4. Intro to X-ray Spectroscopies

0.0(0)
Studied by 0 people
call kaiCall Kai
learnLearn
examPractice Test
spaced repetitionSpaced Repetition
heart puzzleMatch
flashcardsFlashcards
GameKnowt Play
Card Sorting

1/14

encourage image

There's no tags or description

Looks like no tags are added yet.

Last updated 9:08 AM on 4/22/26
Name
Mastery
Learn
Test
Matching
Spaced
Call with Kai

No analytics yet

Send a link to your students to track their progress

15 Terms

1
New cards

What are the basic X-ray matter interactions?

  • Incident photons, I0

  • Photons transmitted, I

  • Photons scattered, I’

  • Photons emitted, IF

<ul><li><p>Incident photons, I<sub>0</sub></p></li><li><p>Photons transmitted, I</p></li><li><p>Photons scattered, I’ </p></li><li><p>Photons emitted, I<sub>F</sub></p></li></ul><p></p>
2
New cards

What are the two fundamental photon group interactions?

  • elastic and inelastic scattering - photon scattered - the photons that are still there after the incident photons are transmitted

  • Photoelectric absorption - the photons that have disappeared

3
New cards

What are the elastic scattering techniques and uses?

  • There is no exchange of energy

  • can be diffraction of crystals: XRD or GIXRD

  • or scattering: in amorphous and liquids - WAXS and SAXS

  • Generally for the microscopic geometric structure

4
New cards

What are spectroscopy techniques and uses?

  • spectroscopy = photoelectric absorption or Inelastic scattering

  • Exchange of energy will take place

  • Absorption: XAS< EXAFS, XANES

  • Emission: XES HERFD

  • Photoelectron: PES, XPEEM, ARPES

  • Inelastic scattering: IXS, RIXS, X-Raman

  • Gives the electronic structure, the local structure and the dynamics, interatomic and subatomic

5
New cards

What x-ray interaction is measure for photoelectron spectroscopy, x-ray emission spec and x-ray absorption spec respectively?

  • photoelectron spec - electrons emitted from sample

  • x-ray emission spec - the photons emitted

  • x-ray absoprtion spec - photons transmitted through sample

6
New cards

What are the basic principles of x-ray absorption spec’s (XAS) absorption coefficient?

  • key parameter measured is the absorptions coefficient, μ

  • done with hard x-rays/high photon energies of 5-10keV, below 0.2 - 0.1nm wavelength

  • I = I0e-μt

  • μt = ln (I0/I)

<ul><li><p>key parameter measured is the absorptions coefficient, μ</p></li><li><p>done with hard x-rays/high photon energies of 5-10keV, below 0.2 - 0.1nm wavelength </p></li><li><p>I = I<sub>0</sub>e<sup>-μt</sup> </p></li><li><p>μt = ln (I<sub>0</sub>/I)</p></li></ul><p></p>
7
New cards

What is the setup of XAS?

  • synchotron source generates high energy photons/x-ray

  • polychromatic x-rays travel through a monochromator where x-rays of specifc energies are selected

  • monochromatic x-rays travel to incident flux monitor and then hit the sample

  • Transmitted flux monitor then sits after the sample

  • I0 and I are measured as a function of Ex - Ex will be the graph y-axis and I0 will be the x-axis

<ul><li><p>synchotron source generates high energy photons/x-ray </p></li><li><p>polychromatic x-rays travel through a monochromator where x-rays of specifc energies are selected</p></li><li><p>monochromatic x-rays travel to incident flux monitor and then hit the sample</p></li><li><p>Transmitted flux monitor then sits after the sample </p></li><li><p>I<sub>0</sub> and I are measured as a function of E<sub>x</sub> - E<sub>x</sub> will be the graph y-axis and I<sub>0</sub> will be the x-axis </p></li></ul><p></p>
8
New cards

What does the absorbance graph for XAS look like and the equation to determine μt?

  • μ will depend on x-ray energy, E, atomic no, Z, density, ρ and atomic mass, A

  • μ will have sudden jumps - absorption edges - that occur at energies characteristic of the element and its shell numbers

  • heavier elements have more edges

  • At very high Ex, the absorption tends to 0 as the material will become transparent to x-ray

<ul><li><p>μ will depend on x-ray energy, E, atomic no, Z, density, ρ and atomic mass, A</p></li><li><p>μ will have sudden jumps - absorption edges - that occur at energies characteristic of the element and its shell numbers </p></li><li><p>heavier elements have more edges </p></li><li><p>At very high Ex, the absorption tends to 0 as the material will become transparent to x-ray </p></li></ul><p></p>
9
New cards

How is μ generated in XAS?

  • μ comes from the photoelectric absorptions

  • x-rays with energy 1-200 keV are all absorbed by matter through photoelectric effect

  • upon absorption of x-rays with certain energies, core-level electrons - K, L or M shells - from an atom are ejected

  • Ejected electrons = photoelectrons

  • The atom becomes excited and left with a core hole/absence of an electron

<ul><li><p>μ comes from the photoelectric absorptions </p></li><li><p>x-rays with energy 1-200 keV are all absorbed by matter through photoelectric effect </p></li><li><p>upon absorption of x-rays with certain energies, core-level electrons - K, L or M shells - from an atom are ejected </p></li><li><p>Ejected electrons = photoelectrons </p></li><li><p>The atom becomes excited and left with a core hole/absence of an electron </p></li></ul><p></p>
10
New cards

Which shell determines if the excited photoelectron is from K, L or M shells?

  • shell n = 1 are K-edges

  • 2s shells ar L1 edges

  • 2P shells are L2 and L3 edges

11
New cards

What happens to the excited core hole and what happens during the auger effect?

  • The excited core hole will return to ground state through having a higher level core electron fill the hole and emit its excess energy by fluorescent x-ray or auger electron

  • Auger effect is very uncommon and is a non-radiative way of coming to the ground state

  • energy of fluorescence or auger electron is the energy difference between the core levels

<ul><li><p>The excited core hole will return to ground state through having a higher level core electron fill the hole and emit its excess energy by fluorescent x-ray or auger electron </p></li><li><p>Auger effect is very uncommon and is a non-radiative way of coming to the ground state </p></li><li><p>energy of fluorescence or auger electron is the energy difference between the core levels </p></li></ul><p></p>
12
New cards

What data is measured/collected during XAS?

  • measure energy dependence of x-ray absorption coefficient, μ(E) at and above absorpition edge of element

  • It can be measured through transmission or fluorescence:

  • Transmission: gives and EXACT measurement of μ, absorption measured directly by measuring what is transmitted through the sample, limited by sample quality, thickness, conc etc

  • fluorescence: estimate of μ, radiative signals from re-filling of deep core hole is detected, μ(E) ~ If/I0

13
New cards

What is XAFS?

  • X-ray Absorption Fine Strucutre: oscillatory variation of x-ray absorption as a function of photon energy beyond absorption edge, AKA XAS

  • has 2 measuring regimes

  1. XANES: x-ray absorption near-edge spec - for low energy photons

  2. EXAFS: Extended x-ray absorption fine-structure - for high energy photoelectrons, 50 - 100 eV from edge

14
New cards

What do XANES and EXAFS measure or obtain data form?

  • XANES: covalency, local site symmetry, coordination chem, coord number, orbital hybridisation, orbital occupancy

  • EXAFS: local structure (bond distance, no of or type of neighbours), e.g. types of ligands, distance of neighbouring ligands and bond angle info

15
New cards

What is XES vs XAS?

  • XES is x-ray emission spec

  • XES is highly sensitive to local magnetic moments, spin transitions

  • XAS is x-ray absorption spec

  • XAS is sensitive to element (characteristic binding energies), chemical (shape and position of edge), spin (absorp coefficient is different for circular polarised x-rays in magnetic materials)