u toronto, february 18, 2011darin j. ulness, concordia college 1 noisy light spectroscopy noisy...
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U Toronto, February 18, 2011Darin J. Ulness, Concordia College 1Noisy Light Spectroscopy
Noisy LightSpectroscopy:
Putting noise to good use
Darin J. UlnessDepartment of Chemistry
Concordia CollegeMoorhead, MN
U Toronto, February 18, 2011Darin J. Ulness, Concordia College 2Noisy Light Spectroscopy
OutlineI. IntroductionII.TheoryIII. Experiment
• Coherent Raman Scattering
IV. Connections
U Toronto, February 18, 2011Darin J. Ulness, Concordia College 3Noisy Light Spectroscopy
SpectroscopyUsing light to gain information about matter
• Lineshape function• Transition frequencies• Cross-sections• Susceptibilities
Information Uses of information• In Chemistry• In Biology• In Engineering
U Toronto, February 18, 2011Darin J. Ulness, Concordia College 4Noisy Light Spectroscopy
Modern SpectroscopyFrequency Domain• Measure Spectra• Examples• IR, UV-VIS, Raman
• Material response• Spectrally narrow• Temporally slow
Time Domain• Response to light pulse• Examples• PE, transient abs.
• Material response• Spectrally broad• Temporally fast
U Toronto, February 18, 2011Darin J. Ulness, Concordia College 4Noisy Light Spectroscopy
Modern SpectroscopyFrequency Domain• Measure Spectra• Examples• IR, UV-VIS, Raman
• Material response• Spectrally narrow• Temporally slow
Time Domain• Response to light pulse• Examples• PE, transient abs.
• Material response• Spectrally broad• Temporally fast
U Toronto, February 18, 2011Darin J. Ulness, Concordia College 4Noisy Light Spectroscopy
Modern SpectroscopyFrequency Domain• Measure Spectra• Examples• IR, UV-VIS, Raman
• Material response• Spectrally narrow• Temporally slow
Time Domain• Response to light pulse• Examples• PE, transient abs.
• Material response• Spectrally broad• Temporally fast
Is there another useful technique?Noisy light? YES!
U Toronto, February 18, 2011Darin J. Ulness, Concordia College 5Noisy Light Spectroscopy
Light
frequency
Spectrum
time
One frequency (or color)
Electromagnetic radiation•Focus on electric field part
U Toronto, February 18, 2011Darin J. Ulness, Concordia College 6Noisy Light Spectroscopy
Noisy Light: Definition• Broadband• Phase incoherent• Quasi continuous wave
Ele
tric
Fie
ld S
tren
gth
Time
Noi
sy L
ight
Spe
ctru
m
Frequency
Time resolution onthe order of the correlation time, tc
U Toronto, February 18, 2011Darin J. Ulness, Concordia College 7Noisy Light Spectroscopy
Noisy Light: Alternative• Its cw nature allows precise measurement
of transition frequencies.• Its ultrashort noise correlation time offers
femtosecond scale time resolution.• It offers a different way to study the
lineshaping function.• It is particularly useful for coherent
Raman scattering.• Other spectroscopies: photon echo, OKE,
FROG, polarization beats…
U Toronto, February 18, 2011Darin J. Ulness, Concordia College 8Noisy Light Spectroscopy
Theory
Optical coherence theory
Perturbation theory: Density operator
Noisy Light Spectroscopy
U Toronto, February 18, 2011Darin J. Ulness, Concordia College 9Noisy Light Spectroscopy
Theoretical Challenges•Complicated Mathematics•Complicated Physical Interpretation
Difficulty•The cw nature requires all field action permutations. The light is always on.
•The proper treatment of the noise cross-correlates chromophores.
U Toronto, February 18, 2011Darin J. Ulness, Concordia College 10Noisy Light Spectroscopy
Bichromophoric Model
a
b
Noisy light
P(t)(3)
P(s)(3)*
< >
Solution•Factorized time correlation (FTC) diagram analysis
U Toronto, February 18, 2011Darin J. Ulness, Concordia College 11Noisy Light Spectroscopy
FTC Diagram Analysis
Set of intensity level terms
(pre-evaluated)
Set of evaluated intensity level
terms
Messy integration and algebra
Set of FTC diagrams
ConstructionRules
EvaluationRules
Physicshard hard
easy
U Toronto, February 18, 2011Darin J. Ulness, Concordia College 12Noisy Light Spectroscopy
Example: I(2)CARS
a
b
P(t,{ti})
P(s,{si})
arrow segments: t-dependent correlation
line segments: t-independent
correlation
U Toronto, February 18, 2011Darin J. Ulness, Concordia College 13Noisy Light Spectroscopy
Experiment•Coherent Raman Scattering: e.g., CARS•Frequency resolved signals•Spectrograms•Molecular liquids
U Toronto, February 18, 2011Darin J. Ulness, Concordia College 14Noisy Light Spectroscopy
Nonlinear Optics
P= c ESignal
Material
Light field
Perturbation series approximation
P(t) = P(1) + P(2) + P(3) …
P(1) = c (1)E, P(2) = c (2)EE, P(3) = c (3)EEE
U Toronto, February 18, 2011Darin J. Ulness, Concordia College 15Noisy Light Spectroscopy
CARSCoherent Anti-Stokes Raman Scattering
wR
w1
w1w2
wCARS
w1-w2= wR
wCARS= w1 +wR
U Toronto, February 18, 2011Darin J. Ulness, Concordia College 16Noisy Light Spectroscopy
CARS with Noisy Light•I(2)CARS• We need twin noisy beams B and B’.• We also need a narrowband beam, M.• The frequency of B (B’) and M differ by
roughly the Raman frequency of the sample.• The I(2)CARS signal has a frequency that is
anti-Stokes shifted from that of the noisy beams.
B
B’M
I(2)CARS
U Toronto, February 18, 2011Darin J. Ulness, Concordia College 17Noisy Light Spectroscopy
I(2)CARS: Experiment
Monochromator
NarrowbandSource
BroadbandSource(noisy light)
Lens
Sample
Interferometer
t
B
B’
MI(2)CARS
ComputerCCD
U Toronto, February 18, 2011Darin J. Ulness, Concordia College 18Noisy Light Spectroscopy
I(2)CARS: SpectrogramMonochromator
NarrowbandSource
BroadbandSource
Lens
Sample
Interferometer
t
B
B’
MI(2)CARS
ComputerCCD
• Signal is dispersed onto the CCD
• Entire Spectrum is taken at each delay
• 2D data set: the Spectrogram
U Toronto, February 18, 2011Darin J. Ulness, Concordia College 19Noisy Light Spectroscopy
I(2)CARS: Spectrogram
Pixel A
A
Pixel B
B
Pixel C
C
Dark regions: high intensityLight regions: low intensity
Oscillations: downconversion of Raman frequency.Decay: Lineshape function
U Toronto, February 18, 2011Darin J. Ulness, Concordia College 20Noisy Light Spectroscopy
SpectrogramNo new information can be extracted.
However…
• Huge oversampling gives much enhanced precision.
• Visually appealing presentation of data gives much insight.
U Toronto, February 18, 2011Darin J. Ulness, Concordia College 21Noisy Light Spectroscopy
I(2)CARS: Data Processing
18000 18100 18200 18300 18400
-2
-1
0
1
2
BenzeneT22
0 200 400 600 800 1000 1200
0
25
50
75
100
125
150
BenzeneT22
100 200 300 400
0.2
0.4
0.6
0.8
Fourier
Transformation
X-Marginal
U Toronto, February 18, 2011Darin J. Ulness, Concordia College 22Noisy Light Spectroscopy
Virtues of I(2)CARS•Less expensive.•Easier experiment to perform.•Signals are more robust.• Immune to dispersion effects. •Exquisitely sensitive to relative changes in the vibrational frequency and dephasing rate constant.
U Toronto, February 18, 2011Darin J. Ulness, Concordia College 23Noisy Light Spectroscopy
17300 17400 17500 17600
-400
-200
0
200
400
Pyridine
Pyridine and Water
17300 17400 17500 17600
-400
-200
0
200
400
Pyridine
17300 17400 17500 17600
-400
-200
0
200
400
ave x.45 pyr_water
FT
NeatPyridine
Pyridine/Water Xw= 0.55
U Toronto, February 18, 2011Darin J. Ulness, Concordia College 24Noisy Light Spectroscopy
Pyridine and Water
-0.2
0
0.2
0.4
0.6
0.8
1
1.2
955 975 995 1015 1035 1055
pure pyr
x=.15
x=0.3
x=0.45
x=0.75
Wavenumber / cm-1
U Toronto, February 18, 2011Darin J. Ulness, Concordia College 25Noisy Light Spectroscopy
Pyridine and Water
960 970 980 990 1000 1010 1020 1030 1040
0.0
0.2
0.4
0.6
0.8
1.0 Pyridine/water solution: X(py)=0.6
T = -4o
T = 3o
T = 23o
T = 32o
T = 42o
T = 52o
T = 62o
T = 72o
T = 76o
No
rma
lize
d X
-ma
rgin
al
Wavenumber / cm-1
U Toronto, February 18, 2011Darin J. Ulness, Concordia College 26Noisy Light Spectroscopy
Halogen bondingPyridine and C3F7I
0
0.5
1
1.5
2
2.5
3
3.5
4
900 920 940 960 980 1000 1020 1040 1060 1080 1100
Frequency (cm-1)
Norma
lized In
tensity
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
0.9
Neat
C6F13I and Pyridine
0
0.5
1
1.5
2
2.5
3
3.5
4
900 920 940 960 980 1000 1020 1040 1060 1080 1100Frequency (cm-1)
Norma
lized In
tesity
Neat
0.1
0.2
0.3
0.4
0.5
0.6
0.7
.8
0.9
U Toronto, February 18, 2011Darin J. Ulness, Concordia College 27Noisy Light Spectroscopy
ProspectusSummary:•Noisy light provides an alternative method for probing ultrafast dynamics of the condensed phase.
•Experimentally it is relatively easy.•Theoretically it is relatively hard.•FTC diagram analysis helps with theoretical understanding.
U Toronto, February 18, 2011Darin J. Ulness, Concordia College 28Noisy Light Spectroscopy
ProspectusFuture of noisy light at Concordia:• I(2)CARS is an exquisitely sensitive probe of vibrational frequency shifts
•A principle goal is to explore halogen bonding. I(2)CARS is one tool available to us.
U Toronto, February 18, 2011Darin J. Ulness, Concordia College 29Noisy Light Spectroscopy
ConnectionsCoherent Energy Transfer:•Noisy light can produce a nonlinear response.
•Noisy light is “incoherent.” •Amplitude level correlation.
U Toronto, February 18, 2011Darin J. Ulness, Concordia College 30Noisy Light Spectroscopy
Connections
< >
P(t) P(s)
Stimulus
“ReactionCenter”
U Toronto, February 18, 2011Darin J. Ulness, Concordia College 31Noisy Light Spectroscopy
AcknowledgementsFormer StudentsTheoryJahan DawlatyDan BiebighauserJohn GregioreDuffy Turner
Other Group MembersDr. Mark Gealy, Department of PhysicsDr. Eric Booth, Post-doctoral researcherDr. Haiyan Fan, Post-doctoral researcher
FundingNSF CAREER Grant CHE-0341087Henry Dreyfus Teacher/Scholar programConcordia Chemistry Research Fund
Method DevelopmentPye Phyo AungTanner SchulzLindsay WeiselKrista CosertPerrie ColeAlex HarshBritt BergerZach JohnsonThao Ta
Hydrogen/Halogen bondingEric BergJeff EliasonDiane MolivaJason OlsonScott FlancherDanny Green
U Toronto, February 18, 2011Darin J. Ulness, Concordia College Noisy Light Spectroscopy
U Toronto, February 18, 2011Darin J. Ulness, Concordia College A1Noisy Light Spectroscopy
Utility of FTC Diagrams•Organize lengthy calculations•Error checking• Identification of important terms• Immediate information of about features of spectrograms
•Much physical insight that transcends the choice of mathematical model.
U Toronto, February 18, 2011Darin J. Ulness, Concordia College A2Noisy Light Spectroscopy
Example: I(2)CARS
a
b
P(t,{ti})
P(s,{si})
arrow segments: B, B’ correlation
t-dependentline segments: B, B or B’,B’ correlation
t-independent
FTC analysis• Each diagram with arrows
has a topologically equivalent partner diagram containing only lines: 2:1 dynamic range
• Each diagram with arrows has a topologically equivalent partner diagram that has arrows pointing in the opposite direction: signal must be symmetric in t
U Toronto, February 18, 2011Darin J. Ulness, Concordia College A3Noisy Light Spectroscopy
Example: I(2)CARS
Pixel A
A
Pixel B
B
Pixel C
C
The I(2)CARS data shows • 2:1 dynamics range• t symmetry
U Toronto, February 18, 2011Darin J. Ulness, Concordia College A4Noisy Light Spectroscopy
0 1 2 3 4 50.00
0.05
0.10
0.15
0.20
0.25
0.30
s g
S/N
(a)
0 1 2 3 4 50.00
0.05
0.10
0.15
0.20
0.25
0s w
D
S/N
(b)
U Toronto, February 18, 2011Darin J. Ulness, Concordia College A5Noisy Light Spectroscopy
U Toronto, February 18, 2011Darin J. Ulness, Concordia College A6Noisy Light Spectroscopy
U Toronto, February 18, 2011Darin J. Ulness, Concordia College A7Noisy Light Spectroscopy
-20 0 20 40 60 800.8
0.9
1.0
1.1
1.2
1.3
1.4
1.5
Fit Results:ratio =0.00783 T + 0.905R = 0.9942
Fre
e p
yr.
to
H-b
ou
nd
pyr
Temperature (Co)
- ∆G° Product Favored
- ∆H° Exothermic
- ∆S° Entropically unfavorable
U Toronto, February 18, 2011Darin J. Ulness, Concordia College A8Noisy Light Spectroscopy
17300 17400 17500 17600
-400
-200
0
200
400
pyridine with .4g AgNO3
960 970 980 990 1000 1010 1020 1030 1040-0.2
0.0
0.2
0.4
0.6
0.8
1.0Pyridine / AgNO
3
g AgNO3/ml py
0.00 0.061 0.097 0.121 0.170 0.238 0.298 0.341 0.409
No
rma
lize
d X
-ma
rgin
al
Wavenumber / cm-1
0.00 0.05 0.10 0.15 0.20 0.25-0.2
0.0
0.2
0.4
0.6
0.8
1.0
1.2
1.4 Pyridine/AgNO3
Ratio
27.1 Xeff
2 -.97 X
eff + 0.013
Co
mp
lexe
d p
yri
din
e t
o
Fre
e p
yri
din
ed
Effective mole fraction AgNO3
c(3)complex = Icomplex c(3)
free xfree
Icomplex = Ifree at 0.21 mole fraction
c(3)complex = 1 c(3)
free .79
c(3)complex = 3.76 c(3)
free