in Strontium-Titinate

  • TEM diffraction

    Electrons like X-rays are scattered by atoms

    and can be used to analyze crystal structures

    in a similar way.

    As in X-ray diffraction (XRD), the scattering

    event can be described as a reflection of the

    beams at planes of atoms (lattice planes)

    There are however fundamental differences:

    ─ Electrons have a much shorter wavelength

    than the X-rays

    ─ X-rays are scattered by the electrons that make

    up the bulk of the atom. Electrons are charged

    particles and interact with the electrons

    surrounding atoms and also the nucleus.

    ─ The elastic cross section of the electron is ca.

    106 times larger than that of X-rays.

    ─ Electron beams can be focused using

    electromagnetic lenses

    21

  • TEM: electron diffraction22

    𝜆 = 2𝑑ℎ𝑘𝑙 sin 𝜃ℎ𝑘𝑙Bragg’s law:

    x-ray electrons

    𝜆 = 1.54Å (Cu K) 𝜆 = 0.037Å (100kV)

    A wide range of 𝜃ℎ𝑘𝑙 𝜃 = 0.26𝑜 𝑓𝑜𝑟 𝑑 = 4Å

    For electron diffraction, the incident beam has to

    be almost parallel to the planes for diffraction to

    occur, so that 𝜆 = 2𝑑ℎ𝑘𝑙𝜃ℎ𝑘𝑙𝑟

    𝐿=

    𝜆

    d→ 𝑟 = 𝜆𝐿

    1

    𝑑

    L is the camera length (mm)

    r is the distance between T and D spots

    1/d is the reciprocal of interplanar distance (Å−1)

    Specimen foil

    e-

    L 2

    r

    e-beamZone axis

    of crystal

    sample

    𝑑ℎ𝑘𝑙

    𝑟

    𝐿= sin 2𝜃 ≈ 2𝜃

    hkl

    Real lattice

    [001]

    For electrons: 𝜆 𝑛𝑚 =1.5

    𝑉+10−6𝑉2

  • Reciprocal latticeReciprocal lattice is another way to view a crystal lattice and is used to

    understand diffraction patterns. A dimension of 1/d (Å-1) is used in

    reciprocal lattices.

    g – reciprocal lattice vector─

    23

  • TEM: diffraction intensity

    Spot (ring) intensity: 𝐼ℎ𝑘𝑙 ∝ 𝐹ℎ𝑘𝑙2

    24

    𝐹ℎ𝑘𝑙 =

    𝑏𝑎𝑠𝑖𝑠

    𝑓𝑗𝑒𝑥𝑝 2𝜋𝑖(ℎ𝑢𝑗 + 𝑘𝑣𝑗 + 𝑙𝑤𝑗)

    where 𝑓𝑗 is the atomic scattering factor, and is dependent on atomic number

    𝑢𝑗,𝑣𝑗 , 𝑤𝑗 are the fractional distances within the unit cell

    ℎ, 𝑘, 𝑙 is the Miller indices of the plane

    Atomic scattering factor:

    𝑓 𝜃 ∝𝜆

    sin𝜃2

    𝑍

    where Z is the atomic number of the atom

    Structure Factor:

    lattice

    +

    basis Crystal structure

  • We can consider the BCC structure as a simple

    cubic lattice with a two atom basis, with atoms at

    [000] and [½½½]

    𝐹ℎ𝑘𝑙 =

    𝑏𝑎𝑠𝑖𝑠

    𝑓𝑗𝑒𝑥𝑝 2𝜋𝑖(ℎ𝑢𝑗 + 𝑘𝑣𝑗 + 𝑙𝑤𝑗)

    𝐹ℎ𝑘𝑙 = 𝑓𝑒𝑥𝑝 𝑖0 + 𝑓𝑒𝑥𝑝 2𝜋𝑖(1

    2ℎ +

    1

    2𝑘 +

    1

    2𝑙)

    𝐹ℎ𝑘𝑙 = 𝑓 1 + 𝑒𝑥𝑝 𝑖𝜋(ℎ + 𝑘 + 𝑙)

    Hence: 𝐹ℎ𝑘𝑙 = 2𝑓 𝑖𝑓 ℎ + 𝑘 + 𝑙 𝑖𝑠 𝑒𝑣𝑒𝑛0 𝑖𝑓 ℎ + 𝑘 + 𝑙 𝑖𝑠 𝑜𝑑𝑑

    For a monatomic BCC crystal diffraction from (111), (003), (201), (221), etc. are missing and these are the forbidden diffractions

    TEM: structure factor (example)

    (000)

    ( 1 2 1

    2 1

    2)

    25

  • (010)

    (100)

    TEM: diffraction pattern26

    Real lattice

    reciprocal lattice

    2𝜃

    T D

    For a simple cubic structure

    𝑑ℎ𝑘𝑙 =𝑎

    ℎ2 + 𝑘2 + 𝑙2

    T

    r

    r010

    100 110

    𝑟ℎ𝑘𝑙 = 𝐿𝜆/𝑑ℎ𝑘𝑙

    Diffraction pattern: points with space distance proportional to the reciprocal

    of the interplanar spacing (1/d) in the direction of the normal to the plane

  • Polycrystalline materials

    The electron diffraction pattern is a set of rings, with some spots depending on

    the crystallite sizes.

    Nano to Amorphous materials

    As the crystal size get smaller (nm) the

    rings get more diffuse and eventually

    become halo-like when the material

    becomes amorphous

    TEM: diffraction pattern

    Al single crystalPolycrystalline Pt

    silicide (PtSi)

    Silicon with epitaxial nickel

    silicides ( Si - NiSi - NiSi2)

    Polycrystalline nickel mono

    silicide (NiSi) on top of

    single crystalline silicon

    (Si).

    Amorphous GaNAsnanocrystalline GaNAs

    27

  • TEM: selected area electron diffraction (SAED)

    Combined with sample tilting,

    diffraction images of single

    crystallites can be obtained in

    various orientations.

    Single crystals of a few

    hundred nm in size can be

    examined in this way.

    28

    Selected Area Electron Diffraction SAED is probably the most commonly used

    TEM technique.

    A selected area aperture is located underneath the

    sample holder and can be adjusted to block parts of

    the beam so as to examine just selected areas of the

    sample.

  • SAED aperture

    Many grains covered by SAED aperture

    TEM: diffraction pattern

    Each grain is a single crystal

    A single grain Two grainsAnother grain

    (different orientation)More grains Many grains

    29

  • TEM: convergent beam electron diffraction

    Parallel beam (SAED) Convergent beam (CBED)

    disksT D

    Convergence angle

    Spatial

    resolution

    beam size

    [hkl]

    30

    http://www.feic.com/support/tem/silicon.htmhttp://www.feic.com/support/tem/silicon.htm

  • TEM: convergent beam electron diffraction31

    Convergent Beam Electron Diffraction (CBED): converging the electrons in a

    cone onto the specimen, one can in effect perform a diffraction experiment over

    several incident angles simultaneously. This technique can reveal the full three-

    dimensional symmetry of the crystal. Each spot in SAED then becomes a

    disk within which variations in intensity

    can be seen.

    CBED patterns contain a wealth of

    information about symmetry and

    thickness of specimen.

    The information is generated from

    small regions beyond reach of other

    techniques (

  • TEM: convergent beam electron diffraction32

    The convergence semiangle, α, can be

    adjusted by changing the C2 aperture. The

    size of the diffraction disk depends on α.

    Depending on α different patterns are

    produced.

    Electrons are scattered in all directions in the

    convergent conical illumination.

    Each point in the disc can be scattered by the

    same 2θ. Therefore the diffracted electrons

    also form discs, one for each Bragg reflection.

    Weaknesses:

    Limited to crystalline specimens

    Complicated analysis, normally compared to

    computer simulated pattern.

    The focused beam gives a very high current

    density which causes damage to the sample.

    Specimens are typically cooled with LN2

  • CBED: phase identification in BaAl2Si2O8

    200oC 400oC 800oC

    Hexagonal Orthorhombic Hexagonal

    6mm 2mm 6mm

    CBED (top) and SAED (bottom) patterns6 - rotation axis (rotation about axis by 360/6 degrees) m – mirror plane

    mm

    33

  • Scanning Transmission Electron Microscopy (STEM)34

    In a STEM the electron beam is focused into a narrow spot which is scanned

    over the sample in a rastering mode.

    With STEM we can use many more of these signals in a highly spatially

    resolved way than we can with TEM

    Z-contrast image

    EELS

    EDS

    CL

    SEM

  • Scanning Transmission Electron Microscopy (STEM)

    The rastering of the beam across

    the sample makes these

    microscopes suitable for analysis

    techniques such as mapping by

    energy dispersive X-ray (EDX)

    spectroscopy

    electron energy loss

    spectroscopy (EELS)

    annular dark-field imaging

    (ADF).

    By using a high-angle detector

    (high angle annular dark-field

    HAADF), atomic resolution

    images where the contrast is

    directly related to the atomic

    number (z-contrast image) can

    be formed.

    SAED =0.26o or ~6.4 mrads

    I Z2

    35

    X-rays

    EDX detector

    luminescence

  • STEM: Z-contrast imaging36

    Low angle scattering: Coulombic

    interaction with the electron cloud

    Higher angle scattering: Coulombic

    interaction with the nucleus─Rutherford

    scattering with cross section 𝜎𝑅

    𝜎𝑅(𝜃) ∝ 𝑍2

    Rutherford scattering will dominate when the

    scattering angle > screening parameter 𝜃𝑜

    𝜃𝑜 =0.117𝑍1/3

    𝐸𝑜1/2

    , 𝐸𝑜 𝑖𝑛 𝑘𝑒𝑉

    e.g. Cu for 200 keV e-beam, 𝜃𝑜 ≈ 25 𝑚𝑟𝑎𝑑

    Z-sensitive electrons can be collected by

    using a detector/camera length combination

    that gives large collection angles (e.g. β

    >80–100 mrad): high-angle annular dark-

    field (HAADF)

  • STEM: HAADF images37

    STEM HAADF micrographs of 2 layers

    of Bi absorbed along the general GBs of

    a Ni polycrystal quenched from 700oC

    http://www.jeol.co.jp/en/products/

    detail/JEM-2800.html

    HREM-TEM HR Z-contrast STEM http://www.microscopy.ethz.ch/HD-1.htm

    Pt pn TiO2 Pt on C foil

    (a) HRTEM and (b) HAADF-STEM images of Pt

    nanoparticles (diameter 1-2 nm) dispersed on

    ceria. Krumeich and Müller

    SrTiO3

  • Electron probe microanalysis (EPMA)38

    Electrons lose energy through inner-shell

    ionizations are useful for detecting the

    elemental components of a material.

    In Electron Energy Loss Spectroscopy

    (EELS) characteristic spectral signature,

    termed the edge profile, is derived from the

    excitation of discrete inner shell levels to

    empty states above the Fermi level.

    By studying the detailed shape of the

    spectral profiles measured in EELS, the

    electronic structure, chemical bonding, and

    average nearest neighbor distances for each

    atomic species detected can be derived.

    Quantitative elemental concentration

    determinations can be obtained for the

    elements 3 ≤ 𝑍 ≤ 35 using a standard-less data analysis procedure

    Electron energy loss spectroscopy (EELS)

  • EPMA: electron energy loss process39

    Measures the changes in the energy

    distribution of an electron beam

    transmitted through a thin specimen.

    The energy loss process is the primary

    interaction event.

    All other sources of analytical information

    ( i.e. X-rays, Auger electrons, etc.) are

    secondary products of the initial inelastic

    event.

  • EPMA: EELS spectrum40

    Region 1: zero loss peak,

    represents electrons that have

    passed through the specimen

    suffering either negligible or no

    energy losses

    Region 2 (~1-50 eV): low loss

    regime, exhibits a series of broad

    spectral features related to inelastic

    scattering with the valence electron

    structure of the material.

    ─ In metallic systems these peaks arise

    due to a collective excitation of the

    valence electrons, and are termed

    plasmon oscillations or peaks

    Region 3 (extending to 100-1000 eV): a series of “edges” resulting from

    electrons that have lost energy corresponding to the creation of vacancies in

    the deeper core levels of the atom (K, L, M shells).

    ─ Edge energies are characteristic for each element and therefore can identify

    different elements and their quantity (edge height).

  • EPMA: EELS elemental mapping41

    a) HREM image of a carbon

    nanotube.

    b) Carbon map at the same

    region.

    c) EELS spectrum

    d) Intensity profile of carbon map

    perpendicular to the tube axis.

    The intensity profile

    corresponds well to the

    calculated number

    distribution of carbon atom

    (solid line) based on the size

    and the shape of nanotube.

    The intensity dip at center

    part corresponds to 20

    carbon atoms.

    http://eels.kuicr.kyoto-u.ac.jp/eels.en.html

  • EPMA: EELS spectrum42

    The inner shell edge profile in

    EELS varies with the edge type

    (K, L, M, etc.), the electronic

    structure, and the chemical

    bonding. The details of the profile

    is a measure of the empty local

    density of states above the

    Fermi level of the elemental

    species being studied.

    For example, Carbon edge from

    graphite, C60 and diamond show

    very different fine structures.

    Comparing spectra with data

    library or computation can reveals

    the bonding state and local

    electronic structure of the

    particular sample.

    http://eels.kuicr.kyoto-u.ac.jp/eels.en.html

  • EELS: examples43

    Two-dimensional EELS elemental

    mapping of Fe (red) and Pt (green) in a

    PtFe nanowire

    Zhu et al. JACS, 137 (32 (2015)

    a) Ti L2,3-edges elemental map; b) La M4,5-edges

    elemental map; c) Sr L2,3-edges at 1940 eV

    elemental map; d) Mn L2,3-edges elemental map;

    e) colorized map using the color scheme from

    Figures 9a-d.

    SrTiO3/SrLaMnO3 interface

    http://www.gatan.com/atomic-level-eels-mapping-using-high-energy-edges-dualeels-mode

    Ti La

    Sr Mn

    SrLaMnO3SrTiO3

  • EPMA: Energy dispersive x-ray spectroscopy44

    Energy-dispersive X-ray spectroscopy (EDS, EDX, or XEDS), sometimes called

    energy dispersive X-ray analysis (EDXA) or energy dispersive X-ray microanalysis

    (EDXMA), is an analytical technique used for the elemental analysis or chemical

    characterization of a sample. It relies on an interaction of some source of X-ray

    excitation and a sample.

    A high-energy beam of charged particles such as electrons or protons (PIXE),

    or a beam of X-rays (XRF), is focused into the sample.

    The incident beam excites an electron in an inner shell, ejecting it from the

    shell while creating an electron hole.

    An electron from an outer shell fills the

    hole, and the difference in energy

    between the two shells may be released

    in the form of an X-ray.

    The emitted x-rays are characteristic to

    specific elements and can be measured

    by an energy-dispersive spectrometer

    giving information on the identity and

    amount of the atoms in the sample.

  • EDS detectors: Si(Li), Ge(Li)45

    A ED-spectrometer is p-n junction (or Schottky) of a high purity Si or Ge semiconductor crystal (typically compensated with Li).

    A high negative voltage is applied over the crystal (500-1000 V) create a depletion width larger than the x-ray penetration depth (mm).

    When x-rays enter the crystal electron-hole pairs are formed and the number is proportional to the energy of the x-ray.

    The 𝑒 − ℎ pairs are swept across the semiconductor creating a current pulse with an amplitude proportional to the energy.

    The crystal is cooled (using a LN2 dewar or thermal-electric cooled) to reduce thermal excitation (noise).

    Measuring the amplitude and counting produces the ED-spectrum.

    Energy resolution ~100-150 eV

  • EDS: characteristic x-rays46

    Characteristic x-ray line energy= 𝐸𝑓𝑖𝑛𝑎𝑙 − 𝐸𝑖𝑛𝑖𝑡𝑖𝑎𝑙

    Relative intensities of major x-ray lines

    𝐾𝛼1 = 100 𝐿𝛼1 = 100 𝑀𝛼1,2 = 100

    𝐾𝛼2 = 50 𝐿𝛼2 = 50 𝑀𝛽 = 60

    𝐾𝛽1 = 15 − 30 𝐿𝛽1 = 50

    𝐾𝛽2 = 1 − 10 𝐿𝛽2 = 250

    𝐾𝛽3 = 6 − 15 𝐿𝛽3 = 1 − 6

    𝐿𝛽4 = 3 − 5

    𝐿𝛾1 = 1 − 10

  • EDS: in SEM/TEM/STEM47

  • SEM-EDS analysis: example48

    Scanning electron microscopy (SEM) and energy-dispersive X-ray spectroscopy

    (EDS or EDX) microanalysis for calcium oxalate (CaOx) crystals.

    Chen et al. Kidney intnl. 80, 369 (2011)

  • SEM-EDS elemental mapping49

    Fe3O4/graphene prepared at a low concentration of Fe2+ ions

    Lim et al., in Advanced Topics on Crystal Growth, Chapter 12 (2013) ISBN 978-953-51-1010-1

  • EDS vs EELS mapping50

    Fast joint EELS / EDS color map across a 32 nm

    transistor device

    http://www.gatan.com/techniques/edsedx

    EELS / EDS color map of a SrTiO3 crystal

  • Wavelength dispersive x-ray spectroscopyWavelength-dispersive X-ray spectroscopy (WDXRF or WDS) analyzes the wavelength (instead of the energy in EDS) of the emitted x-rays.

    51

    Note that: 𝐸 𝑒𝑉 =ℎ𝑐

    𝜆𝑛𝑚 𝑜𝑟 𝜆 Å =

    12.26/𝐸 𝑘𝑒𝑉

    So we can either measure the energy or

    wavelength of an emitted x-ray

    Wavelength Dispersive Spectrometers

    measure by diffraction from a crystal

    utilizing Braggs’ law:

    n𝜆 = 2𝑑 sin 𝜃 𝑤ℎ𝑒𝑟𝑒 𝑛 = 1,2,3…

    In WDS the emitted X-rays are diffracted by

    a crystal and counted by a detector.

    The intensity of the diffracted X-rays is

    recorded as a function of the diffraction

    angle.

    WDS can achieve superb energy resolution

    of a few eV.

  • WDS52

    Zr L-line portion of an ED spectrum of zirconia

    (ideally, ZrO2) containing Y acquired using 15kV.

    Blue: WDS energy scan of the same spectral region

  • EPMA: WDS vs EDS53

    WDS EDS

    Spectra acceptance One element/run Entire spectrum in one shot

    Collection time > 10 mins Mins

    Sensitive elements Better for lighter elements

    (Be, B, C, N, O)

    Resolution ~few eV ~130 eV

    Probe size ~200 nm ~5 nm

    Max count rate ~50000 cps

  • EPMA: EELS vs EDS54

    EELS EDS

    Energy resolution ~0.1 eV ~130 eV

    Energy range 0-3000 eV 1-50 keV

    Element range Better for light elements Better for heavy

    elements

    Ease of use Medium high

    Spatial resolution Good beam broadening

    Information Elemental, coordination,

    bonding

    Only elemental

    Quantification Easy Easy

    Peak overlap No Can be severe

  • Related techniques: x-ray fluorescence55

    X-ray fluorescence (XRF) is the emission of characteristic X-rays from a material that has been excited by bombarding with high-energy X-rays. Characteristic x-rays can be measured either in energy or wavelength dispersive mode.

    Hot cathode tube (Coolidge tube) is the most

    common x-ray source.

    electrons are produced by thermionic effect from a

    tungsten filament heated by an electric current.

    A high voltage potential is applied between the cathode

    and the anode, the electrons are thus accelerated

    The anode is usually made out of tungsten or

    molybdenum. So the x-ray generated are characteristic

    x-rays of the anode materials

    High intensity sources: rotating anode, synchrotron

  • Comparison: XRF and EPMA56

    SEM-EDS

    (STEM)

    ED-XRF

    probe Electron X-ray

    Sample

    applicability

    Conductive samples Conductive or

    insulating

    Vacuum

    requirement

    Yes (10

    Analysis

    time

    Minutes Minutes