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Surface Analysis with Many Positrons
Alex Weiss
Physics DepartmentThe University of Texas at Arlington
TX 76019, USA
Acknowledgments: Current Students::
1. Saurabh Mukherjee Ph.D. Program in Physics, 2. Karthik Shastry, M.S. Physics
Undergraduate Students:Aale Naqvi
Former Students:
Ph.D.-1. M. Jibally, .2. D.Mehl, 3. K.H. Lee, 4. G. Yang, 5. H.Q. (Amy) Zhou, 6. E. Jung, 7. J.H. Kim 8.Wu-Chi Chen, 9.S. Xie 10. J. Zhu, 11. M. Nadesalingam, 12 R. Sundaramoorthy
MS: 1. C. Lei 2. K.H. Lee 3. L.-W.Tyan 4. J.H. Kim 5. S. Wheeler 6. R.Venkataraman 7. A. Nangia 8.R. Nayak 9. N. Jiang 10. S. Starnes 11. J. Yan 12. S. Kim 13. R. Sundaramoorthy 14. M. Nadesalingam15. S. Mukherjee
Collaborators (UTA): A. R. Koymen, .J.L.Fry, N. Fazleev, W.Chen, M. Tao, K. Rajeshwar, C. Kim,(Japan): Hasegawa, Nagai, (Germany): G. Brauer, (BNL)S. Hulbert, R. Bartynski
Former Post-Docs/Collaborators: J. Kaiser – UTA, K.O. Jensen - U. of East Anglia, U.K., G. A.Mulhollan – SLAC, Rulon Mayer, Arnum Schwab – BNL, Anat Eshed- MIT
Previous and Current Funding: NSF, DOE, Texas-ARP, DOE, TheWelch Foundation
� Lecture I: Positron Surface Spectroscopies
� Review of important positron surface interactions
� Overview of Positron Surface Spectroscopies
� Introduction to PAES spectroscopy
� Lecture II: Applications
� Examples of Applications of Positron Surface Spectroscopies
� Lecture III: High Flux e+ Beams: New Possibilities
� Surface island traps: possible means of increasing e+ densities
� New kinds of surface measurements
Why study surfaces with positrons?
� Corrosion
� Electrical Contacts
Adhesion
Adhesion
Corrosion Catalysis
Ultra Thin layers
Solid or � Adhesion
� Ultrathin Layers
� Heterogeneous Catalysts
� >95% of all products synthesised by Catalysts
� ~20% of world economy depends on Catalysts
Electrical Contacts
Corrosion CatalysisLiquid
Technique Depth Probed in Atomic Layers Comments
Many Techniques to Probe Many Techniques to Probe Surfaces Surfaces
LEED 3-5 Need theory
SIMS 1-5 Destructive of thin films. Hard to qualify
XPS 3-10
e- Auger 3-10
STM ~1 Difficulty with element identification
e+ Auger ~1 Significant advantages over E-AES
� Capable of detecting both structure and elemental
composition
� Highly surface selective due to trapping in surface state
� Capable of probing active sites and chemical mechanisms� Capable of probing active sites and chemical mechanisms
� Capable of probing internal surfaces of porous materials
� Low Background
� Very low damage –low energy dose to surface
e+
beam
Energy Loss:
-plasmons
-electron-hole pairs
-Phonons
Thermalized
After: Schultz and Lynn, Rev. Mod. Phys. 60, 1988
e+
Ps
Thermalized
Positron surface state Diffusion
Annihilation in
the bulk
γ
γ Surface StatePs self-annihilation
Thermally Desorbed
e+
beam
γ
γ
Diffusion
Annihilation with Surface Electrons
Positron may give up all or most of its kinetic energy to an electron at or near the Fermi level and directly drop into the surface state;
Thus transferring the surface state binding energy to the electron in
the process. The maximum kinetic energy for an electron emitted in
this process is given by:
Recently Demonstrated Direct Surface Trapping Mechanism
Φ
Metal Vacuum E=∆E
EEEpE ssK ∆=−+= −ϕ max
eVEeVEeVEeV PKss 2 ,0for so 3,5 Now, max >>==−ϕ
Vacuum level
Φ+
Surfaces potential
Ess
εPs
Positron emission (εe+)
εe+
J. Phys. C: Solid State Phys. 21 (1988)Branching ratios for electron-volt positrons at a Cu(ll0)
surfaceJ A Baker, M Touat and P G Coleman
Positronium emission (εPs)
Surface State Trapping (εS)
εS
positrons in positrons out
LEPD,
positron work function,
positron reemission
spectroscopy,
positron tunneling
spectroscopy
positron backscattering
positrons in
positronium
out
gamma rays out
positrons in
positrons out
positrons in
positrons in electrons out
PAES,
positron-induced secondary electrons
surface
ACAR
positronium
emission
spectroscopyor Ps in Ps diffraction
Principal Advantages of PAES:
1. Higher surface selectivity than electron spectroscopies.
2. Very low background-elimination of primary beam induced secondary electron background.
3. Selective sensitivity to nano structures and impurities.
Low energy (~10ev) positron in.Implantation, thermalization,
diffusion, encountering the surface
Positron trapped in surface state
10-12 -10-11 sec
10-10 sec
Time scales of physical processes underlying PAES
Annihilation of surface state positron with core electron
Emission of Auger electron –
Higher energy (20-800 eV) electron out.
10-14 sec
10-10 sec
Vacuum Level
Valence Band
φEz
Ey
Auger Electron
Ex
γ
γ
E Auger = E x- E z- E y- φφφφ
Elimination of Secondary Electron Background
3 keV e- in
30eV -1keV Auger e-+
0-3 keV secondary e-
EAES 30 eV e+ in
30eV -1keV Auger e-+
0-30 eVsecondarye-
PAES
Why is PAES more surface selective than other electron surface spectroscopies?
EAES samples several layers below the surface
metal vacuumλ- escape depth;
λ~ 4 – 10 Å
1000 Å
Incident electrons ~ keVExcited Atoms
~50% of signal
Electrons:
EAES samples several layers below the surface
PAES probes only top layer
λλλλ ~ 1 Å
Thermalized positron in surface state
~from 2nd layer and
below
Positrons:
~95% of signal from top layer
Construct positron potential:
V+(r) = VH(r) + Vcorr(r).
0 Z- ))(n_(
effZ4
1
04π
2e- = )(
imageV
rr χ
ε
Detailed Calculations: ~95% of positron in surfacestate on Cu annihilate with top atomic layer
Solve for positron-surface-state wave function:
[ ] )(ψEi )(ψ)(V )(V )(ψ2m iii
22
CorrH rrrrr +++ =++∇− h
Calculate annihilation probability ( α positron-electron overlap)
∑∫
+=i
ilndcorln
2)(,
2)(32
, rr r ψψπλ
PAES vs EAES ~1 ML Pd deposited on Cu
Cu MVV Pd NVV Cu LVV
PAES
EAES
Cu MVV Pd NVV Cu LVV
Cu MVV Pd NVV Cu LVV
•TOF method collects all energies simultaneously rather than sequentially stepping an energy window.
UTA Time of Flight (TOF) PAES Spectrometer
•100 times the collection efficiency of previous PAES systems.
•Permits observation of Auger peaks from chemically important light elements (e.g. C, O, N).
22Na Positron Source E X B Plates
Sample Position Sample Preparation Chamber
Retarding Tube
Sample manipulator
Accelerator MCP
1 m
Ion Pump Ion Pump
Positron Annihilation-Induced Auger Spectroscopy (PAES) System with
Time-of-Flight (T-O-F) Energy Analyzer
Sample
MCPEXBPlates D
Permanent magnet
EXBPlates C EXB
Plates BEXB
Plates A
TungstenBarrier C
ModeratorTOF retarding tube
B = 40Gauss
TungstenBarrier B
TungstenBarrier A Accelerator
B = 100Gauss
γe-
Schematic of T-O-F PAES system
Vbia
s
Vrt
d
VEXB
2
V
m
VEXB
1
γ e+
Timing scheme of the Time-of-Flight (TOF) PAES spectrometer
NaI Detector
BaF2 Detector
Magnet
Sample TOF Retarding tubeEXB Plates
e-
e+
Micro-channel Plate (MCP)
Fast pre-amplifier
Time to Amplitude converter(TAC)
stop start
γ
γ
CFD
The energy distribution of outgoing electrons in the TOF technique can be calculated by the equation:
2
startstop
e
2
ekinetic ttL
m21
vm21
E
−−−−========
Counter Fast pre-amplifier Time delayCFD
Multi-channel Analyzer(MCA)
0.007
0.008
0.009
0.010
0.011
0.012
0.013
0.014
0.015200 400 600 800 1000 1200 1400 1600
274.9ns (#1118)
Channel
Cou
nts/
sec
0.003
0.004
0.005200 400 600 800 1000 1200 1400 1600
132.3ns (#1483)
274.9ns (#1118)
Channel
Cou
nts/
sec
TOF-PAES Flight Time Spectrum
Copper Sample
0.000
0.001
0.002
0.003
0.004
0.005
0.006
0.007
195.6ns (#1325)
Cou
nts/
sec
Flight time (ns)
650 600 550 500 450 400 350 300 250 200 150 100 50
0.000
0.001
0.002
104.2ns(#1555)
115.1ns(#1527)195.8ns
(#1320)
Cou
nts/
sec
Flight time (ns)
650 600 550 500 450 400 350 300 250 200 150 100 50
Clean Cu Surface Cu Surface with adsorbates
Electron Energy Spectrum
0.3
0.4
0.5
(b)
Experimental data 5 point smoothing
Cu M2,3
VV (59.3 eV)
Inte
nsity
(cou
nt/s
ec)
0.10
0.12
0.14
0.16
0.18
Experimental data 5 point smoothing
Cu M2,3
VV (58.3 eV)
Inte
nsity
(cou
nt/s
ec)
100 200 300 400 500 6000.0
0.1
0.2
Cu M1VV (108.7 eV)
Inte
nsity
(cou
nt/s
ec)
Energy (eV)
100 200 300 400 500 600 700 8000.00
0.02
0.04
0.06
0.08
O KLLN KLL
C KLL(268.0 eV)
Cu M1VV
(108.0 eV)
Inte
nsity
(cou
nt/s
ec)
Energy (eV)
Cu with adsorbates:C (C KLL), N (KLL) and O (KLL)
Clean Cu Surface
Energy spectrum of graphite surface
0.009
0.012
0.015
C KLL (258.4 eV)C
ou
nts
/sec
Auger spectrum of graphite initial surface
100 200 300 400 500 600 700 8000.000
0.003
0.006 O KLL (497.5 eV)Co
un
ts/s
ec
Energy (eV)
Table 2: adsorbate Copper Surface
Core level annihilation probability (%)
Cu 3p Cu 3s C 1s N 1s O 1s
Cu (polycrystalline)Adsorbate surface 0.850 0.191 0.352 0.077 0.070
Core level annihilation probability
*is the theoretical value from reference (Jensen and Weiss), all the adsorbate coverage is 0.5relative to the substrate atomic density for theoretical results.
Cu (110) * with CAdsorbate surface 1.62 0.44 0.14
Cu (110) * with NAdsorbate surface 1.41 0.39 0.21
Cu (110) * with OAdsorbate surface 1.75 0.48 0.10
Core level annihilation probability
Theory Experimental
ps
Comparison of Calculated core-annihilation probabilities (Jensen and Weiss) and experimental results of TOF-PAES as functions of the binding energy of the core levels
Positron removed from surface state
by thermal desorption of Ps
ThermalThermal desorption of Psdesorption of Ps
φ-
Eb
Function of z/γ (desorption rate/ss annihilation rate)
A.P. Mills, Sol. St. Comm., 31 (1979) S. Chu, A.P. Mills, C.A. Murray, PRB, 23 ( 1981)
Rate of Ps desorption:
φ-
Eb
In the positron in a potential well picture:
Where Eb is the binding energy of a positron in the surface state
In the Ps in a potential well picture:Ea is the binding energy of Ps in the well
Energy available when e+ from outside sticks to surfaceEb =Ea-φ- + 1/2Ry
fPs
Ps self-annihilationNo core e-
PAES
fss= 1-fPs(neglecting free e+ channel)
Surface state annihilation~1-10% surface atom core e-followed by Auger emission
1-fPs
RepulsiveRepulsiveRepulsiveRepulsive + van + van + van + van derderderder WaalsWaalsWaalsWaals
Where α(ω)α(ω)α(ω)α(ω) is Ps polarizabilityand ε(ω)ε(ω)ε(ω)ε(ω) is the bulk dielectric function.
Repulsive term approximation: vR(z) = V0e−(z−zo)/l
Positrons can pair up with electrons as Ps Positrons can pair up with electrons as Ps at a surface of quartz and Ps can stick
to the surface.
Saniz, B. Barbiellini, P. M. Platzman, and A. J. Freeman, PRL 99, 096101, (2007);
PRL 100, 019902, (2008).
Michael Schirber, Phys Rev. Focus 20, story 7
Ground state : Ground state : Ground state : Ground state : ----0.112 0.112 0.112 0.112 eVeVeVeV
Excited state: Excited state: Excited state: Excited state: ----0.005 0.005 0.005 0.005 eVeVeVeV
~1/z3
Construct positron potential:
V+(r) = VH(r) + Vcorr(r).
0 Z- ))(n_(
effZ4
1
04π
2e- = )(
imageV
rr χ
ε
Theory used to calculate PAES annihilation probabilities:Positron in potential well at the surface
Jensen and Weiss, PRB 41 (1990) Nieminen and Puska, PRL 50 (1983)
~1/z
Solve for positron-surface-state wave function:
[ ] )(ψEi )(ψ)(V )(V )(ψ2m iii
22
CorrH rrrrr +++ =++∇− h
0 Z- ))(n_(
effZ40 r
Calculate annihilation probability ( α positron-electron overlap)
∑∫
+=i
ilndcorln
2)(,
2)(32
, rr r ψψπλ
Core level annihilation probability
Theory Experimental
ps
Comparison of Calculated core-annihilation probabilities (Jensen and Weiss) and experimental results of TOF-PAES as functions of the binding energy of the core levels
� Properties of positron interactions with surfaces
give positrons significant advantages as probes of
surfaces and surface processes.
� PAES allows measurements of the elemental PAES allows measurements of the elemental
content of the top most atomic layer.
� Temperature dependence of PAES intensities
consistent with surface state origin of PAES signal.
� Theory: Positron in a single particle potential
convenient and accurate calculations of PAES
intensities.