pyrene C 16 H 10 using a quantum cascade laserbased cavity ringdown spectrometer Jacob T Stewart and Brian E Brumfield Department of Chemistry University of Illinois at UrbanaChampaign ID: 369077
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Slide1
Rotationally-resolved infrared spectroscopy of the polycyclic aromatic hydrocarbon pyrene (C16H10) using a quantum cascade laser-based cavity ringdown spectrometer
Jacob T. Stewart and Brian E. Brumfield, Department of Chemistry, University of Illinois at Urbana-ChampaignBenjamin J. McCall, Departments of Chemistry and Astronomy, University of Illinois at Urbana-ChampaignSlide2
Our goal at 8.5 µmOur goal is to observe the 8.5 µm vibrational band of C60 to aid in astronomical studiesWe have built a sensitive mid-IR spectrometer and measured the 8 mode of methylene bromideWe have attempted to observe C60, but have not seen any signal yet
B. E. Brumfield, J. T. Stewart, B.J. McCall,
J. Mol. Spec.
,
266
, 57 (2011).Slide3
Seeking an intermediate challenge
Trip to the moon
Pyrene C
16
H
10
Coronene C
24
H
12
Ovalene C
32
H
14
T
oven
increasing with mass to produce necessary
number density
400 K
1000 K
Increasing Q
vib
26 atoms
60 atoms
C
60
Walk in the park
Only
pyrene
has an IR active mode within QCL frequency coverage
Largest molecule to be rotationally resolved using infrared direct absorption spectroscopySlide4
Previous work on this band1184 cm-1 band previously measured by Joblin et al.Band strength has been measured experimentallyAllows us to estimate degree of vibrational cooling
Joblin
et al.,
Astron.
Astrophys
.
, 299, 835 (1995).Ne matrix (4 K)
CsI pellet (300 K)Gas phase (570 K)Slide5
Getting sample into the gas phase
Designed an oven to hold >50 g of sampleHorizontal orientation allows liquid sampleCan operate up to at least 700°C for hours
Need an oven that can operate up to 700°C for many hours
Needs to be able to hold large amount of sample
Must be able to hold liquidSlide6
Our mid-IR spectrometer
B. E. Brumfield et al., Rev. Sci. Instrum
.
,
81
, 063102 (2010).
Rhomb and polarizer act as an optical isolator
Total internal reflection causes a phase shift in the light
Fabry
-Perot quantum cascade lasers provided by Claire
Gmachl
at Princeton
Housed in a liquid nitrogen cryostat
Lasers can scan from ~1180-1200 cm
-1
(not necessarily continuous)Slide7
The pyrene vibrational modeThis mode is a C-H bending modePyrene is an asymmetric top (D2h point group)This is a b-type band (ΔJ = 0,±1; ΔKa
=±1; ΔKc=±1)Slide8
Overall spectrumPQQR structure of a b-type band with little intensity near the band centerStrong P and R-branches indicate a small change in rotational constants in the
vibrationally excited stateSlide9
Changing rotational constants in the excited state
Simulation from our assignment of the spectrum
Simulation with B’ decreased by 0.1% relative to B’’
Each tall peak we observe is actually a stack of many transitionsSlide10
Simulating the spectrumWe used PGOPHER to fit and simulate the spectrumGround state rotational constants published by Baba et al.Values obtained from fluorescence excitation spectroscopy
PGOPHER, a Program for Simulating Rotational Structure, C. M. Western, University of Bristol,
http://pgopher.chm.bris.ac.uk
Baba et al.,
J. Chem. Phys.
,
131
, 224318 (2009).Slide11
Cannot fit spectrum using Baba et al.’s constantsIf we allow ground and excited state constants to float during the fitting we obtain a good fit (standard deviation of 0.00036 cm-1 (11 MHz))Ground state constants from fit are statistically different from Baba et al.This discrepancy between ground state constants is still being investigated – combination differences using our data confirm our ground state assignmentDiscrepancy with fluorescence excitation spectrum
T
rot
= 20 K
linewidth
= 10 MHz
300 MHz
Our fit (cm
-1
)
Baba et al.
Difference
% difference
A’’
0.0337202(12)
0.0339147(45)
-1.95×10
-4
0.6%
B’’0.0185559(12)0.0186550(32)-9.91×10-50.5%C’’0.01197271(61)0.0120406(24)-6.79×10-50.6%Slide12
Vibrationally excited statev=0 (cm-1)
v=1Difference% Difference0
1184.035561(32)
A
0.0337202(12)
0.0337138(13)
6.4×10-60.019%B
0.0185559(12)0.0185554(12)5.0×10
-7
0.002%
C
0.01197271(61)
0.01197111(64)
1.8×10
-6
0.013%
Rotational constants change very little in the
vibrationally
excited state
B is statistically unchanged between ground and excited statesCentrifugal distortion constants were unnecessary to fit the bandSlide13
Estimating the vibrational temperatureUsing our assignment, we can calculate the expected spectrum at a vibrational temperature of 0 KCompare expected spectrum to experimental spectrum to estimate TvibEstimate column density from:rate of mass loss from the oven (25 g in ~20 hr)
gas velocity in the expansionvertical distribution in the expansionoverlap of TEM00 mode of cavity with expansion
Slide14
Estimating the vibrational temperatureBand strength for pyrene mode is known (10 km/mol)Using this information we can calculate Qvib × Ccluster to be ~1.3
Doubling backing pressure did not lead to decrease in absorption – assume Ccluster = 1 (no clustering)Use scaled harmonic frequencies to calculate Qvib as a function of temperature
S. R.
Langhoff
,
J. Phys. Chem.
,
100, 2819 (1996).Tvib
= 60 – 90 KSlide15
ConclusionsWe have measured and assigned rotationally-resolved infrared spectrum of pyreneLargest molecule observed with rotational resolution using infrared absorptionLarge molecules can be cooled effectively by supersonic expansionSlide16
Future WorkTry to resolve discrepancy between our work and fluorescence excitation spectroscopyContinue to try and observe C60 spectrumDevelop an external-cavity QCL system to extend frequency coverageContinue on to larger PAHs, such as coroneneSlide17
Acknowledgments
McCall Group
Claire
Gmachl
Richard
Saykally
Kevin Lehmann