Line Broadening - XRD

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    XRD Line Broadening

    With effects on Selected Area Diffraction (SAD) Patterns in a TEM

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    In the example considered was far away (at a larger angular separation) from

    (Bragg) and it was easy to see the destructive interference

    In other words for incidence angle of the phase difference of is accrued just

    by traversing one d.

    If the angle is just away from the Bragg angle (Bragg), then one will have to go

    deep into the crystal (many d) to find a plane (belonging to the same parallel

    set) which will scatter out of phase with this ray (phase difference of) and

    hence cause destructive interference

    If such a plane which scatters out of phase with a off Bragg angle ray is absent

    (due to finiteness of the crystal) then the ray will not be cancelled and diffraction

    would be observed just off Bragg angles too line broadening!

    (i.e. the diffraction peak is not sharp like a -peak in the intensity versus angle plot)

    This is one source of line broadening of line broadening. Other sources include:

    residual strain, instrumental effects, stacking faults etc.

    When considering constructive and destructive interference we considered the

    following points:

    http://localhost/var/www/apps/conversion/tmp/scratch_13/constructive_interference.ppthttp://localhost/var/www/apps/conversion/tmp/scratch_13/constructive_interference.ppt
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    Instrumental

    Crystallite size

    Strain

    Stacking fault

    XRD Line Broadening

    Other defects

    Unresolved 1 , 2 peaks

    Non-monochromaticity of the source (finite width of peak)

    Imperfect focusing

    In the vicinity ofB the ve of Braggs equation not being satisfied

    Residual Strain arising from dislocations, coherent precipitates

    etc. leading to broadening

    In principle every defect contributes to some broadening

    Bi

    BC

    BS

    ...)( SFsci BBBBFWHMB

    BSF

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    ...)( SFsci

    BBBBFWHMB

    The diffraction peak we see is a result of various broadening mechanisms at work

    Full Width at Half-Maximum (FWHM) is typically used as a measure of the peak width

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    Crystallite size

    Size > 10 m Spotty ring

    (no. of grains in the irradiated portion insufficient to produce a ring)

    Size (10, 0.5) Smooth continuous ring pattern

    Size (0.5, 0.1) Rings are broadened

    Size < 0.1 No ring pattern

    (irradiated volume too small to produce a diffraction ring pattern & diffraction occurs only at low angles)

    Spotty ring

    Rings

    Broadened RingsDiffuse

    10 m0.5

    Rings

    0.1 0.5

    In a TEM Selected Area Diffraction (SAD) pattern, with decreasing crystallite size the

    following effects are observed on the pattern obtained

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    Effect of crystallite size on SAD patterns

    Single crystal

    Spotty pattern

    Few crystals in the selected region

    Schematics

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    Effect of crystallite size on SAD patterns

    Ring patternBroadened Rings

    Schematics

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    Subtracting Instrumental Broadening

    Instrumental broadening has to be subtracted to get the broadening effects due to

    the sample

    1

    Mix specimen with known coarse-grained (~ 10m), well annealed (strain free) does not give any broadening due to strain or crystallite size (the only

    broadening is instrumental). A brittle material which can beground into powder form without leading to much stored strain is good.

    If the pattern of the test sample (standard) is recorded separately then the

    experimental conditions should be identical (it is preferable that one or morepeaks of the standard lies close to the specimens peaks)

    2

    Use the same material as the standard as the specimen to be X-rayed but with large

    grain size and well annealed

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    rsci BBBBB

    ...)( SFsci BBBBFWHMB

    For a peak with a Lorentzian profile

    222

    ir BBB For a peak with a Gaussian profile

    222 )( iir BBBBB A geometric mean can also used

    Longer tail

    The peaks are fitted to various profiles

    12

    2 210 2

    1( )

    ( ) ( )L x

    x x

    2

    2

    1 ( )( ) exp

    22

    xf x

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    Scherrers formula

    ( )c

    B

    kB

    L Cos

    Wavelength

    L Average crystallite size ( to surface of specimen)

    k 0.94 [k (0.89, 1.39)]

    ~ 1 (the accuracy of the method is only 10%)

    For Gaussian line profiles and cubic crystals

    0

    2

    4

    6

    8

    10

    12

    14

    0 30 60 90t

    1/Cos(t)

    The Scherrers formula is used for the determination of grain size from broadened peaks.

    The formula is not expected to be valid for very small grain sizes (

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    Strain broadening

    ( )s BB Tan

    Strain in the material

    Smaller angle peaks

    should be used to

    separate Bs and Bc

    0

    2

    4

    6

    8

    10

    12

    14

    0 20 40 60 80 100

    t

    Tan(t)

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    Separating crystallite size broadening and strain broadening

    scr BBB )(

    CosL

    kBc )(TanBs

    )()(

    Tan

    CosL

    kBr

    )()(

    SinL

    kCosBr

    Plot of [BrCos] vs [Sin]

    Crystallite size broadening

    Strain broadening

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    Annealed Al

    Peak No. 2 () hkl Bi = FWHM () Bi = FWHM (rad)

    1 38.52 111 0.103 1.8 103

    2 44.76 200 0.066 1.2 103

    3 65.13 220 0.089 1.6 103

    Cold-worked Al

    2 () Sin() hkl B() B (rad) BrCos (rad)

    1 38.51 0.3298 111 0.187 3.3 103 2.8 103 2.6 103

    2 44.77 0.3808 200 0.206 3.6 103 3.4 103 3.1 103

    3 65.15 0.5384 220 0.271 4.7 103 4.4 103 3.7 103

    222

    ir BBB

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    3107.1

    L

    knmLSizeGrain 90)(

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