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Chemisorption -- basic concepts and models
NEVF 514 Surface Physics
Winter Term 2011 - 2012
Troja, 2nd December 2011
Bedřich Velický
VII.
This class …
• … is an introduction into the microscopic physics of adsorption
• two model treatments of chemisorption of atoms• a sequence of simple models of electronic states
culminating with the Anderson-Grimley-Newns m.• semi-infinite jellium with adsorbates as a model
treated in LDA … an ab initio approach
Adsorption of atoms
3
weak long range forces (v.d.W.) true chemical bond
AdsorptionPhysisorption Chemisorptio
Dynamical
n
full process in time static nuclei, no time
Description Ad a i batic
BULKmechanical
thermodynamicframework
energy bandselectron pool EF
ATOMisolated
discrete levelsfixed el. number
“surface molecule”
U N E V E N P A R T N E R S
STANDARD AB INITIO LOOP
Questions the adiabatic theory may answer
4
Trustworthy answers are given by a fully ab initio theory at the cost of an extensive computational effort;models provide illustrative partial results of a limited relability achieved in a “cheap” manner
TOTAL ENERGY
GEOMETRY
inner loop
1-el. orbitals
sc potential
INPUT
ADS TOT
clean atom
adsorption energy
adsorption site
ad
vibrational pro
QUESTIONS AT TWO LEVEL
sorption geo
S
chemical bond + electron struc
( )+
perties
metr
( )
y
ture
0= − ≥E E E E
electronic properties
Model one-electron Hamiltonians
to study in a non- selfconsistent way the orbital structure of electrons near a
surface with adsorbates(instead of the inner “green” loop)
One-electron potential at a clean surface• atomic around each site• periodic in the bulk• the zero fixed by the barrier with respect to infinity in the vacuum• the potential inside may be smoothed using the pseudopotential
concept
BARRIER
VACUUM
MODELS I. AND II. of Lecture 3.
PSEUDOPOTENTIAL
One-electron potential with an adatom• atomic around each site• periodic in the bulk• the zero fixed by the barrier with respect to infinity in the vacuum• the potential inside may be smoothed using the pseudopotential
concept• the adatom creates a local disturbance just above the surface
ADATOM
VACUUM
MODELS: A. SommerfeldB. tight binding (LCAO)C. AGN
PSEUDOPOTENTIAL
BARRIER
What we are going to do
8
( )2
2
solve the one-electron Schrödinger
( ( )) ( ) (
equation
)
I.
em V Eα α αψ ψ− ∆ + =r r r
Many-electron state sequence of occup. numbers ,
add spinPauli principle Auf
(
b
II.)
fill from the bottomau principle up 0 1
n
n
ασ
ασ
σ ↓↑
≡• =• ≤ ≤•
( ) ( ) ( )
... highest occupied
... lowest
HOMO
unoccupiL dO
eUM( )
C(III.) harge balance
e e eJ
F E
n N N N Z
n Eασ α
ασ
ϑ
↑ ↓
=
∑ = + = = ∑
−defines Fermi energy
( )(IV.)
( ) ( )
Observables local particle density local spin densit ( ) ( )y ) (
n n nm n n
↑ ↓
↑ ↓
= += −
r r rr r r
2ˆ ( ) ( )( ) orbital interpretationnn nσ ασσ ασ ψ= = ∑r rrdouble average
Schrödinger eq. → matrix problem
Schrödinger eq. → matrix eq.basis of fragment eigenstatesGreen’s function technique
elementary use of universal methodMODEL C. AGN
Three of the ways to solve the Schrödinger eq.
9
2
2
one-electron Schrödinger equati
( ( )) ( ) (
)
on
em V Eα α αψ ψ− ∆ + =r r r
orbital representation
ˆ 0( )HH c
S
c
Eλµ
λ λλ
µ
µµ
λ
ψ ϕ
µ µλ λ
= ∑
∑ − =
orbital representationon-shell at Eα
matching of the wave function(boundary conditions)
textbook approachMODEL A. choose simple V(r)
on-shell at Eαbasis of atomic-like orbitals
sparse matrix techniquestoday a recognized approach
MODEL B. fitted matrix elem.
in real space
tight binding
Three of the ways to solve the Schrödinger eq.
2
2
one-electron Schrödinger equati
( ( )) ( ) (
)
on
em V Eα α αψ ψ− ∆ + =r r r
on-shell at Eαmatching of the wave function
(boundary conditions)textbook approach
MODEL A. choose simple V(r)
in real space
On the way to the Sommerfeld type model A.
BARRIER
VACUUM
MODELS I. Lecture 3
CLEAN SURFACE• The smooth pseudopotential bottom is modeled by a completely flat
Sommerfeld plateau• The barrier is modeled by a step-like abrupt rise from the plateau to
the vacuum zero
PSEUDOPOTENTIAL
On the way to the Sommerfeld type model A.
ADATOM
VACUUM
MODEL A.
PSEUDOPOTENTIAL
BARRIER
SURFACE DECORATED BY AN ADATOM• The smooth pseudopotential bottom is modeled by a completely flat
Sommerfeld plateau• The barrier is modeled by a step-like abrupt rise from the plateau to
the vacuum zero• The atomic potential is modeled by an attractive δ - well• Unrealistic model soluble by hand and giving very good insight
MODEL A. 1D Sommerfeld, step barrier, δ-atom 1
x→
V
FE
0E <
Fermi sea d ( )A x dδ− −
region III.region I. region II.
T
T
h
hr
re
ee p
e ma
arameter
tching r
,
e
,
g
s
ions
V A d
MODEL A. 1D Sommerfeld, step barrier, δ-atom 2
x→
V
FE
0E <
Fermi sea
region I. region II.
RESULT• standing wave in region I.• exponential leaking into
region II.• energy dependent phase shift
needed for smooth matching
Solution of the Schrödinger equation by matching A. SEMI-INFINITE SAMPLE2
22
22 2 2
022 2
2
Ibound sta e e 0 e
.
I .te
Is ikx ikx
xm m
m
k E Vk V kV E Eκ
ψ α βκ
ψ γ κ
−
−
= + = + + = ≡− < < = = −
( ) 2 cos( ) 0
2 cos e 0x
A k x xx
A xκ
ψ ∆
∆ −
= + <
= ⋅ >0
0
| | e tan
| | e sin
2 | | cos cos
i
i
k
k
k
k
∆
∆
κ
κα α ∆
β α ∆
γ α ∆ ∆
−
= =
= =
= =
we know that as model I
SUBST
. of
RATE ALO
Lect
NE
ure 3
MODEL A. 1D Sommerfeld, step barrier, δ-atom 3
x→
d
( )A x dδ− −
region III.region II.
reminesc
THE -A
ent of
TOM
deut
ALO
er
NE
ium
δ
( )
2
2
2
2
| |
( )
( ) ( )( ) ( )
ed
dm
m
b x d
A x d E dx
A d Od d
ω
ω
κ
ψ δ ψ ψ
ψ ωψ ω ψ ω
ψ ε+
−
− −
′′− − − =
′ ′− − =+ − −
=
∫
bE2
2 2
22
2 4
select a
0
so th t
b
b
b
m A
Am
A
V E
E
κ =
= −
− < <
⋅
⋅
MODEL A. 1D Sommerfeld, step barrier, δ-atom 4
x→
V0E <
d ( )A x dδ− −
region III.region I. region II.
( )
I. e eII. e eIII. e
ikx ikx
x x
x d
κ κ
κ
ψ α βψ γ δψ ε
−
−
− −
= += +=
S
full model
UBSTRATE + THE -ATOM δ
2
2
2
2
| | e , | | e
1 etan
1 e
| || |
b
b
i i
d
dk
EyV Ek
∆ ∆
κ
κ
κκκκ
α α β α
κ∆
κ
−
−
−
= =
− −= ⋅
− +
= =−
( )( ) ( )
222
2 2 22 211
2e
| | (1 ) 1 e 2e
b
b
d
d dyyy
κ
κ κ
κκ
κκ
εα
−
− −−+
= + − − +
resonance shifted exponential broadening
For the adsorbate, the atomic bound state dissolvesinto a resonance in the bulk bandThe coupling and the reonance width depends on 2e dκ−
MODEL A. 1D Sommerfeld, step barrier, δ-atom 5
x→
V
FE
0E <
Fermi sea d ( )A x dδ− −
region III.region I. region II.
S
full model
UBSTRATE + THE -ATOM δ
GLOBAL AND LOCAL EFFECTS
• locally, the band states are strongly affected• global effect of a single atom is small (change in the phase shift)
2 2
2
2
1
1. quantization2. normalization | | 2 | | ( ) unchanged by the adsorbate3. density of states ( ) m
V E
L L
Lh
k ndx L o L
g E
π ∆
ψ α
−
= ⋅ +∫ = + =
Refresher
2
( )
2
( )
1
1 1
22
general definition
for suitable for smoothing
in particul
Band filling( ) 1 ( )
22 1
( ) 2
( ) 2
without spin
, ar 2
k F
eF F k
E E k
k
eF
m L L
E E E
pE k k n n p
n E mE L L a
E mE L mE L
π
π π
π ∆
ϑ≤
≡ = ∑ = ∑ −
= = ⋅ + = +
≈ ⋅
= ⋅ = ⋅
N N
N N
IDOS DOS
2 1
general definiti
DOS density of states
( ) ( ) ( )
( ) ( ) ( ) ( )
( )
on
basic fo
our
r
mo l
m
de
E
kk
ddE
mEh
dE d g g EdE
E E g E E E
g E
hustota stav
L
ů
η η
ϑ δ δ−∞
≡ =
= = ∑ −
= ⋅ ⋅
∫N
N
2
2
LDO
2
2( )
SSUM RULE I.
SUM RULE II.
LDOS local densit
( )( ) ( ) ( , )
( )( , ) ( )
( )( , ) ( ) ( )
LDOS f or our model( )
y of states
( )
1
, (
F FE E
k kk
k kk
k kk
k Ek
xn x d E d g x
xg x E E E
xdx g x E dx E E g E
xg x E E E
ψ ηδ η η η
ψ δ
ψ δ
ψ δ
−∞ −∞
= ∑ − ≡
= ∑ −
∫ = ∑ ∫ − =
= ∑ −
∫ ∫
2( )
2
( )) ( )
( , ) | | ( )
k Ek x g E
g d E g E
ψ
ε
=
=
Refresher
Schrödinger eq. → matrix problem
Three of the ways to solve the Schrödinger eq.
20
2
2
one-electron Schrödinger equati
( ( )) ( ) (
)
on
em V Eα α αψ ψ− ∆ + =r r r
ˆ 0( )HH c
S
c
Eλµ
λ λλ
µ
µµ
λ
ψ ϕ
µ µλ λ
= ∑
∑ − =
orbital representation
on-shell at Eαbasis of atomic-like orbitals
sparse matrix techniquestoday a recognized approach
MODEL B. fitted matrix elem.
tight binding
Schrödinger eq. → matrix problem
Tight binding method
21
ˆ 0( )HH c
S
c
Eλµ
λ λλ
µ
µµ
λ
ψ ϕ
µ µλ λ
= ∑
∑ − =
orbital representationAε
Aϕ
εt
2ϕt
ε T
1ϕT
0 1 1 2 2 3 3
0 1
write
Schrödinger equation becomes a difference equation for the coefficient
termination of the chain of
( equa
1D -band with nearest neighbor h
) 0 ti
oppi
ns
n
o
g
sA
n
A
c c c c
c
s
E a Ta
T
ψ ϕ ϕ ϕ ϕ
ε
= + + + +
− + =
0 1 2
1 2 3
1 2
( ) 0
( ) 0
( ) 0
(to infinity)n n n
a E a ta
ta E a ta
ta E a ta
ε
ε
ε + +
+ − + =
+ − + =
+ − + =
The states form a band,
In a chain of substrate atoms, there are states
( of the substrate+one d
2 2
issolved adatom state)
+1
t E t
N N
N
ε ε− ≤ ≤ +
Projected density of states (PDOS)
22
3 *
2 2FD
Probability amplitude = d (
Orbital occupancy
In word
Again, distinguish the global and
PDOS SUM RU
the local prop
) ( )
| | ( ) ( ) | |
( ) ( )
ert
,E
i
sL
s
1
e
n n dE f E E E
g EdE g E
α
ϕ α αα α
ϕ
ϕ
ψ ϕ ϕα
δϕ ϕα α
∫ =
= ∑ = ∫ ∑ −
∫ =
r r r
2 20
2 20 0
the orbital is spread over all eigenenergieswith the total weight equal to 1.PDOS for the adatom in
( ) ( ) | | ( ) | ( ) |
(
our model
) | ( ) | ( ) | (
resona t b
) (
n
|
)
A
A
g E E E E E c EA
g E c E E E c E g E
α α αα α
αα
δ δα
δ
= ∑ − = ∑ −
=
•
∑ − = ⋅
2 just liehavior ke i width n the prev| | ious modelT• ∝
Schrödinger eq. → matrix problem
Schrödinger eq. → matrix eq.basis of fragment eigenstatesGreen’s function technique
elementary use of universal methodMODEL C. AGN
Three of the ways to solve the Schrödinger eq.
23
2
2
one-electron Schrödinger equati
( ( )) ( ) (
)
on
em V Eα α αψ ψ− ∆ + =r r r
orbital representation
ˆ 0( )HH c
S
c
Eλµ
λ λλ
µ
µµ
λ
ψ ϕ
µ µλ λ
= ∑
∑ − =
orbital representation
Anderson - Grimley - Newns model 1W i d e l y u s e dC o n c e p t u a l l y c r u c i a l a l s o t o d a y
System = substrate + adsorbate + couplingˆ ˆ ˆ ˆ
While we may visualize these parts in space,
their description is abstractˆ
S AH H H V
H
•
= + +
•
=
0ˆperturbation
Somewhat like "tunneling Hamiltonians"
P.W. Anderson thought about a d-level impurit
Not
| |
y in bulk
| |
ˆunperturbed
1D, it
|
| . .
may
b A bAb b
b E b A E A b V A h
H
c
V
•
∑ ⟩ ⟨ + ⟩ ⟨ + ∑ ⟩ ⟨
•
•
+
cover any 3D situation, if the bands and
the couplings are properly chosen
Anderson - Grimley - Newns model 2
band
resonance AE
bound state AE
2| | secular equation
for the bo
Schrödinger eq.ˆ( ) | 0 | | |
( ) 0( ) 0
Inside the band, the adsorbate
und state energy
provided it does not fall into the band
bAb
b
A Ab b
b b bA
AVE E
E H A b
E E VE E V
E E
ψ ψ α β
α ββ α
−
− ⟩ = ⟩ = ⟩ + ∑ ⟩
− + ∑ =− + ∑ =
= + ∑
2
22
| |0
Self-consistent e
level becomes unstable
xact equation for
the c
Golden rule decay rate (for weak cou
omplex energy of the resonant sta
pling)
t
| )
e
| (
bAb
bA b
AV
E i E
w V E E
E E
π δ
+ −
= ∑ −
= + ∑
this gives the resonant energy its imaginary part
Anderson - Grimley - Newns model 3
2
0| |
Making sense of the equation for
the complex energy of the
resonance
(*)AbA
b
VE i EE E + −= +∑
22| |
agrees with Golden Rule
( 0) ( ) ( )
First it
( 0) |
eratio
| ( )
n o
adsorption function
(self-
(*
energy)
f yield)
( ) (
s
)
bAb bA b
A A A
VE EE i i V E E
E E E
i
E
EE i
i
E
Σ
Σ ∆
δ
Λ
Λ
π
∆
−+ = ∑ − ∑ −
−+
= + −
=
10
1 ( )
Dirac identity
b
b
b
E E i
E E i E Eπδ
− +
− − −
=
the level goes downbroadensthe Ferm
i energy fixedpartial occupancy resu
EXAMPLE Na on
ltsAl is mo
Al
(synopsis of ab initio calculations)
re electronegative t back e
hanffect of o
Nac
•••••• cupancy on the level
Anderson - Grimley - Newns model 4
2
1
PDOS ( ) ( ) | | |1transformation ( ) Im | |0
1ˆGreen's function ( 0) | |0
ˆ ˆˆSchrödinger eq. ( )
A gentle introduction into the kingdom of Green's func
(
tions
)
A
A
g E E E A
g E A AE i E
G E iE i E
z H G z =1
ζ
ζ
ζ
δ ζ
π ζ ζ
ζ ζ
−
= ∑ − ⟨ ⟩
= − ∑⟨ ⟩ ⟨ ⟩+ −
+ = ⟩ ⟨+ −
− =
∑
2
1
1
2 2
| |1ˆprojected GF | ( ) | ; ( )( )
ˆPDOS again ( ) Im | ( 0) |
| |
( )( ( )) ( )
nearly Lorentzian, except for the energy dependence of and
bAb
A
A
A
Vz EA G z A z
z E zg E A G E i A
EE E E E
ΣΣ
ππ ∆Λ ∆
ζ ζ
Λ ∆
−
−
−⟨ ⟩ = = ∑− −
= − ⟨ + ⟩
=
∑ ⟩⟨
− − +
Anderson - Grimley - Newns model 5
2 ½0
0
Grimley semi-elliptic modelof the chemisorption function
(E)= (1 ( ) )
( ) by Kramers-Kronig
coupling strength, half-band width
Ew
E
w
ε∆ ∆
Λ
∆
−−
0 0
bound statesadsorbate induced resonances
Two basic situations
Zeros of eq. ( ) 0
1 we1 2ak coupling 1 strong coupling
A
w w
E E E
∆ ∆
Λ− − =
< >
Anderson - Grimley - Newns model 6
Semi-infinite jellium in DFT-LDA
fully self-coonsistent ab initio study of the simplest model of a solid incorporating
the exchange and correlations
Recapitulation of bulk jellium 1
J 31
neutral crystal ionic charge evenl
( ) ( )
y spread
Definit
n
i
o
J Jn Z n d nΩ
Ωδ+ +
→
= ∑ − → = ∫r R r r
( )Bohr radius dimensionless paramet
0er
3
3
volume per electron
41
single parameter determines all equilibrium properties
WIGNER RADIUS
3
1.612 10
m
s
n n
a rn
n
π
+=
=
= ×
30 3
simple metals 2 ... 6
s
s
r
r
−
=
Recapitulation of bulk jellium 2
32
2
WIGNER FORMULTOT H X AC
8.72.21 0.916 0.88
TOTAL ENERGY/ELECTRON atomic units
Jellium is stabilized by exchangeand further by the correlations
XC
hol )e (
s s sr r r
g r
ε ε ε ε
+
= + +
= − −
22
)
(
n r
n≡
Recapitulation of bulk jellium 3
0 10 20sr →
0
0.06−
0.12−
CRyε Wigner ... historical, approx.
compared with QMC numerical, heavy computation
in practice -- Perdew-Zunger fit by a
Correlation energ
nalytic expressio
y in jelliu
ns
m
range of previous slide
Recapitulation of DFT-LDA 1
34This is the complete set of equations
of the Kohn-Sham theory
2 2
3 30 0
( ) ( )0
0( )
Lagrange multiplier
non-interacting el 's Kohn-Sham0 0
[ ] [ ] ( ) ( ) [
Write Euler-Lagrange eq
] [ ]
uati
[ ] ( ) ( )
0 0
(
on theory
)
s
s s
s se e
n
e e
n n d n n n n d n
δ δδ
υ υ
δ µδ δ µδ µ
υ µ
′ ′= ≠
= + ∫ = + + ∫
− = − =
+ =r
r r r r r r
rT T
E T E T G
E N E N
2 2
eff
0 eff
2 2
3 30 0
( ) ( )
2 2
Here, the solution is known Use the eff. potential as a real one
( )
( )
( ( )) ( ( ))
( ) ( )( ) ( )e e
s s
n n
m mE E
n n
E d n d n
E
α α α α α α
α α
α
α
δδ δ υ µ
υ
υ ψ ψ υ ψ ψ
ψ ψ
υ υ
+ + =
− ∆ + = − ∆ + =
= ∑ = ∑
= ∑ = + ∫ = + ∫
= ∑
r r r
r
r r
r rr r
r r
G
E T E T G +
E
( )3eff
( )
e
d nδ
δ
υ υ
µ
−− ∫ +
=
rE
N
G
Recapitulation of DFT-LDA 2
35
2 23 3 3 3
H C
K
X
S1 12 2| | | |
defines KS XC energy
Exact decompositi
KS XC hole different from the true one, but similar properties
sum
[ ] ( )
on
( ,
rule
( ) ( )
)xce en d hn d n d n d′ ′− −′ ′′ ′ ′= ∫ ∫ + ∫ ∫
≡
′
+
r r r r r rr r r r r r rG
U E
XC
2
3 KS
KS 3 KSXC
eff H
3H xc XC
12
( ) ( )
| |
( , ) 1
( , ) (
Effective pote
XC energy p
ntial
Final expression for the
, )
( ) ( ) (
er particle
total ener
)
y
)
g
(
xc
xc
n n
e
d h
n d h
E d nα
δ δδ δ
ε
υ υ υ υ
υ
′− ′
′ ′∫ = −
′ ′= ∫
= + = + +
= ∑ − − ∫ + +
r r
r r
r r r
r r r r
r r r r
r
G E
E U E
Recapitulation of DFT-LDA 3
( )
2
XC
KS JXC XC
KS JXC XC
XCxc
JH xc
( )
2
defines the LD
For jellium, KS theory is exact
LDA Ansatz
LDA KS equation
( , ) ( )
( ,[ ]) ( ( ))
( )
( ( ) ( ) ( )
A XC energy
(1) As eas
)
y
s
e
n n
m
n n
n n
n
Eα α α
δδ
ε ε
ε ε
ευ
υ υ υ ψ ψ
∂∂
=
=
= →
− ∆ + + + =
r
r
r r
r
r r r
E
to solve as Hartree or Slater equations
(2) Of course, by iteration in a self-consistent cycle
Clean semi-infinite jellium semi-infinite jellium far more realistic than truncated Sommerfeld simplest theory of surface ever -- a single parameter or treated in DFT-LDA means fully ab initio,
no additional fud
ging wi
t
sn r+
h parameters etc. the calculation permitted to find also total energies, in paticular
the surface energy here, we inspect only a few figures of surface charge distribution
and related quantities (N.D.
Lang and W. Kohn, PRB 1(1970), 4555)
Semi-infinite jellium as a substrate 1
semi-infinite jellium (parameter ) is approached by a point charge treated in DFT-LDA means fully ab initio the calculation permitted to find also total energies and the equilibrium
dis
tances
sr Z
of the adsorbed atoms here, we inspect only a few figN.D. Lang and A.R. Williams, PRB 18(1978)
ur,
es ( )616
Semi-infinite jellium as a substrate 2
Semi-infinite jellium as a substrate 3
The end