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Anion slow electron velocity-map imaging (SEVI): applications to
spectroscopy and dynamics
ColumbusJune, 2009
Motivation: spectroscopy and dynamics of transient species
Reactive free radicals play key role in combustion, planetary atmospheres, interstellar chemistry• Map out electronic and vibrational structure, with special
focus on vibronic coupling between close-lying electronic states
• Optical spectroscopy (LIF, infrared, microwave) are well-established probes
Our (complementary) approach: anion photoelectron spectroscopy (PES)and its variants• Slow electron velocity-map imaging (SEVI), a high
resolution version of PES
Specific systems: Open-shell radicals and reactive
species (C3O, C3S, CnH, C2H3O, i-C3H5O, HCO2)• Use SEVI to resolve low-frequency
vibrational modes, fine-structure, low-lying electronic states
• High resolution of SEVI particularly useful for probing vibronic coupling, Duschinsky mixing, internal rotations, …
Anion photoelectron spectroscopy:
N orm al C oord ina te
ele
ctro
n K
inet
ic E
ne
rgy
()
eKE
C ross S ectionM -
M
M
0
Po
ten
tial E
ne
rgy
ele
ctro
n B
indi
ng
En
erg
y (
)eB
Ehn
eBE h eKE
Why negative ions?
Easy to mass-select Hard to make in large
concentrations, but can usually photodetach at h <4 eV
Can access many interesting neutral species by anion photodetachment• Radicals, clusters, transition states…
Selection rules in PESElectronic: all “one-electron” transitions are allowed
BN¯: X 2+ (…2p2p4)
Detachment from 2p MO X 3, b1 states of BNDetachment from 2p MO a 1+, A 3+ states of BN
So can directly measure a-X singlet-triplet splitting (0.031 eV in BN)
Asmis, 1998
Vibrational selection rules:
1( , 1... ) ( ,..., )hi nABC i n ABC e
Mode i totally symmetric(sym stretch in CO2) : any i allowed. “Active” modes: large changes in normal coordinate upon photodetachment
Mode i non-totally symmetric (CO2 bend, antisym stretch) : only even i, but i =0 typically dominates
2
1
'n
i ii
I
Simplest possible expression-product of 1-dim Franck-Condon factorsNo non-adiabatic effects, i.e.
,v e v e for anion, neutral
Odd i transitions in non-totally symmetric modes are signature of vibronic coupling: Jahn-Teller coupling (degenerate neutral state, i.e. CH3O X 2E state)or Herzberg-Teller coupling between nearby electronic states (X 2u
+, A 2g+ states of BNB )
1 1 1 2 2 2,v e c v e c v e
Vibronic coupling in PES
PES of BNB- (Asmis 1999)odd 3 transitions (i.e. 30
1) occur only because of vibronic coupling between X and A states of BNB
Photoelectron angular distributions
2(1 (cos ))4
dP
d
e¯E
limiting cases:=0: s wave=2: p wave=-1: s+d wave
overlapping electronic bands, vibronic coupling
2A1
2B2
X1, A5 are 301 transitions:
intensity borrowing
Xu,1998
BNB-
How to improve resolution?
Photoelectron spectroscopy• Very general, limited to 5-10
meV ZEKE (zero electron kinetic
energy) spectroscopy• High resolution (0.1-0.2 meV)• Experimentally challenging
SEVI• Resolution comparable to
ZEKE without expt’l complications
An ion
Neu tral
eKE
Fixed hn
Tunable hn
ZEKE SEVI
SEVI apparatus
Adaptation of ideas by Chandler, Houston, Parker Electrons with 50-100 meV fill detector Very high resolution for the slow electrons Energy and angular distributions
Grid Discharge Source
Expansion goes in a 2.5mm x 30mm canal and pass through 2 fine stainless steel grids separated by 1mm with the 2nd grid held at ~-500VDC
TEFLON
Aluminum
SEVI of Cl- Cl(2P3/2), Cl*(2P1/2)
0 50 100 150 200 250 3000.0
0.2
0.4
0.6
0.8
1.0
r = 2.3 pixels
E = 19 cm-1
eKE = 906 cm-1
Radius (pixels)
r = 2.1 pixels
E = 2.8 cm-1
eKE = 23.3 cm-1
Quadrant symmetrized SEVI image
Inverse Abel transformed image
2P1/2
2P3/2
Cl
Cl*
PES of C3O¯
Poorly-resolved progression (550 cm-1) Difficult to determine EA
EA=1.34EA=1.34±0.15 eV
Calculated EA 0.93±0.1 eV
1) J.M Oakes and G.B. Ellison, Tetraedron, 42, 6263 (1986)2) J.C. Rienstra-Kiracofe, G.B. Ellison, B.C. Hoffman, and H.F. Schaefer III, J. Chem. Phys. A, 104,
2273 (2000)
1+
2A’
SEVI of C3O¯ and C3S¯
closely spaced doubletsphotoelectron angular distributions are different
Garand, submitted
SEVI of C3O¯
n04
n04
9000 10000 11000 12000 13000 14000 15000 16000 17000
Ele
ctro
n S
igna
l (A
rb. u
nits
)
eBE (cm-1)
B2
D1E1
D2D3
D4
E2E3
E4
x5 A1
A4
A5
A6
A7
A8
A9
A10
A11
B3
B4
B5
B6
B7
B8
B9
B10
B11
A0A3
A2
D5
D6 D7
D8
D9
E5
E6 E7
E8
E9
B1
D0
E0
B0
C3O
C1
C2
An : 4n
0
Bn :4n
o51
0
Dn: 31
04n
0
En: 31
04n
051
0
EA = 1.238 ± 0.003 eV
v5 (CCC bend) = 109 cm-1
v4 (CCO bend) = 581 cm-1
v3 (sym. str.) = 935 cm-1
EA
SEVI of C3S¯
11500 12000 12500 13000 13500 14000 14500 15000 15500 16000
C3S
Ele
ctro
n Sig
nal (
arb.
uni
ts)
eBE (cm-1)
A0
A1
A2
A3
A4 A5
A6
B0
B1
B2
B3
B4
B5
B6
C0
C1
C2
C3
C4
C5D0
E0
D1
D2F1
F2
G
D3
a
An: 4n
0
Bn: 4n
051
0
Dn: 31
04n
0
En: 31
04n
051
0
EA = 1.5957±0.0010 eV
v5 (CCC bend) = 151 cm-1
v4 (CCS bend) = 478 cm-1
v3 (sym. str.) = 721 cm-1
EA
C3O, C3S summary
C3O¯ SEVI spectrum represents dramatic improvement over previous PES
Accurate EA’s for C3O, C3S, several vibrational frequencies determined for first time
Analysis still needs work• large-amplitude bending motion in
anions, R-T effects
SEVI of CnH¯ anions
anions and neutrals seen in interstellar medium
even n: closely spaced 2+, 2 states in neutral
odd n: evidence for linear and cyclic isomers in anion, neutral
Taylor, 1998
C4H-(1+) C4H (2S+ and 2P)
2S+
2P
2S+ - 2 splitting is only 213 cm-1
Progressions in bending modesvibronic coupling
Zhou, 2007
B, C have different PAD’s
CnH, odd n
C3H: cyclic isomers slightly lower energy than linear isomers in C3H¯ and C3H
C5H: numerous low-lying structures calculated for anion, neutral
Structures I, II have been observed by microwave spectroscopy
PES/SEVI of C5H¯
19000 19500 20000 20500 21000 21500 22000 22500 23000 23500
Ele
ctro
n S
ign
al (
arb
. u
nits
)
eBE (cm-1)
C5HA
B C D
E
F
G
29750 30000 30250 30500 30750 31000 31250 31500 31750 32000
Ele
ctro
n S
ign
al (
arb
. u
nits
)
eBE (cm-1)
C5HH
I J
X0: “linear”linearA0, B0: cycliccyclic
(Sheehan, 2008)
PES
SEVI SEVI
C5H simulations
19000 19500 20000 20500 21000 21500 22000 22500 23000 23500
Ele
ctro
n S
ignal (
arb
. units
)
eBE (cm-1)
C5H (X2)A
B C D
E
F
G
51
0 62
0 41
0
31
0
21
0
11
0
v1 = C-H str.
v2-v5 = C-C backbone str.
v6 = CCH bend
29750 30000 30250 30500 30750 31000 31250 31500 31750 32000
Ele
ctro
n S
ignal (
arb
. units
)
eBE (cm-1)
C5H (a4-
)
51
0
B3LYP/AVTZ
Nearly everything can be fit with linear-linear simulation
SEVI of C7H¯ and C9H¯
22500 23000 23500 24000 24500 25000 25500 26000 26500 27000
Ele
ctro
n S
igna
l (ar
b. u
nits
)
eBE (cm-1)
C7H
32500 33000 33500 34000 34500 35000 35500
Ele
cron
Sig
nal (
arb.
uni
ts)
eBE (cm-1)
C7H
25000 25500 26000 26500 27000 27500
Ele
ctro
n S
igna
l (ar
b.un
its)
eBE (cm-1)
C9H
34500 34750 35000 35250 35500 35750 36000
Ele
ctro
n S
igna
l (ar
b. u
nits
)
eBE (cm-1)
C9H
Spin-orbit splittings of 28 cm-1 seen for both species: transitions to linear 2 neutral states
Vinoxy radical: C2H3O
Combustion intermediate
Studied extensively by Terry Miller (BX transition using LIF)
X, B states well-characterized, less known about A state, anion
Anion
Neutral
Vinoxy: SEVI versus PES
L. S. Alconcel, H. J. Deyerl, V. Zengin, and R. E. Continetti, J. Phys. Chem. A 103, 9190 (1999).
XXAX
Main Vibrations
ν9: CCO bend524;498;423
ν4: CO stretchexp:---;1528;1533
ν7: CC stretch---;1137;1533
a'
a"ν10: CH wagexp: 813;---;---
thy: 939;942;n/a
ν11: all CH wag358;---;---
469;734;n/a
ν12: CH2 twist643;---;---
670;429;n/a
anion radical
anion radical ; ;
Franck-Condon Simulations
Franck-Condon Factor
Duschinsky Rotation
• Q’ and Q : normal coordinates• J : Duschinsky Rotation Matrix : mixing of normal modes• K : mass-weighted geometry change between normal
coordinates
2' viv
fv dIntensity
' 'Q Q K J
Vinoxy SimulationsParallel mode approximation: J = 1
Manually match modes
Full Duschinsky rotation
SEVI overview spectrum
Assignments: a' modes
ν4 : CO stretchν7 : CC stretchν9 : CCO bend
10
1079
10
30 4,9
107
209
109
10
2079
0-0
019
0-0
10
10 54
109 1
08
106
105
104
ν4 : CC stretchν5 : CH2 scissorsν6 : OCH bendν8 : CH2 rockν9 : CCO bend
Assignments : a" modes
1111
1110
1112
1111 1
110 114
1111
Combination bands with
*
*
** *
v10: CH wagν11 : all H wagν12 : CC torsion
ν11 : out-of-plane mode
1-Methylvinoxy: SEVI vs PES
L. S. Alconcel, H. J. Deyerl, and R. E. Continetti, J. Am. Chem. Soc. 123, 12675 (2001).
Vibrational Assignments
10141
020
10
20 10,14
109
ν9 : CC stretchν10 : CH2 a' rockν14 : CCC bendν20 : CH2 wag
0-0
10
102014 1
014
2014 1
010149
109
0-0
?
Hindered Rotor Simulation
imm e)(
1D Potential
)()(2
2
3
VBCH
H
Hamiltonian & free rotor basis
...)3cos1(2
)( 3
VV
Vinoxy, methyl-vinoxy:
Precise EA & T0
Vinoxy: new frequencies for A state, Duschinsky rotation needed to simulate X state
Methyl-vinoxy: resolve hindered rotor progressions in X band as well as vibrational structure
Electron Afinity First Term Energy
Vinoxy 1.8250 ± 0.0014 eV 0.996 ± 0.003 eV
1-Methylvinoxy 1.7471±0.0018 eV 1.039±0.003 eV
HCO2 and DCO2
Intermediate in H+CO2 reaction
Anion is closed-shell, C2v species
Neutral has nearly degenerate 2A1, 2B2 states (2A2 state somewhat higher)
vibronic coupling via 5, 6 modes (b2)
artifactual symmetry breaking problem for electronic structure calculations
1
6
32
5 4
Results from SEVI:
Many more peaks resolved, including hot-bands
Band A is an apparent origin Peaks exhibit two distinct PAD’s:
• For HCO2, A, D, F, H are p-like• B, C, E, G are s-like
Implies transitions to two electronic states Sort out with simulations including vibronic
coupling, Duschinsky rotation (with John Stanton)
HCO2 Simulations
Vibronic symmetry:
Red : A1
Blue : B2
EA = 3.4961 ± 0.0010 eV
Ground State: 2A1
T0(2B2) : 318 ± 8 cm-1 113
Peaks D, F have contributions from 601 (2A1)
(in blue), higher peaks strongly mixed
2 3
6
DCO2 Simulations
EA = 3.5164 ± 0.0010 eV
Ground State: 2A1
T0(2B2) : 87 ± 8 cm-1
Vibronic symmetry:
Red : A1
Blue : B2
2 3
6
again see vibronic coupling via 6 mode
Summary
SEVI offers “next generation” of anion photodetachment experments• First technique that systematically improves
resolution of anion PES without sacrificing (much) generality
Where are we headed?• Bare and complexed metal/semiconductor
clusters• Pre-reactive complexes and transition states (in
progress)• Cold ions via trapping/cooling• Development of improved methods to simulate
spectra beyond simple harmonic analysis
SEVI Group:
Jia ZhouEtienne Garand
Tara Yacovitch
$$$ from AFOSR
Matt Nee
AndreasOsterwalder
John Stanton
18000 17800 17600 17400 17200 17000 16800 16600 16400 16200 16000
eBE (cm-1)
X(1Ag)(SEVI)
A(3B3u)(ZEKE)
ZEKE, SEVI of Si4-
ZEKE, SEVI spectra show much more vibrational structure
Why is SEVI better?• ZEKE is experimentally
challenging!• Band X is missing in ZEKE
spectrum- Wigner threshold law12( )lthE E
s-wave only
Arnold, 1993Garand, unpub