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7/24/2019 lesson 8 uv-vis spectroscopy.pdf
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What is Spectroscopy?
The study of molecular structure and
dynamics through the absorption,
emission and scattering of light.
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What is Light?
According toMaxwell, light is anelectromagnetic field
characterized by afrequency f, velocity v( c in vacuum), andwavelength . Lightobeys therelationship
= c / .
Its energy is E= h
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The Electromagnetic Spectrum
= c / lE = h
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X-ray:
core electronexcitation
UV:
valenceelectronic
excitation
IR:
molecularvibrations
Radio waves:
Nuclear spin states(in a magnetic field)
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Spectral Distribution of Radiant Energy
Wave Number (cycles/cm)
X-Ray UV Visible IR Microwave
200nm 400nm 800nm
WAVELENGTH(nm)
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Spectroscopic Techniques
UV-vis UV-vis region bonding electrons
Atomic Absorption UV-vis region atomic transitions (val. e-)
FT-IR IR/Microwave vibrations, rotations
Raman IR/UV vibrations
FT-NMR Radio waves nuclear spin states
X-Ray Spectroscopy X-rays inner electrons, elemental
X-ray Crystallography X-rays 3-D structure
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UV = 300 kcal/mol
10-5
10-5
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Molecules have quantized energy levels:
ex. electronic energy levels.
energy
hv
energy
}= hv
Q: Where do these quantized energy levels come from?
A: The electronic configurations associated with bonding.
Each electronic energy level(configuration) has
associated with it the many
vibrational energy levels we
examined with IR.
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2s 2s
s
s*
s
s*
p*
p
2p 2pn
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C C
s
s*
hv
s
s*
s s*
C C
H
H
H H
HH
lmax
= 135 nm (a high energy transition)
Absorptions having lmax< 200 nm are difficult to observe because
everything (including quartz glass and air) absorbs in this spectral
region.
Ethane
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C C
s
s*
hv
p
p*
s
s*
p
p*
p p*
Example: ethylene absorbs at longer wavelengths:lmax= 165 nm = 10,000
= hv=hc/l
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s
s*
hv
p
p*
n
s
s*
p
p*
n
C O
p*n
The n to pi* transition is at even lower wavelengths but is notas strong as pi to pi* transitions. It is said to be forbidden.
Example:
Acetone: ns* lmax= 188 nm ; = 1860
np* lmax= 279 nm ; = 15
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C C
C C
C O
C O
H
s s* 135 nm
p p*165 nm
n s* 183 nm weak
p p* 150 nm
n s* 188 nmn p* 279 nm weak
l
A
180 nm
279 nm
C O
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C C
HOMO
LUMO
Conjugated systems:
Preferred transition is between Highest Occupied Molecular Orbital
(HOMO) and Lowest Unoccupied Molecular Orbital (LUMO).
Note: Additional conjugation (double bonds) lowers the HOMO-
LUMO energy gap:
Example:
1,3 butadiene: lmax= 217 nm ; = 21,000
1,3,5-hexatriene lmax= 258 nm ; = 35,000
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Lycopene:
lmax= 114 + 5(8) + 11*(48.0-1.7*11) = 476 nm
lmax(Actual) = 474.
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Electronic (UV) spectroscopy Light absorbedelectron excited to higher
molecular orbital Transitions occur from HOMO to LUMO
- Highest Occupied Molecular Orbital
- Lowest Unoccupied Molecular Orbital
E=h
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What functional groups are observed
in UV/vis spectrum?
UV/vis (200-600 nm)
Functional groups
KetoneEster
Amide
Conjugated D.B
Not observedC-C
C-H
C=C (isolated)
C-C
LUMO s
HOMO s
C=C
LUMO p
HOMO p
C=C-C=C
LUMO
HOMO
l=217 nm
Excitation
p4
p3
p2
p
1
l=165nm
l=125nm
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Chromophores
Chromophores- Part of molecule responsible forabsorption
Auxochromes- Groups that modify absorption ofneighboring chromophores- Often have lone pairs, e.g.OH, -OR,
-NR2, -halogen- Bathochromic shift: towards longerwavelength
- Hypsochromic shift: towards shorterwavelen th
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The wavelength and amount of light that a compound
absorbs depends on its molecular structure and theconcentration of the compound used.
T itt d
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Transmittance and
Concentration
The Bouguer-Lambert Law
PathlengthConst
eIIT
0/
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Transmittance and Path Length:
Beers Law
ionConcentratConsteIIT 0/
Concentration
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BEER LAMBERT LAW
Glass cell filled with
concentration of solution (C)
IILight0
As the cell thickness increases, the intensity of I
(transmitted intensity of light ) decreases.
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T- Transmittance
T = I0- original light intensity
I- transmitted light intensity
% Transmittance = 100 x
Absorbance (A) or optical density (OD) = Log
= Log
Log is proportional to C (concentration of solution)
and is also proportional to L (length of light path
through the solution).
I
I0
I
I0
I0
I
1
T
I
I0
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A CL = KCL by definition and it is called
the Beer Lambert Law.
A = KCL
K = Specific Extinction Coefficient ---- 1 g of
solute per liter of solution
A = ECL
E = Molar Extinction Coefficient ----
Extinction Coefficient of a solution containing
1g molecule of solute per 1 liter of solution
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L = Cm
C = Moles/Liter
A = KCL
A = No unit C = Gram/Liter L = Cm
A = ECL = ( LiterCm x Mole
) x MoleLiter
x Cm
K=
Liter
Cm Gram
A = KLC = (Liter
Cm x Gram
Gram
Literx Cm) x
UV VIS SPECTROMETERS ARE UBIQUITOUS
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P 8
BEGIN
HERE
UV-VIS SPECTROMETERS ARE UBIQUITOUS
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Characteristics of UV-Vis spectra of
Organic Molecules
Absorb mostly in UV unless highlyconjugated
Spectra are broad, usually to broad for
qualitative identification purposes Excellent for quantitative Beers Law-type
analyses
The most common detector for an HPLC
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Broad spectra
Overlapping vibrational and rotational
peaks Solvent effects
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P354
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A = 0.8
Conc: 4x10-5M
Path: 1 cm
= 0.8/4x10-5x1
= 2x104
= 20000
Isoprene
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P356
(see also 359)
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Conventional
Spectrophotometer
Schematic of a conventional single-beam spectrophotometer
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Light Sources
Hydrogen Gas Lamp
Mercury Lamp
Tungten lamp (350-2500 nm)
Deuterium (200-400 nm)
Xenon Arc lamps (200-1000 nm)
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Dispersion Devices
Non-linear dispersion
Temperature sensitive
Linear Dispersion
Different orders
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Cells
UV Spectrophotometer
Quartz (crystalline silica)
Visible Spectrophotometer
Glass
IR Spectrophotometer
NaCl
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Open-topped rectangular standard cell (a)
and apertured cell (b) for limited sample volume
Cell Types I
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Conventional
Spectrophotometer
Optical system of a double-beam spectrophotometer
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STEPS IN DEVELOPING
SPECTROPHOTOMETRIC
N LYTIC L METHOD
1. Run the sample spectrum
2. Obtain a monochromatic
wavelength for the
maximum absorption
wavelength.
3. Calculate the concentration
of your sample using Beer
Lambert Equation: A = KCLWavelength (nm)
Absorbance
0.0
2.0
200 250 300 350 400 450
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Slope of Standard Curve = A
C
1 2 3 4 5
1.0
0.5
Concentration (mg/ml)
Absorbance at 280 nm
There is some A vs. C where graph is linear.
NEVER extrapolate beyond point known where
becomes non-linear.
SPECTROMETRIC ANALYSIS USING
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SPECTROMETRIC ANALYSIS USING
STANDARD CURVE
1 2 3 4
0.4
0.8
1.2
Absorbance at 540 nm
Concentration (g/l) glucose
Avoid very high or low absorbencies when drawing a
standard curve. The best results are obtained with 0.1 < A
< 1. Plot the Absorbance vs. Concentration to get astrai ht line
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Every instrument has a useful range for a
particular analyte.
Often, you must determine that rangeexperimentally.
This is done by making a dilution series of
the known solution.
These dilutions are used to make a
working curve.
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Make a dilution series of a known quantity
of analyte and measure the Absorbance.
Plot concentrations v. Absorbance.
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What concentration do you think the
unknown sample is?
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In this graph, values above A=1.0 are not linear. If we
use readings above A=1.0, graph isnt accurate.
C lib ti M th d
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Calibration MethodsStandard Addition
1.) Protocol to Determine the Quantity of an Unknown(i) Known quantities of an analyte are added to the unknown
-known and unknown are the same analyte
- increase in analytical signal is related to the total quantity of the analyte
-requires a linear response to analyte
(ii) Very useful for complex mixtures
- compensates for matrix effect change in analytical signal caused by
anything else than the analyte of interest.
(iii) Procedure:
(a) place known volume of unknown sample in multiple flasks
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C lib ti M th d
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XS
X
ff
i
I
I
XS
X
Calibration MethodsStandard Addition
1.) Protocol to Determine the Quantity of an Unknown(iii) Procedure:
(d) Measure an analytical response for each sample
- signal is directly proportional to analyte concentration
solutionfinalfromsignal
solutioninitialfromsignal
solutionfinalindardtansplusanalyteofionConcentrat
solutioninitialinanalyteofionConcentrat
Standard addition equation:
V
VSS
V
VXX Sif
oif
dardtansofvolumeaddedV,volumeinitialunknownV,VVV SoSo
Total volume (V):
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VIS-Transmission and Color
The human eye sees the complementary color to that which is
absorbed
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