Transcript Columbus 2012
Slow Electron Velocity-map Imaging of Negative Ions: Applications to Spectroscopy and Dynamics
Columbus June 2012
Spectroscopy and dynamics of free radicals, transition states, clusters • • • • Reactive free radicals play key role in combustion, planetary atmospheres, interstellar chemistry – Map out electronic and vibrational structure, with special focus on vibronic coupling Spectroscopy of potential energy surfaces for chemical reactions – Pre-reactive van der waals complexes – Transition state spectroscopy Clusters: evolution of properties of matter with size – Semiconductor clusters, metal oxides, water clusters, He droplets How do we do this? Anion photoelectron spectroscopy (PES) and its variants – Anion slow electron velocity-map imaging (SEVI), a high resolution version of PES – Combine with ion trapping and cooling to maximize resolution
Neutral Fixed h n How to improve energy resolution of photoelectron spectroscopy?
ZEKE SEVI Tunable h n • • • Photoelectron spectroscopy – Very general, limited to 5-10 meV ZEKE (zero electron kinetic energy) spectroscopy – High resolution (0.1-0.2 meV) – Experimentally challenging – restricted to s-wave detachment SEVI – Resolution comparable to ZEKE without expt’l complications – Versatile structural probe Anion
SEVI apparatus
• • • • Adaptation of ideas by Chandler, Houston, Parker Energy and angular distributions Electrons with 300-500 meV fill detector Very high resolution for the slow electrons
Slow electron velocity-map imaging
-350V -255V GND -200V -146V GND Mass-selected anion beam Pulsed MCP detector 1024x1024 • • • Flight tube: 50 cm μ-metal shielding (2 layers) Low VMI voltages, long flight tube – Photoelectrons with 4500 cm -1 (0.5 eV) or 2500 cm -1 (0.3 eV) fill the detector Optimized VMI conditions – – Collinear geometry, pulsed detector -metal shielding, large VMI electrodes, DC voltages only – Small interaction region, finely adjustable extraction voltage Best resolution for the slower electrons (E R 2 ) – Tune photon energy closer to a given transition threshold
Quadrant symmetrized SEVI image Inverse Abel transformed image
SEVI of Cl
Cl(
2
P
3/2
), Cl*(
2
P
1/2
)
Cl* Cl 2 P 3/2 1.0
0.8
0.6
0.4
0.2
0.0
0 50 2 P 1/2 r = 2.1 pixels E = 2.8 cm -1 eKE = 23.3 cm -1 r = 2.3 pixels E = 19 cm -1 eKE = 906 cm -1 100 150 200 Radius (pixels) 250 300
(m -1 )
SEVI of NeSˉ
Sˉ NeSˉ: D 0 =79 cm -1 NeS: D 0 =34 cm -1 X2-I1 splitting (A-B)=9 cm -1
SEVI of ArSˉ, KrSˉ
ArSˉ: D 0 =409 cm -1 ArS: D 0 =120 cm -1 A, B, E are X2, I1, II0 origins KrSˉ: D 0 =630 cm -1 KrS: D 0 =163 cm -1 A, B, G are X2, I1, II0 origins
SEVI of S
-
(D
2
)
j= 0 1 2 3 n 0 1 2 S (D 2 ) S D D Progressions in hindered rotor, S-D 2 stretch 17000 17200 17400 eBE (cm -1 ) 17600 17800
SEVI of C
n
Hˉ anions
• • • anions and neutrals seen in interstellar medium 2 even n: closely spaced + , 2 states in neutral odd n: evidence for linear and cyclic isomers in anion, neutral PE spectra Taylor, 1998
C
4
H
-
(
1 +
)
2 2 +
C
4
H (
2 +
and
2
)
Zhou, 2007 B, C have different PAD’s 2 + 2 splitting is only 213 cm -1 Progressions in bending modes vibronic coupling Zhou, 2007
SEVI of C
n
Hˉ, odd n
• • Direct measurement of S-O splitting in X state of C 5 H (25 cm -1 ) and T 0 for a state (1.309 eV) FC simulations show anion has linear X 3 g ˉ ground state Garand, Chem. Sci. 2010
Longer chains
Next generation of SEVI experiments:
• • • • Peak widths in SEVI spectra of polyatomic molecular anions are typically 20-30 cm -1 wide (i.e. spin-orbit splitting in C n H ground state) Why is resolution worse than for atomic species?
Ion temperature limits resolution – Unresolved rotational contours, incomplete vibrational cooling Implement anion trapping and cooling Lai-Sheng Wang
Modified SEVI apparatus
Another view
Buffer gas: H 2 (35 K) or He (5K) Trapping time: 49 ms (20 Hz rep rate) Gas density: 3*10 13 cm -3
Determination of Ion Temperature
SEVI spectrum of C 5 ˉ
C
5 (
X
2 1/ 2,3/ 2 )
C X
5 ( 1
g e
3/2 =1/2 22900 22950 23000 eBE (cm -1 ) 23050 23100 Population of anion spin-orbit states (splitting 26.5 cm -1 ) serves as temperature probe. Distribution corresponds to 30K. Taken with He at 5K.
Impact of ion cooling on SEVI spectrum of S 3 ˉ (bent anion and neutral) trap at 35K EL Valve buffer gas H 2 buffer gas He 18000 19000 eBE [cm -1 ] 20000 Comparison of SEVI spectra recorded with ions that come straight from the Even-Lavie Valve and ions that have been thermalized in the rf trap at 35K. 17000 18000 19000 20000 eBE [cm -1 ] 21000 For S 3 ˉ, the choice of buffer gas plays a crucial role. Both spectra were recorded at trap temperatures of 35K with very similar H 2 and He densities inside the ion trap.
Indenyl Radical
• • Combustion intermediate – acetylene-oxygen-argon flames Intermediate in the formation of PAHs Marinov, N. M.; Castaldi, M. J.; Melius, C. F.; Tsang, W. Combust. Sci. Technol. 2007, 128, 295.
Calculations
• • • B3LYP/ aug-cc-pVTZ Harmonic frequencies C 2v geometry E rel (eV) 2.7
1.7
Radical: 2 B 1 Radical: 2 A 2 hv 0.0
Anion: 1 A 1
• • • • Cooled to 35 K with H 2 buffer gas in ion trap FC simulation, 130 cm -1 FWHM EA = 1.802(1) eV T 0 ≈ 0.86 eV
Overview
220 cm -1 FWHM
Closer look
20 cm -1 FWHM 11 cm -1 FWHM
Compare to simulation
• • • Non-FC allowed transitions Mix of s- and p-wave Vibronic coupling to 2 B 1 state?
Spectroscopy of reactive potential energy surfaces?
• • F CH 4 has a C 3v structure short F —HCH 3 bond – Near transition state of F + CH 4 reaction
F + CH
4
reaction
E assympt
Czako et al, JCP 2009.
Cheng et al. JCP 2011.
K. Liu et al: evidence for reactive resonances in correlated product distributions (PRL, 2004)
Comparison to Recent Published Results
F( 2 P 3/2 )CH 4 F( 2 P 1/2 )CH 4
SEVI overview Cheng et al.
Cheng, M.; Feng, Y.; Du, Y. K.; Zhu, Q. H.; Zheng, W. J.; Czako, G.; Bowman, J. M. J. Chem. Phys. 2011, 134.
FCH 4
SEVI of Fˉ CH
4
Bound van der
E asympt 29400 29500 29600 29700 eBE (cm -1 ) 29800 29900 30000 • • • Structure below E asympt is from bound states Structure at higher eBE is from transition state region Partially-resolved features; combination of internal rotor and C F stretch expected
Cold, near threshold Fˉ CD
4 FCD 4 29400 29500 29600 29700 eBE (cm -1 ) 29800 29900 Distance between vertical lines 115 cm -1 • • • • See structure above E asympt associated with TS region Considerably less signal from vdW region Progression(s) at 115 cm -1 Assignment in progress (new data!)
Summary
• • SEVI offers “next generation” of anion photodetachment experiments – First technique that systematically improves resolution of anion PES without sacrificing (much) generality Where are we headed?
– Cold ions via trapping/cooling – – Bare and complexed metal/semiconductor clusters Pre-reactive complexes and transition states (in progress) – Theory needed to simulate TS spectra, vibronic coupling
Andreas Osterwalder Matt Nee Jia Zhou $$$ AFOSR
Many thanks:
Etienne Garand Tara Yacovitch Jongjin Kim Christian Hock
… and the rest of the group!
Why is SEVI spectrum of H
2
Fˉ so sensitive to photon energy?
• • • Detachment occurs by p-wave (l=1) Wigner threshold law comes into play Features at low eKE are less intense h n 1 h n 2 (
h
n
E th
) 1 2
Bound van der Waals states
F + CH
4
ground state
Intermolecular stretch Hindered methyl rotation or intermolecular bend narrow: resonances?
• • • Tentative assignments : no TS simulations yet Large geometry differences Isotope effects