june 3 lecture _spectroscopy intro
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Chapter17: Fundamentals of Spectrophotometry
HW: To be posted after class
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Electromagnetic Radiation
-rays 0.001 - 0.01 nm Nuclear transitions
X-rays .01 -10 nm Core e-s
Ultraviolet 10 - 400 nm Valence e-s
Visible 400 - 800 nm Valence e-s
Infrared 800 - 106 nm Molecular Vibrations
Microwave 106 - 108 nm Molecular Rotations
Radio 108 - 1011 nm Nuclear Spin
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The Visible Spectrum The visible spectrum
400 nm 750 nm
IRUV
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Energy/Photons
-rays 10-14 J/photonX-rays 10
-16J/photon
Ultraviolet 10-18 J/photonVisible 10-19 J/photon
Infrared 10-20
J/photon
Microwave 10-22
J/photon
Radio 10-24
J/photon
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Absorption Energy Levels
E
N
E
R
G
Y
Electronic level
Rotational level
Vibrational level
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E = UV/Vis photon
E = IR photon
E = wave photon
E
N
E
R
G
Y
Absorption Energy Levels
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What happens to excited molecule?
1. UV-Vis Absorption: from ground state (S0) toexcited state (S1)
10-15 seconds
S0 T1: Spin-Forbidden (low probability)
2. Vibrational Relaxation: excited molecule bumps intosolvent, drains some E (radiationless transition)
10-12 seconds
Cascade down manifold of excited vibrationallevels (not electronic)
3. Internal Conversion: radiationless transition betweenstates with the same spin quantum number (S1 to S0)
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Fluorescence/Phosphorescence
4. Fluorescence: the emission of radiation from excited
state to ground state (into range of vibrational states)
10-6 to 10-10 seconds
5. More internal conversion: non-radiant relaxation
(spreading out energy/heat)
6. Intersystem crossing: radiationless transition between
states with different spin quantum numbers (S1
to T1)
7. Phosphorescence: emission of radiation from T1 to S1)
> 10-6 seconds (very long: different spins!)
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Luminescence
For fluorescence the intensity is
I = KP02.3bc
Measure absolute number of photons
I is DEPENDENT on P0
K depends upon:
efficiency of fluorescence
light collection efficiency
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1. Significant overlap across
the entire spectrum.
2. Regions of no overlap
A
X
Y A
XY
]Y[b]X[bA YXm
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Know that absorbance of mixture of X and Y at
any l is
Prepare standard solutions of X and Y
]Y[b]X[bA YXm
SXX ]X[bA S
SYY ]Y[bA S
S
X
X
b[X]
A
S
S
Y
Yb[Y]
A
S
Case 1
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SX
Y
SX
m
]X[
]X[
A
A
]Y[
]Y[
A
A
S
S
S
b[Y]
b[Y]
Ab[X]
b[X]
AA
S
Y
S
X
mSS
S
Y
S
X
m[Y]
[Y]A
[X]
[X]AA SS
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SX
Y
SX
m
]X[
]X[
A
A
]Y[
]Y[
A
A
S
S
S
y = m x + b
Case 1
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How do we get enough data points to construct a line?
Case 1
SX
m
A
A
S
S
X
Y
A
AFind[Y]fr
omslope
Find [X] from y-intercept
SX
m
A
A
S
S
X
Y
A
AFind[Y]fr
omslope
Find [X] from y-intercept
SX
Y
SX
m
]X[
]X[
A
A
]Y[
]Y[
A
A
S
S
S
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i. measure absorbance at lmax for X
ii. measure absorbance at lmax for Y
A
X
Y
l l
]Y[b]X[bA YX
]Y[b]X[bA YX
Case 2
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Isosbestic points
Analytical useful if one analyte (X) can be converted toanother (Y) and/or vice versa.
Examples:
X = B (base) and Y = HB+ (conjugate acid)
X = HA (acid) and Y = A- (conjugate base)
Characteristic feature of mixture of X and Y Abs spectra
REQUIREMENT:
Absorbance spectra of pure X and pure Y must cross
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Absorbance spectra of separate solutions of
HA and A- prepared at same concentration
HA
A- ]HA[bA465HA
465HA
]A[bA 465A
465
A
465
A
465
HA
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Vary pH of a solution to vary principal species
pKa = 5.1
HA A- + H+
Will these peaks necessarily be equal?
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]A[b]HA[bA 465A
465HA
465m
465
A
465
HA
])A[]HA([bA465465
m
Mass balance: ([HA] + [A-]) = constant
The Absorbance at 465 is constant!
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Other analytical uses:
Monitor progress of titration (equivalence point) by
following absorbance.
Useful in situations where analyte and producthave very different values at a given l
Example: analyte has color but product does not,or vice versa.
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Due to large number of vibrational states,
IR spectra can be quite complex
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IR Absorption: real strength is ID
Functional Group Wavenumber(cm-1)
Wavelength( m)
C-H, aliphatic 3000-2850 3.3-3.5
C-H, aromatic 3150-3000 3.2-3.3
O-H 3600-3000 2.8-3.3
C=O,
aldehyde/ketone
1740-1660 5.7-6.0
-CH2Cl 1300-1200 7.6-8.2
C-C 850-890 13.2-14.0
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