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X-ray absorption Spectroscopy

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X-ray absorption Spectroscopy

Dr. Gavin Mountjoy, University of Kent, UK



Nell'ambito del programma "Visiting Professor",

finanziato dalla Regione Sardegna.

Outline

1) Introduction

2) Theory of X-ray Absorption Spectroscopy

3) Experimental Method

4) EXAFS Theory

Experimental Method

Data Analysis

Examples

5) XANES Theory

Experimental Method

Data Analysis

Examples

6) Conclusions

1) Introduction

X-ray Absorption Spectroscopy (XAS)

• is a structural characterisation technique

• uses X-rays as a "probe" of structure

• spectroscopy = measure the energy of an interaction



Two methods:

• EXAFS FS = Fine Structure

• XANES NE = Near Edge

Structural characterisation techniques

• study the interaction of a "probe" with a sample

• knowledge of interaction → information about structure

• different types of probes → different types of interactions

• different types of probes

– electromagnetic radiation

– particles

– physical contact





→ different energy

– used for spectroscopy

different wavevector

– used for scattering

X-rays

• a type of electromagnetic radiation

– higher energy compared to UV light

• energy E in electron volts (eV) or kilo eV (keV)

– where1 eV = 1.6 10-19 J, and blue light has E = 3 eV





• energy E from 120 eV (soft) to 120 keV (hard) E (keV ) = 12.4keV

• wavelength λ from 100 Å to 0.1 Å ()

λ A

Sources of X-rays

• natural sources of high energy rays

– radioactive isotopes (gamma rays)

– cosmic rays





• artificial processes which produce X-rays

– excitation of core electrons in atoms (energy from 100s eV to 10s keV)

– acceleration of electrons causes emission of electromagnetic radiation





• artificial sources of X-rays

– X-ray tube (cost €1k) by excitation of core electrons

– synchrotron (cost €500M) by acceleration of electrons

Alternative X-ray sources

• rotating anode

– lab-based source based similar to X-ray tubes





• energy dispersive X-ray absorption spectroscopy

– simultaneously measures X-rays of different energies

Encountering X-rays

• X-rays are harmful to human tissue

– require sheilding using heavy elements, e.g. Pb

• in everyday life

– "box" television: uses accelerated electrons to make picture

– airport security: X-rays are penetrating

– medical imaging: X-rays are penetrating

• in laboratory

– electron microscope: uses accelerated electrons to make picture

– X-ray diffraction: X-ray wavelength ~ atom size

– X-ray fluorescence: X-rays are unique to each element

Interaction of X-rays with atoms

• X-rays interact with electrons in atoms

(i) elastic scattering (no energy transfer)

– used in X-ray diffraction

(ii) inelastic scattering (some energy transfer)

– called "Compton scattering"

– similar to Raman spectroscopy

(iii) absorption (all energy transferred)

– similar to infrared spectroscopy

elastic

inelastic









* absorption

Not to be confused with

• Energy-Dispersive X-ray Spectroscopy (EDX or EDS)

• X-ray Fluorescence Spectroscopy (XRF or XRS)



• no word "Absorption"

• completely different techniques! EDX









XRF

2) Theory

• Transmission of X-rays is given by IT=I0exp(-µt)

– Beer-Lambert law for infrared spectroscopy

– t is thickness

– µ is linear absorption coefficient

– µ increases with atomic number Z (more electrons)

• Absorption coefficient is defined µt=ln(I0/IT)

• spectroscopy: measure µt as a function of energy E

– t is constant

– µ decreases with E (X-ray more penetrating)









absorption µt

sample

X-ray

detector detector

X-ray energy E

X-ray absorption edges

• Absorption edges occur for each shell of core electrons

– when E ~ binding energy of core electron





• X-ray absorption edges are labelled after core electrons

K: 1s1/2 L1: 2s1/2 L2: 2p1/2 L3: 2p3/2 (nj notation)



– note that emitted X-rays

have slightly different labels

Kα, Kβ





• energy of absorption edge E0

is unique for each element

– element-specific technique

Absorption edge energies

• difficult for light elements, e.g. Z57 (La)

100

X-ray absorption edge energy (keV)









40 keV

K-edge

10 L3-edge

4 keV









1

10 20 30 40 50 60 70 80

atomic number (Z)

Element-specific technique

• sample contains several elements

• each element has several X-ray absorption edges

• measurement of a single X-ray absorption edge

• other edges form a uniform background



whole sample single edge of element X



total

absorption µt









absorption µt

background

element X from X

element Y background

element Z from Y& Z

X-ray energy E X-ray energy E

The excited atom

• atom which absorbs X-ray is "excited"

• core electron which absorbs X-ray is ejected from core shell

– sometimes involves "many-electron" effects

• core shell is now has a "core hole"

– other electrons are less shielded from nucleus and "relax"

• another atomic electron drops down in to fill core hole

– timescale for this is called core-hole "lifetime"

• this releases energy similar to X-ray energy

– new X-ray released (X-ray fluorescence)

– additional atomic electron ejected (Auger electron)

The photo-electron

• core electron undergoes transition to a higher energy state

– called a photo-electron

– energy of new state = X-ray energy E - binding energy ionisation

photo-electron

• higher energy state must be:

– unoccupied

– around the excited atom

– obey the dipole selection rule, ∆= 1, e.g. s → p

• molecular orbital approach: → LUMO

• band structure approach : → conduction band

binding

X-ray energy E energy





core electron

Regions of the absorption edge



E0=absorption edge energy Ti K-edge



-5.6

1) pre-edge region (E57 (La)

100









X-ray absorption edge energy (keV)

L1-edge

L2-edge









40 keV

L3-edge









K-edge

10 L3-edge

4 keV









L3 is limited to kmax=11Å-1

due to overlap with L2 and L1 1

50 60 70 80

atomic number (Z)

EXAFS: Examples

Fe-Co alloy nanocrystals





Fe K-edge Co K-edge





Fe Co









k3χ(k)

k3χ(k)









BCC (a=2.87Å) FCC (a=3.51Å)

N R(Å) N R(Å)

8 2.49 12 2.48

6 2.87 6 3.51

12 4.06 24 4.26









k(Å-1) k(Å-1)

samples ?

Fe K-edge Co K-edge

FT









FT

Fe Co

BCC (a=2.87Å) FCC (a=3.51Å)

N R(Å) N R(Å)

8 2.49 12 2.48

6 2.87 6 3.51

12 4.06 24 4.26









R(Å) samples = BCC R(Å)

samples ≠ FCC

CoFe2O4 Nanocrystals

c a

CoFe2O4 is a partially inverted spinel

normal spinel: A2+[Tet](B3+2)[Oct]O4

inverse spinel: B3+[Tet](A2+B3+)[Oct]O4

z x

y



degree of inversion x:

(Co1-xFex)[Tet][CoxFe2-x][Oct]O4

b



distance site [Oct] site

[Tet]



M[Tet]-O 4xO -

M[Oct]-O - 6xO

M[Oct]-M[Oct] - 6xM[Oct]

M[Tet]-M[Oct] 12xM[Oct] 6xM[Tet]

M[Tet]-O 12xO -

Co K-edge

15 (A)

20 (B)

(b)





EXAFS results









FT

0

k3χ(k)









10wt% 900 C

k χ(k)









FT

(b)

(a)

3









0

degree of inversion x=0.69

0

(a)



0 metal cation Co2+/Fe3+

4 6

k(Å-1)

8 10 12 1 2

r(Å)

3 4 5 occupancy

k(Å-1) R(Å) [Tet] site 31%/35%

Fe K-edge [Oct] site 69%/65%

20

(D)

20



distances R (Å)

(b)

M[Tet]-O 1.89/1.84

kk χ(k)









0

M[Oct]-O 2.06/1.98

FT

χ(k)









(b)

3

3









(a) 0

M[Oct]-M[Oct] 2.96

0

(a) M[Tet]-M[Oct] 3.48

0

M[Tet]-O 3.50

1 2 3 4 5

4 6 k(Å-1) 8 10 12

r(Å)

k(Å-1) R(Å)

Nanocrystalline TiO2 materials for Li ion battery applications

studied by Ti K-edge EXAFS in situ



U. Lafont, E. Kelder, D. Carta, G. Mountjoy, et al

Nanocrystalline TiO2

– nanocrystalline TiO2 used in Li ion battery materials

– during charging cycle TiO2 (Ti4+) → Li:TiO2 (Ti3+)

– Ti K-edge EXAFS was measured in situ

structural

changes

charging cycle

– EXAFS results show progression

– three different structures depending on Li content









Anatase TiO2 I41/amd Li0.5TiO2 Imma LiTiO2 I41/amd

15 % Li 40 % Li 100% Li



R(Å) N 2σ 2 R(Å) N 2σ2 R(Å) N 2σ2



O 1.93 6.0 0.010 O 1.93 3.0 0.010 O 2.01 6.0 0.017



Ti 3.03 4.0 0.015 O 2.01 3.0 0.026 Ti 3.13 4.0 0.032



O 3.82 8.0 0.010 Ti 3.12 4.0 0.025 O 3.80 8.0 0.032



Ti 3.82 4.0 0.025 O 3.50 4.0 0.036 Ti 4.14 4.0 0.030



Rfit =39% O 3.78 4.0 0.028 Rfit = 47%



Ti 3.94 4.0 0.017



R fit = 39

5) XANES

X-ray Absorption Near Edge Structure (XANES)

or Near Edge X-ray Absorption Fine Structure (NEXAFS)

XANES: Theory



• photo-electron excited to low energy state

– several eV below or above ionisation level

ionisation

photo-electron









-5.6 Ti K-edge

µt (arbitrary offset)









-6







-6.4

binding

X-ray energy E energy



-6.8

4800 5000 5200 5400

E (eV) core electron

Peaks in XANES spectra

• 10s eV above the absorption edge multiple scatt. peak

– like EXAFS but very strong scattering (start of EXAFS)

• the absorption edge absorption edge peak:

– beginning of conduction band 1s→np continuum states

~ ionisation level 1.5



• a few eV below the absorption edge

– non- or anti-bonding states

1









1 + χ(E)

0.5



pre-edge peak: Zr K-edge

due to 1s→pd mixing at

non-centrosymmetric sites 0

17960 18000 18040

E(eV)

Describing low energy states

• Molecular orbital approach → LUMO

(Lowest Unoccupied Molecular Orbital)

– around the excited atom

– obey the dipole selection rule, ∆= 1, e.g. s → p (for K edge)





• Band structure approach → conduction band

Note: also called "Electronic structure", valence band is full

– site-symmetry projected density of states





• Multiple scattering approach → resonant wavefunction

– photo-electron has very low kinetic energy

– strongly scattered by neighbouring atoms (can't use EXAFS equation)

• Carbon K-edge XANES

– Carbon K-edge is at 284eV





– transition is 1s->np

– XANES depends on

density of unoccupied p states

– see strong peak for π* states



– XANES is difficult to use

for light elements

Effect of oxidation state on XANES

• higher oxidation state → higher energy of XANES

– higher (+) charge on the excited atom → electron states more tightly bound

• XANES is very good for measuring oxidation state

– typically +1 oxidation state → +3 eV energy









Mn K-edge

L-edge XANES

• X-ray absorption edges are labelled after core electrons

K: 1s1/2 L1: 2s1/2 L2: 2p1/2 L3: 2p3/2 (nj notation)

• L1 edge

– involves s→p transitions, so is similar to K-edge XANES

• L2 and L3 edges

– involve p → d transitions

– transition metals show strong peaks due to empty d-states

• for heavy elements use L edge, e.g. Z>57 (La)

– but core-hole lifetime makes resolution worse than ~3 eV

XANES: Experimental method

• near edge region

– scan X-ray energy from -25eV to +50eV above E0

• need good energy calibration

– to measure oxidation state and pre-edge peak

– use a metal foil as a reference

• need good energy resolution

– to measure pre-edge peak Ti K-edge

– typically 1 eV resolution

-5.6

• typical measurement time 15 mins





µt (arbitrary offset)

– faster (10 sec) for a good sample and beamline -6







-6.4







-6.8

4800 5000 5200 5400

E (eV)

XANES: Data analysis

µtsample − µt post −edge

• only fit background to pre-edge χ (E ) =

and post-edge regions µt post −edge − µt pre−edge





• spectra is function of E and has no kn weighting

– spectra can be shown as function of E or E-E0

– where E0 = absorption edge energy of the metal

1.5

post-edge fit

2

pre-edge fit



normalised absorption

absorption µt









1

1







0 0.5

Ti K-edge Ti K-edge

µt(E) 1+χ(E)

-1 0

4700 4900 5100 5300 5500 -20 0 20 40 60 80 100 120

E (eV) E-E0 (eV)

Interpreting XANES spectra

• The pre-edge peak

– a well-defined peak before the absorption edge

– due to known molecular orbitals with p-type symmetry

– can provide semi-quantitative comparison





• The "Fingerprint" approach

– qualitative comparison with XANES spectra of reference samples

– sample and reference are the same → XANES spectra are the same





• Comparison with simulated XANES spectra

– simulations using Band Structure or Multiple Scattering calculations

– quantitative comparison with sample spectra

XANES: Examples

• Ti oxidation state absorption edge position

– nanocrystalline TiO2 used in Li ion battery materials

– during charging cycle TiO2 (Ti4+) → Li:TiO2 (Ti3+)

– Ti K-edge XANES was measured in situ

1.5 14.0

0%

5%

10%

normalised absorbance









13.0

15%



edge position (eV)

1

40%

70%

12.0

100%

100%

0.5

11.0







0 10.0

-5 0 5 10 15 20 25 30 35 40 45 0 20 40 60 80 100

E-E0 (eV)

% charge/discharge

Ti K-edge pre-edge peak

Ti-O coordination

1.5

anatase

[4]Ti ZrTiO4

4

[5]Ti Na2SiTiO5

1/4 Ba2TiO4

1.0



pre-edge peak









absorbance

least

centrosymmetric 0.5









[6]Ti

4/2 6 0.0

-10 0 10 20 30

E(eV)



Note: E is set to zero at 4966eV



most

centrosymmetric

Ti pre-edge peak in TiO2-SiO2 xerogels

[Greegor et al, J. Non-Cryst.

1 Solids 55, 27 (1983)]

[Farges et al, Geoch. et Cosmoch.

[4]Ti

Acta 60, 3023 (1996)]

[5]Ti

relative peak height









TiO2-SiO2 glass

reference

reference

TiO2-SiO2 xerogel

[6]Ti TiO2-SiO2 xerogel





[Chem. Phys. Lett. 304, 150 (1999)]





0

3.5 4.5 5.5

relative peak position (eV)

Zr K-edge XANES

reference compounds (ZrO2)x(SiO2)1-x xerogels

3 3

ZrSiO4

tetrag. ZrO2 750°C

cubic ZrO2

mono. ZrO2 2 2

Zr(OH)4









1+χ(E)

1+χ(E)







RT

zirconolite

BaZrO3

Zr propox. 1 1

x=0.1

[Farges et al, Am. x=0.2

Mineral. 70, 838 (1994)] x=0.3

x=0.4

0 0

-20 0 20 40 -20 0 20 40

E (eV) E(eV)

CoFe2O4 Nanocrystals

• precursor phases studied by XANES

• Fe K-edge • Co K-edge

• 10wt% 450 C is like FeOOH • 10wt% 450 C is like Co(OH)2

• 5wt% 450 C is like Fe[Tet] silicate • 5wt% 450 C is like Co[Oct] silicate



10wt% 450°C ferrihydrite 10wt% 450°C Co Silicate

5wt% 450°C Fe:MCM 5wt% 450°C





2 2.0





1.5 1.5





1 1.0





0.5 0.5





0 0.0

0 10 20 30 40 50 0 10 20 30 40 50

E(eV) E(eV)

• identifying Fe and S compounds using the Fingerprint method

Magnus Sandström,1 Farideh Jalilehvand,2 Emiliana Damian,1 Yvonne Fors,1 Ulrik





Gelius,3 Mark Jones,4 and Murielle Salomé5

6) Conclusions

• X-ray absorption spectroscopy

– can be routinely performed at Synchrotrons

– is an element-specific technique

• EXAFS

– photo-electron is scattered by the neighbouring atoms

– Fourier Transform analysis gives structural parameters R, N and A

• XANES

– photo-electron goes to states near ionisation energy

– analysis gives oxidation state, site-symmetry, and compound identification

• detailed structural information which is difficult to obtain

from other techniques

Acknowledgements

• collaborators:

– A. Corrias, D. Carta, M.F. Casula, D. Loche, G. Navarra, U. Lafont,

E. Kelder, R.J. Newport, D.M. Pickup

• synchrotrons:

– L. Olivi (Elettra), S. Fiddy, F. Mosslemanns, L. Murphy (SRS)

• funding organisations:

– Marie Curie Fellowship (EU), Royal Society Fellowship (UK), EPRSC (UK)



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