Photoelectron Spectroscopy (PES) - s uxes.fysik.su.se/PDF/Lecture2.pdf · Photoelectron...

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Photoelectron Spectroscopy (PES) hν PES spectrum ICl in the gas phase PES spectrum solid Au

Transcript of Photoelectron Spectroscopy (PES) - s uxes.fysik.su.se/PDF/Lecture2.pdf · Photoelectron...

Page 1: Photoelectron Spectroscopy (PES) - s uxes.fysik.su.se/PDF/Lecture2.pdf · Photoelectron Spectroscopy (PES) hν PES spectrum ICl in the gas phase PES spectrum solid Au. Experiment

Photoelectron Spectroscopy (PES)

PES spectrum ICl in the gas phase PES spectrum solid Au

Page 2: Photoelectron Spectroscopy (PES) - s uxes.fysik.su.se/PDF/Lecture2.pdf · Photoelectron Spectroscopy (PES) hν PES spectrum ICl in the gas phase PES spectrum solid Au. Experiment

Experiment

Photon energy, polarization, incidence angles

Electron kinetic energy, emission angles, spin polarization

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Spectrometers

kinb EhE −= υ measurement of the electron kinetic energy

electrons are dispersed in electric or magnetic fields

hemispherical analyzer

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Spectrometer System

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Background

Electron scattering by transport through solid

Energy losses gives a secondary background

Escape depth of elastic electrons of the order of 5-20 Å

Surface Sensitivity

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Energy Scales

Binding energies •Solids relative to Fermi level

Directly from spectrum

•Gases relative to Vacuum level

Determined using calibration gases with binding energies obtained from optical measurements

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Binding EnergiesGround state picture

εb

Koopmans teorem

Assuming the remaining electrons inert

RelaxationValence electrons change due to electron removal

corrrelaxbb EE-E ++= ε

Difference in total energy

bbE ε−= orbital eigenvalue

relaxation energy

correlation energy

FinalTOT

GroundTOTb EEE −= total energy of the whole

system including all interacting atoms

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Chemical ShiftsChemical shifts of core levels of the same element due to different chemical surroundings

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Spin Orbit Splitting-156 p)3(3ph3p ≈→+ υ

slJ ±=

For l = 1 and s = +1/2 J = 3/2

s = -1/2 J = 1/2

Spin and angular momentum interaction

1/23/2 3p and 3p spectrumin seen lines Two

22/4)1J2/()1(2Jorbitalstheofpopulation by thegiven linestwotheofratiosIntensitie

1/23/2 ==++

3:4 ratio f and f shell f2:3 ratio d and d shell d1:2 ratio p and p shell p

5/27/2

3/25/2

1/23/2

→→→→→→

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Open shell interactions

g1π

s1

Coupling between open shells

O2 and NO paramagnetic molecules

HOMO

Σ2 Σ4

O1s O2

Open valence 4f shell for trivalent Yb 4f13

Final state 4f12

Multiplet splittings

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Lifetime broadeningThe full width (Γ) of a spectral line is given by the lifetime (τ) of the final state τ/h=ΓValence hole states for free atoms no broadening

Lifetime of core hole states is determined by sum of the rate for all decay channels

Auger and fluorescence (X-ray emission)fluoaug Γ+Γ=Γ

fluaug Γ+Γ=Γ

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Sudden Approximation

( )rr 22Ψ

r

Ionization much faster than motion of electrons

Many different final states He atom

Monopole selection rule

He 1s spectrum

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Satellites

Ne 1s Shake up and off spectra

2p—np and 2s---ns excitations

Ni metal

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Vibrational ExcitationsBorn Oppenheimer approximation

nuclearelectronTOT ΨΨ=Ψ

Electrons and nuclei move independent of each other

We separate nuclearΨ

Frank Condon Principle (sudden approximation)

Adiabatic transition

Excitation takes infinite time, only to lowest vibrational state

Vertical transition

Excitation is sudden, no time, nuclear coordinates are frozen

2*v'v dI ∫ ΨΨ= τ

Diatomic molecule

Different potential energy curves in ground and excited states

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Vibrations Valence LevelsAmount of vibrational excitations depends on difference between ground and ionized state potential curves

N2 in the gas phase

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Rotational Excitations

Vibrations in H2

Rotations

Resolution 3meV

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Vibrations Core Levels

C1sCore levels are non bonding orbitals

No vibrational excitations expected?

Relaxation in the ionized stateDifferent potential energy curves

Adsorbed CO on NiChemical shifted components

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Gas to SolidHg gas to solid

Core levels

Valence levels

From orbitals to bands

Hydrocarbons

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Angular Distributions

Photoelectrons are ejected along the E-vector

Dipole selections rules

εgfεfdεdpεps

→→→→

Outgoing waves

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Band StructureAngle resolved photoemission

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Photoionization cross sections

Cross sections decreases with increasing photon energy

Resonance in Eu around 4d threshold

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Resonant PhotoemissionValence band features resonant enhanced at core level threshold

Constructive and destructive interference of direct photoemission and Auger decay

Fano profile

2

AugPES MM I +=Auger emission isotropic Photoemission along E-vector6 eV d-band

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Core Level Electron SpectroscopySurface Science

Electrons interact strongly with matter

Surface sensitivity

( )θλsind/-expII 0=

e-

d

θ

bindkin E-hE υ=

Variation in surface sensitivity with photon energy

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Surface Science

Surface and Interfaces exist all around us

This is the way we perceive the world

Solid-Vacuum, Solid-Gas, Solid-Liquid, Liquid-Gas and Solid-Solid, Liquid-Liquid Interfaces

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Surface ScienceMany important applications

Heterogenous Catalysis Molecular Environmental Science

Magnetic StorageSemiconductor Industry

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Single Crystal Surfaces

fcc crystalfcc (100) fcc (111) fcc (110)

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Core Level Binding EnergyDifference in total energy

FinalTOT

GroundTOTb EEE −= total energy of the whole

system including all interacting atoms

Relaxation

Change of valence electrons

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RelaxationMetallic screening

+ e-

Electron transferWhen N (electrons) are 2310≅

XPS binding energy is onset for XAS

Image screening or polarization

+

-

-δ-δ

Electrostatic

No mixing of electrons between ionized atom and surroundings

No relationship between XPS and XAS

Chemisorbed C on Ni

Physisorbed O2 on graphite

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Z+1 Approximation

Z

+

Z+1=

The valence electrons can not approximately distinguish an extra charge in the core region or in the nucleus

Core ionized final statesC*O = NO

Ni* = Cu

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N2 and CO on Ni(100)

Two different N atoms

1.5 eV binding energy shift

The same ground state for both atoms

FinalTOT

GroundTOTb EEE −=

NO

ON

NN ∆E=1.5 eV

Difference in Adsorption energies

NO

CO

CO

NO

∆E=1eV

Similar ground state energy

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Vibrational effects C-O stretch

High Pressure XPS

High resolution XPS of adsorbatesCO

A.Nilsson, J. El. Spec. in press

Föhlisch et. al Phys. Rev. Lett. 81 (1998) 1730

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High Pressure XPS

New development of XPS at intermediate pressures

Catalysis, solid/liquid interfaces etc.

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Thin films

hv

Electrons interact strongly

Surface Sensitivity

5-20 Å

Dependent on electron kinetic energy

Mårtensson et. al. Phys. Rev. Lett. 60, 1731 (1988)

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Surface Core Level Shift (SLCS)

eV 0.3E −=∆

Variation across the 5d series

GroundTOT

FinalTOTb EEE −=

∆ES Surface segregation energy for Z+1 impurity in Z metal

We have a lower binding energy for Au at the surface than in bulk for Pt (111)

The more open surfaces have a larger ∆ES

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Adsorbate Induced Shift

N2 is physisorbed on Au

CO is chemisorbed

Pt is segregated to the surface in presence of CO

CO forms stronger bonds to Pt compared to Au

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Semiconductor Core Level Shifts

Si(100)

Surface reconstruction

Oxidation of Si Si/SiO2 interface

Si2p chemical shift due to local charge on Si atom

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Electrostatic effects on Shifts

C1s shifts for different compounds

Correlation between local charge on ionized atom and binding energy shifts

Only special cases with ligands with large difference in electronegativity

Do not work for metallic systems

RELAXATION changes the picture

Difference in total energy is the correct approach

Koopmans teorem

Orbital eigenvalue

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Photoelectron Diffraction

N

N

Forward scattering zero order diffraction

Molecular orientations

For a full structure determination

Energy dependent diffraction together with multiple scattering calculations

Scattering angles at different energies