sources and optics for xas

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Stanford Synchrotron Radiation Lightsource Sources and Optics for XAS Apurva Mehta

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Sources and Optics for XAS. Apurva Mehta. X-ray absorption Spectroscopy. Basic Experiment :. =XANES ( X-ay Absorption Near Edge Structure ) =NEXAFS ( Near Edge X ray Absorption Fine Structure ). (EXAFS = Extended X ray Absorption Fine Structure ). E b. EXAFS. Xanes. - PowerPoint PPT Presentation

TRANSCRIPT

Page 1: Sources and Optics for XAS

Stanford Synchrotron Radiation Lightsource

Sources and Optics for XAS

Apurva Mehta

Page 2: Sources and Optics for XAS

Apurva Mehta

X-ray absorption Spectroscopy

Basic Experiment :

Core electron binding energy, Eb

Eb

=XANES (X-ay Absorption Near Edge Structure)=NEXAFS (Near Edge X ray Absorption Fine Structure)

(EXAFS = Extended X ray Absorption Fine Structure)

Xanes EXAFS

Page 3: Sources and Optics for XAS

Apurva Mehta

Two ways of collecting data

White Beam Energy Dispersive

Spectrum in Single Shot Optics and Detector were not Available

But bent crystal optics is making some of this possible

XES – Uwe

Page 4: Sources and Optics for XAS

Apurva Mehta

Two ways of collecting data

Monochromatic “Scanning” Measurement

sam

ple

dete

ctor

Page 5: Sources and Optics for XAS

Apurva Mehta

Two ways of collecting data

Monochromatic “Scanning” Measurement

sam

ple

dete

ctor

Page 6: Sources and Optics for XAS

Apurva Mehta

Two ways of collecting data

Monochromatic “Scanning” Measurement

sam

ple

dete

ctor

Page 7: Sources and Optics for XAS

Apurva Mehta

Two ways of collecting data

Monochromatic “Scanning” Measurement

sam

ple

dete

ctor

Page 8: Sources and Optics for XAS

Apurva Mehta

Two ways of collecting data

Monochromatic “Scanning” Measurement

sam

ple

dete

ctorSlow but doable

Page 9: Sources and Optics for XAS

Apurva Mehta OutlineSources

Slits

Monochromator

Mirrors

XAS BL Layout

Wiggler vs. Undulator

Energy Resolution“Glitches” Harmonic rejection

High Flux Density

Page 10: Sources and Optics for XAS

Apurva Mehta

Measurement Requirements

sam

ple

dete

ctor

Energy Resolution

Very RobustNormalizatio

n

Very High Signal to

Noise

Transparent Detector - Io

Det/Io = signal

Homogeneous Beam

Xanes EXAFS

Page 11: Sources and Optics for XAS

Apurva Mehta Sources

2000 4000 6000 8000 10000

2.00E+013

2.40E+013

2.80E+013

3.20E+013

3.60E+013

Inte

nsity

Energy eV

insertion device

Storage ring with straight sections

wiggler - incoherent superposition

bending magnet - a “sweeping searchlight”

undulator - coherent interference

Bend magnets and Wigglers

Undulators

2000 3000 4000 5000 6000 7000 8000 9000 100000.00E+000

1.00E+012

2.00E+012

3.00E+012

4.00E+012

5.00E+012

6.00E+012

Inte

nsity

Energy eV

Good for EXAFS

Bad for EXAFS

Page 12: Sources and Optics for XAS

Apurva Mehta How to Use an Undulator

5000 5200 5400 5600 5800 60000.00E+000

3.00E+012

6.00E+012

5000 5200 5400 5600 5800 6000

Energy eV

Changing the Undulator K – Scanning the Gap

Page 13: Sources and Optics for XAS

Apurva Mehta

Double Crystal Monochromator

-50 0 50 100

0.0

0.2

0.4

0.6

0.8

1.0

angle/energy

Bragg’s Law:2dsin(q) = h/ENot R

ight!

Page 14: Sources and Optics for XAS

Apurva Mehta

Double Crystal Monochromator

Increasing Energy Resolution

-50 0 50 100

0.0

0.2

0.4

0.6

0.8

1.0

angle/energy

-50 0 50 100

0.0

0.2

0.4

0.6

0.8

1.0

angle/energy

Use Higher Order Reflection

Page 15: Sources and Optics for XAS

Apurva Mehta

Double Crystal Monochromator

Increasing Energy Resolution

Use Narrower Io Slits

Page 16: Sources and Optics for XAS

Apurva Mehta

Double Crystal Monochromator

Increasing Energy Resolution

Use Narrower Mono Slits

Page 17: Sources and Optics for XAS

Apurva Mehta

Double Crystal Monochromator

Increasing Energy Resolution

Use Collimated Beam

Page 18: Sources and Optics for XAS

Apurva Mehta

Double Crystal Monochromator

Harmonics

220

2208keV

440

440 16keV

Rejection

Page 19: Sources and Optics for XAS

Apurva Mehta

Why Harmonics are a Problem

sam

ple

dete

ctor

Transparent Detector - Io

Det/Io = signal

Required Measurement =

DetF

IoF

Actual Measurement =

DetF + DetH

IoF + IoH

Page 20: Sources and Optics for XAS

Apurva Mehta

Double Crystal Monochromator

Harmonics

220

2208keV

440

440 16keV

-50 0 50 100

0.0

0.2

0.4

0.6

0.8

1.0

angle (microrad)

220 @ 8 keV440 @ 16keV

detuning

Rejection

Page 21: Sources and Optics for XAS

Apurva Mehta

Double Crystal Monochromator

Collimating mirror for Harmonic Rejection

Page 22: Sources and Optics for XAS

Apurva Mehta Harmonic Rejection Mirror

2000 4000 6000 8000 10000 12000 14000 16000 18000 200000.0

0.2

0.4

0.6

0.8

1.0

Ref

lect

ivity

Energy eV2000 4000 6000 8000 10000 12000 14000 16000 18000 20000

0.0

0.2

0.4

0.6

0.8

1.0

Ref

lect

ivity

Energy eV

Ni kedgeMn kedge

Page 23: Sources and Optics for XAS

Apurva Mehta Focusing Mirror

A Cylindrical Mirror Bent into a Torous

Focuses Vertically and Horizonally

Page 24: Sources and Optics for XAS

Apurva Mehta XAS BL Optics Layout

insertion device

Storage ring with straight sections

Bend Magnet orWiggler

Preferred.

Undulator – should be scanned.

Collimating/ Harmonic Rejection

Mirror

FocusingMirror

Double Crystal Monochromator

Expt. Hutch“Detune

Mono Slits

Io Slits

M1 Slits

Mo Slits1. Energy Resolution2. Harmonic

Rejection3. High Flux Density

Page 25: Sources and Optics for XAS

Apurva Mehta

Page 26: Sources and Optics for XAS

Apurva Mehta Monochromator “Glitches”

220 220

Page 27: Sources and Optics for XAS

Apurva Mehta

Scattering from a Single crystal

2q

wBragg’s Law:

2dsin(q) = h/E

Page 28: Sources and Optics for XAS

Apurva Mehta

Real Space X-ray Diffraction

Momentum Transfer Space

Scattering from a Single crystal

Real Space Lattice Reciprocal Lattice

Page 29: Sources and Optics for XAS

Apurva Mehta

Q1

Q0

QD

Scattering from a Single crystal

29

Ewald’s Sphere

Page 30: Sources and Optics for XAS

Apurva Mehta

Multiple Reflections

30

Ewald’s Sphere

Resonance between the two

reflections

Energy Transfer between the

two

Page 31: Sources and Optics for XAS

Apurva Mehta

Multiple Reflections – Phi Rotation

31

Ewald’s Sphere F rotation eliminates the

secondary reflection eliminates the

resonance/glitch

Primary reflection

Page 32: Sources and Optics for XAS

Apurva Mehta Monochromator “Glitches”Location Depends on

Phi OrientationSeverity depends on

precise crystal orientation, difficult to predict

Can not be eliminated, but sometimes can be made sufficiently narrow by slits adjustment that EXAFS are not affected.

Page 33: Sources and Optics for XAS

Apurva Mehta

Preparation for an XAS Experiment

Absorbing ElementK, L, M edgeBL with the appropriate energy range

Energy ResolutionMonochromator crystal order (e.g., 111, 220)

Crystal Orientation – phi cut – “Glitch” spectrum.Collimation of the beam prior to the MonoNarrow slits

Harmonic Rejection StrategyMo angle adjustment for appropriate cut-offDetune the monochromator

Flux Density on the sampleSelect an insertion device source if availableAdjust the M1 focusOpen Slits

Page 34: Sources and Optics for XAS

Apurva Mehta XAS BL Optics Layout

insertion device

Storage ring with straight sections

Bend Magnet orWiggler

Preferred.

Undulator – should be scanned.

Collimating/ Harmonic Rejection

Mirror

FocusingMirror

Double Crystal Monochromator

Expt. Hutch“Detune

Mono Slits

Io Slits

M1 Slits

Mo Slits

Page 35: Sources and Optics for XAS

Stanford Synchrotron Radiation Lightsource

Thanks

Questions?

Page 36: Sources and Optics for XAS

Apurva Mehta XAS BL Optics Layout

insertion device

Storage ring with straight sections

Bend Magnet orWiggler

Preferred.

Undulator – should be scanned.

Collimating/ Harmonic Rejection

Mirror

FocusingMirror

Double Crystal Monochromator

Expt. Hutch“Detune

Mono Slits

Io Slits

M1 Slits

Mo Slits