Transcript p007.pptx

EXPERIMENTAL PROGRESS FOR
HIGH RESOLUTION CAVITY
RINGDOWN SPECTROSCOPY OF JETCOOLED REACTIVE INTERMEDIATES
Gabriel M. P. Just, Patrick Rupper, Dmitry G. Melnik and
Terry A. Miller
Peroxy Radicals: Motivations

Alkyl peroxy radicals play a key role as intermediates in the
oxidation of hydrocarbons (atmospheric as well as combustion
chemistry)
Atmospheric and Combustion interest


The low temperature combustion of hydrocarbons is a
critical process in the overall degradation of our
atmosphere quality leading to the formation of the peroxy
radicals which, by reacting with the NO radical upset the
NO NO2 balance and leads to the formation of O3 in
the troposhere.
The formation of peroxy radicals is believed to be
partially responsible for the negative temperature
coefficient (NTC) behavior of hydrocarbon combustion
observed from 550-700 K.
Peroxy Radicals: Motivations

Alkyl peroxy radicals play a key role as intermediates in the
oxidation of hydrocarbons (atmospheric as well as combustion
chemistry)

Ambient cell cavity ring-down spectroscopy (CRDS)
Several peroxy radicals have been studied in our lab → near IR
electronic transition is sensitive, species-specific diagnostic
 Rotational structure is only partially resolved (congestion due to overlap
of different rotational lines and different conformers)

Peroxy Radicals: Motivations

Alkyl peroxy radicals play a key role as intermediates in the
oxidation of hydrocarbons (atmospheric as well as combustion
chemistry)

Ambient cell cavity ring-down spectroscopy (CRDS)
Several peroxy radicals have been studied in our lab → near IR
electronic transition is sensitive, species-specific diagnostic
 Rotational structure is only partially resolved (congestion due to overlap
of different rotational lines and different conformers)


High resolution, rotationally resolved IR CRDS of alkyl peroxy
radicals under jet-cooled conditions would be of great value

provide molecular parameters to characterize radicals and benchmark
quantum chemistry calculations
 identify directly spectra of different isomers and conformers
Cavity Ringdown Spectroscopy
A = L/cτabsorber - L/cτ0
Intensity
L
R
l
0
absorber
A = σ Nl
Time
Sensitivity of Technique:
If R = 99.999% and L = 135 cm
then τ0 = 550 µs
Leff = 165.0 km ~ 100 Miles ~
Columbus – Cleveland
l = 5 cm
leff = 6.1 km
( L / c)
τ=
1-R
τ = ( L / c)
(1 - R)+ σ Nl
0
abs
Experimental Setup
20 Hz, ns, 350 mJ
20 Hz, ns, 150 mJ
Nd:YAG pulse laser
730 - 930 nm,  ~ 1 MHz
Nd:YAG
cw laser
Ti:Sa ring
cw laser
P. Dupré and T. A. Miller,
Rev. Sci. Instrum. 78 (2007) 033102
PD
Ti:Sa
Amplifier
(2 crystals)
slit-jet:
SRS (stimulated Raman scattering)
1 m single pass, 13 atm H2
Raman
Cell
BBO
BBO,
~ 1.3 ~mm
~2-~
3 mJ
1st Stokes,
1.3(NIR),
mm (NIR),
2 mJ
Ring-down cavity with slit-jet
BBO
< 200
100 MHz
SRS ~
(absorption length ℓ = 5 cm)
(specification
of the
laser)
(limited by power
and
pressure
L = 135 cm
broadening in H2)
ℓ
R ~ 99.995 – 99.999% @ 1.3 mm
InGaAs
Detector
S. Wu, P. Dupré and T. A. Miller,
Phys. Chem. Chem. Phys. 8 (2006) 1682
Nd:YAG pulse laser
50 - 100 mJ
 ~ 8 - 30 MHz
(FT limited)
Vacuum Pump
longer absorption path-length
less divergence of molecular density in the optical cavity
Pulsed Supersonic Slit-jet and Discharge
Expansion
carrier gas (300 – 700 Torr Ne)
+ precursor RI (1%) and O2 (10%)
Viton Poppet
9 mm
Electrode
Electrode
5 mm
10 mm
5 cm
IR Beam
Previous similar slit-jet designs:
D.J. Nesbitt group, Chem. Phys. Lett. 258, 207 (1996)
R.J. Saykally group, Rev. Sci. Instrum. 67, 410 (1996)
• radical densities of 1012 - 1013 molecules/cm3 (10 mm downstream, probed)
• rotational temperature of 15 - 30 K
• plasma voltage ~ 500 V, I  1 A (~ 400 mA typical), 220 µs length
• dc and/or rf discharge, discharge localized between electrode plates,
increased signal compared to longitudinal geometry
-HV
Spectra improvement

It is known that the methyl peroxy radical
(CH3O2) has a tunneling splitting which is
due to the methyl torsion1. This tunneling
splitting was estimated to be about 2-3
GHz for CH3O2 and about 200 MHz for
CD3O2
1G.M.P.Just,
A.B.McCoy, and T.A.Miller JCP 127, 044310 (2007)
CRDS Spectroscopy of CD3O2 at RT
000
600
600
absorption / ppm
500
1211
400
400
300
300
1222
200
200
123
100
100
0
7000
7000
801
7200
7200
7400
7400
8011211
8011222
3
7600
7600
7800
7800
8000
8000
cm-1/ cm-1
wave numbers
C.-Y.Chung, C.-W.Cheng, Y.-P.Lee, H.-S.Liao, E.N.Sharp, P.Rupper, and T.A.Miller, JCP 127, 044311 (2007)
CD3O2 using DFM
8
ppm per pass
6
4
2
SRS
0
DFM
-2
7365
7370
7375
cm-1
7380
8
ppm per pass
6
4
2
SRS
0
DFM
-2
7373.4
7373.6
7373.8
cm-1
7374.0
7374.2
More characterization of the
laser source

For characterization purposes and more
importantly spectroscopic purposes, we
decided to change frequency range in
order to go to the MIR using DFM by using
not a BBO crystal but a LiNbO3 crystal and
the fundamental of a Nd:YAG laser
MIR Linewidth CH3I Absorption
1600
1400
ppm per pass
1200
1000
800
600
400
200
3000
3005
3010
cm-1
3015
3020
cm-1
7287.0
7287.2
7287.4
7287.6
7287.8
7288.0
7288.2
350
1400
212  111
147 MHz
1200
221  110
300
142 MHz
250
200
800
150
600
100
71 MHz
400
82 MHz
75 MHz
67 MHz
62 MHz
50
83 MHz
65 MHz
0
200
3006.8
3007.0
3007.2
cm-1
3007.4
3007.6
3007.8
ppm per pass
ppm per pass
1000
Estimating the source linewidth
2
2
2
 NIR
  Doppler

2
(


)
, NIR
Source
2
 MIR

2
 Doppler
, NIR
2.42 2
  Source
2
NIR
MIR
ΔνDoppler
128 MHz
53 MHz
ΔνSource
69 MHz
49 MHz
Conclusion and Future Work



We can obtain an experimantal linewidth of
about 145 MHz in the NIR and of about 70 MHz
in the MIR (nearly Doppler limited).
The improvement in linewidth (from 250 MHz for
SRS to 145 MHz width DFM in the NIR) allowed
us to resolve the tunneling splitting in CD3O2
which wasn’t the case using SRS.
From these investigation, we can estimate that
our source linewidth is about 69 MHz in the NIR
and 49 MHz in the MIR
Aknowledgment
Dr Miller
 The Miller group:

 Dr
Patrick Rupper (Switzerland)
 Dr Erin Sharp (JILA)
 Ming-Wei Chen
 Dr Dmitry Melnik
 Dr Philip Thomas
 Dr Linsen Pei
 Rabi ChhantyalPun
 Dr Shenghai Wu (U. of Minnesota)

NSF $$$