Take away messages: what is XPS e-spectrometer: how it works - - PowerPoint PPT Presentation

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Take away messages: what is XPS e-spectrometer: how it works - - PowerPoint PPT Presentation

Take away messages: what is XPS e-spectrometer: how it works HAXPES: probing depth cross sections AP-XPS introduction future: AP-HAXPES with membranes PhotoElectron Spectroscopy (PES) Photo-Emitted electrons Photoelectron Spectroscopy


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Take away messages: what is XPS e-spectrometer: how it works HAXPES: probing depth cross sections AP-XPS introduction future: AP-HAXPES with membranes

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Photoelectron Spectroscopy (PES) is a widely used technique to investigate the chemical composition of surfaces. “What is?” Elemental composition “How much is?” Quantitative analysis PES can probe many features of the electronic structure, thus providing information useful for the comprehension e.g. of spin/charge transport, magnetic properties, local structural order, etc…

  • Irradiate a solid with

monoenergetic UV/X-ray radiation

  • Analyze the energies of the

emitted electrons

PhotoElectron Spectroscopy (PES)

Photo-Emitted electrons

photons

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EK = h – EB – fAN

h : photon energy EB : core level binding energy fAN: work function of the electron analyzer PHOTOELECTRIC EFFECT

  • 1. H. Hertz, Ann. Physik 31,983 (1887).
  • 2. A. Einstein, Ann. Physik 17,132 (1905). 1921 Nobel Prize in Physics.
  • 3. K. Siegbahn, Et. Al.,Nova Acta Regiae Soc.Sci., Ser. IV, Vol. 20 (1967). 1981 Nobel Prize in Physics.

e- h 2s 2p 2s 2p Valence states

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Exploiting PES features  Atomic specie sensitivity  Chemical state sensitivity  Spin sensitivity  Photon Energy and Polarization dependence

Advantages provided by synchrotron radiation sources

 Tunability in a very large range  Very high intensity  Good energy resolution  Possibility to have polarized light

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True success: chemical analysis with laboratory sources X ray tube

Reference: hanbook of x ray photoemission spectroscopy

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CHEMICAL STATE SENSITIVITY

Spin-orbit splitting

Core levels Valence states

Core level spectral lines are identified by the shell from which the electron was ejected (1s, 2s, 2p, etc.).

Copper h = 1486.6 eV

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Electron energy analysers

Electrostatic energy analyser

Time of flight

Hemispherical or cilindrical

Broad application field with standard and synchrotron sources Require pulsed sources, special applications: Time resolved experiment Angular resolved photoemission

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The king of analysers: electrostatic hemispherical analyser

3 parts: input lenses hemisphers detectors

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Detectors: electron multipliers

Channeltrons Microchannel plate

Both require vacuum better than 10-6 mbar!!!

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1 10 100 1000 10000 1 10 100 1000

le > 50 Å

HAXPES energy range

le ~ 5-20 Å

PES typical range

l (Å)

Electron KINETIC energy (eV)

HArd X-ray PhotoElectron Spectroscopy A tool for looking beneath the surface

Photon Energy 2 - 15 keV

Low surface sensitivity

Probing depth up to 30 nm

No need of in situ sample preparation le enhanced at high energy: this open the possibility to study buried layers in multilayer systems

e

z

e z I

l 

 ) (

EK = h – EB – fAN

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1 10 100 1000 10000 1 10 100 1000

le > 50 Å

HAXPES energy range

le ~ 5-20 Å

PES typical range

l (Å)

Electron KINETIC energy (eV)

le (6 keV) ≈ 5 nm le (9 keV) ≈ 8 nm le (1 keV) ≈ 1 nm

le enhanced at high energy: this open the possibility to study buried layers in multilayer systems

le can be tuned by varying the photon energy EK = h – EB – fAN

e

z

e z I

l 

 ) (

e-

z d1 d2 Detector

e

d

e

l

1

e

d

e

l

2

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parentheses: the universal curve FAKE!

There are different behaviour below 100eV, not universal

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The VOLPE Project

VOLume PhotoEmission from solids with Synchrotron Radiation

5th Framework RTD European Project - 3 years (2002-2005)

ELETTRA (Trieste), INFM (Rome and Trieste), ESRF (Grenoble), LURE (Paris), EPFL (Lausanne) ,Univ. Neuchatel

OBJECTIVES: 20-40 meV Energy resolution @ 6-10 keV

1) High Resolution/High Flux ESRF ID16 beamline 15-100 meV at 8-10 keV 2) Dedicated Spectrometer, power supplies and detector

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Challenges:

Power supply stability @HV Low noise detector: CROSS SECTION!!! Use the Elettra resource:

https://vuo.elettra.eu/services/elements/WebElements.html

Return to periodic table

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Experimental chamber and sample holder

Laboratoire LURE (France)

Manipulator with helium cryostat

T < 20 K EPFL (Switzerland)

ID16 beamline at ESRF experimental hutch

1011 photons/s/200 mA with DE ≤ 50 meV ESRF, (France)

VOLPE apparatus at the ID16 beamline of the ESRF

  • P. Torelli et al. RSI 76 023909 (2005)
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Bulk sensitivity in PES is typically estimated via measurements of electron effective attenuation length (l), the thickness of the overlayer that reduces to 1/e the intensity IS of a core level emission from the substrate. The “overlayer” experiment:

I0 = intensity from the bare substrate

Estimation of the bulk sensitivity in HAXPES

) 1 ( ) ( ) (

l l x T x S

e I x I e I x I

 

  

Overlayer: Co, Cu, Ge, and Gd2O3 IT = intensity for an infinite overlayer

  • M. Sacchi et al., Phys. Rev. B 71, 155177 (2005)

PROBING DEPTH ≈ 3le

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Bulk vs Surface sensitivity

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Change in the partial cross section

  • G. Panaccione, G. Cautero, M. Cautero, A. Fondacaro, M. Grioni, P. Lacovig, G. Monaco, F. Offi, G. Paolicelli, M. Sacchi,
  • N. Stojic, G. Stefani, R. Tommasini and P. Torelli,

”High-energy photoemission in silver: resolving d and sp contributions in valence band spectra”,

  • J. Phys.: Condens. Matter 17 (2005) 2671-2679.
  • G. Panaccione, F. Offi, M. Sacchi and P. Torelli,

Hard X-ray PhotoEmission Spectroscopy

  • f strongly correlated systems,

Comptes Rendus de Physique 9, 524 (2008)

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Ambient pressure XPS

Motivation:

  • surface structure may differ from what observed in

UHV

  • Dynamic effect can play a significant role
  • Dynimic processes may be studied
  • Material with high vapor pressure can be studied

Problems: 1) Electron analyser require UHV 2) Electron escape depth

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Analyser for NAP-XPS (a smart solution…)

Extremely expensive, brute force………… Several differential pumping stages Input lenses focalize electron in small apertures to help differential pumping

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Example 1: chemical reactivity @ surfaces

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Example 2: solid/liquid interfaces

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Example 3: the new solution: membranes!

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Take away messages: XPS basic principles e-spectrometer: how it works HAXPES: incresed probing depth change in relative (s,p,d) cross sections AP-XPS introduction future: AP-HAXPES with membranes