Practical Absorption Spectrometry: Ultraviolet Spectrometry Group
CHAPTER 2 ULTRAVIOLET-VISIBLE ABSORPTION...
Transcript of CHAPTER 2 ULTRAVIOLET-VISIBLE ABSORPTION...
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CHAPTER 2
ULTRAVIOLET-VISIBLE
ABSORPTION SPECTROSCOPY
Expected Outcomes
Able to discuss the interaction of electromagnetic waves with atomic and molecular species
Describe the transmittance and absorbance
State the functions of each components of instrumentation for optical spectroscopy
Differentiate the type of optical instruments
Describe the function of ultraviolet-visible instrument
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2.1 Electromagnetic spectrum
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http://mail.colonial.net/~hkaiter/electromagspectrum.html
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Theory of Electromagnetic Radiation
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Charged particles emit or absorb energy in a wavelike form known as electromagnetic radiation.
This radiation consists of two components: an electric field and a magnetic field
EM radiation travels at the speed of light, in a vacuum
The basic unit of EM radiation is the photon,
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Theory of Electromagnetic Radiation
Electromagnetic Radiation
• Wave properties:
v = c c = velocity of light (3.0x108 ms-1 in vacuum) = wavelength (m) v = frequency (cycles/s, cps, Hz)
• Particle properties (Photon energy)
E = energy of quantum (J)
h = Planck’s constant (6.63 x 10-34 J.s)
v = frequency
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Absorption of Radiation
• The energy difference between the two energy states, E1 and Eo, must be equal to the energy of the absorbed radiation (E = hv).
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E1
(excited state)
E0 (ground state)
Theory of Electromagnetic Radiation
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Atomic Absorption
• When atoms absorb radiation, only e-s are excited.
• Line spectrum can be observed.
• Electronic transition - The transition of an e- between two orbitals.
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Theory of Electromagnetic Radiation
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Molecular Absorption
•Molecules undergo three types of quantized transitions when excited by ultraviolet, visible, & infrared radiation:
Electronic transition
Vibrational transition
Rotational transition
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Decrease in
energy
Theory of Electromagnetic Radiation
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• Absorption of Radiation • When light passes through an object, the object will absorb certain of the
wavelengths, leaving the unabsorbed wavelengths to be transmitted.
• These residual transmitted wavelengths will be seen as a colour.
• The absorption can be detected by suitable detectors
Absorption and Emission
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Absorption and Emission
nm Colour Complimentary
~180-380 UV -
400-435 Violet Yellow-green
435-480 Blue Yellow
480-490 Blue-green Orange
490-500 Green-blue Red
500-560 Green Purple
560-580 Yellow-green Violet
580-595 Yellow Blue
595-650 Orange Blue-green
650-750 Red Green-blue
Visible spectrum
UV
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Question?
• Why is the red solution red?
Because the object absorbs
green component from the
incoming white radiation and
thus transmits red
components.
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A plot of the amount of radiation absorbed
by a sample as a function of the
wavelength is called an absorption
spectrum
Absorption and Emission
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Absorption and Emission
UV-VIS absorption spectrum for
bromothymol blue
0
0.2
0.4
0.6
0.8
350 450 550 650 750
wavelength (nm)
Ab
so
rban
ce
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Absorption and Emission • Emission of a photon occurs when an analyte in a
higher energy state returns to a lower energy state.
• The higher energy state can be achieved by heat, photon and chemical reaction
• The emission of the sample itself provides the light and the intensity of the light emitted is a function of the analyte concentration.
• When molecules or atoms are in the excited state, they are very unstable and will lose their energy of excitation and drop back to a lower energy state or the ground state – relaxation.
The excess energy is released in the form of electromagnetic radiation, heat, or both.
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Po = initial radiant power
P = final radiant power
Transmittance: T = P / Po ,
% Transmittance: %T = P / Po x 100%
Absorbance:
Po P
The Beer’s Law
bcTP
PA o
1loglog
L mol-1 cm-1
cm
mol L-1
2.2 Transmittance & Absorbance
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The Beer’s Law
Transmittance (T): the ratio of the radiant power (P) in a beam of radiation after it has passed through a sample to the power of the incident beam (Po).
Absorbance (A) is also known as the optical density, = log (base 10) of the reciprocal of the transmittance (T).
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What values of absorbance correspond to
100%T, 10%T, and 1%T?
Exercise 2
Solution:
100%T, 10%T, and 1%T correspond to transmittances of 1.00, 0.10 and 0.010.
From the definition of A:
100%T has A = -log1 = 0
10%T has A = -log0.10 = 1.0
1%T has A = -log0.010 = 2.0
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A = Absorbance
b = Optical path distance (cm)
= Molar absorptivity (M-1cm-1)
c = Concentration (M)
The Beer’s Law
Absorption of radiant energy
When radiation of specified wavelength is passed through a solution containing only one solute which absorbs that wavelength, the absorbance (no units) can be calculated by:
A = b c
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Exercise 3
Monochromatic light was passed through a 1.00 cm cell containing a 0.0100M solution of a given substance. The absorbance obtained was 0.245. Calculate the molar absorptivity of the substance.
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0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0 2 4 6 8 10
Concentration
Ab
so
rb
an
ce
A = bc
The Beer’s law
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Deviation from Beer’s Law
Non-linear curve may be obtained due to:
1. Fundamental limitations of Beer’s law
2. Chemical deviations
3. Instrumental deviations
The Beer’s Law
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Concentration
Abso
rpti
on
Negative deviation
Positive deviation Ideal Calibration Curve
The Beer’s Law
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Fundamental limitations of Beer’s law Beer’s Law is only valid for: Low concentration of analyte. At high conc. (usually >0.01M): the individual particles of analyte no longer
behave independently of one another The absorbance changes - value of changed
- deviation from Beer’s Law
High concentration of solute may result in a shift of maximum
absorption, and may also change the value of the molar absorptivity, .
The Beer’s Law
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• depends on sample’s refractive index (RI).
• Thus, may change at high conc but at low conc, RI remains essential constant.
• Calibration curve will be linear.
2. Chemical limitations of Beer’s law • Occur for absorbing species that are involved in an
equilibrium reaction. For example in the case of weak acid and conjugate base
The Beer’s Law
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Example
Benzoic acid exists as a mixture of ionised and unionised form:
C6H5COOH + H2O C6H5COO- + H3O
+
( max = 273 nm) ( max = 268nm)
In higher dilution, or higher pH, more ionised
benzoate is formed, thus the absorbance at 273nm
decreases. On the other hand, at lower pH,
benzoic acid remains in its unionised form whereby
the absorbance at 273 nm is optimised.
The Beer’s Law
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A
Conc
273nm
268nm
The Beer’s Law
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3. Instrumental deviations • Beer’s law is only valid for monochromatic
radiation.
• The output from a continuous source (D2 lamp) will always produce a specific band width (about +5 nm).
• e.g. 220 nm may imply 215 to 225 nm
The Beer’s Law
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2.3 Components of Instrumentation for Optical Spectroscopy
Source Monochromator Sample
Detector
Meter
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Components of Instrumentation for Optical Spectroscopy
Components
Most spectroscopic instruments are made up of : 1. source 2. wavelength selector 3. sample container 4. detector 5. signal processor and readout
http://analytical.biochem.purdue.edu/~courses/undrgrad/221/www
board/handouts/supplemental/spectrophotometry.pdf
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Components of Instrumentation for Optical Spectroscopy
Spectroscopic sources
A good radiation source should have the following characteristics :
• the beam emits radiation over a wide range of the spectrum.
• sufficient intensity to be detectable.
• stable
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Components of Instrumentation for Optical Spectroscopy
• Line source – consists of one or more very narrow bands of radiation whose wavelengths are known exactly (Hollow cathode lamp)
• Continuous source – produces radiation of all wavelengths within a certain spectral region (D2 lamp)
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Components of Instrumentation for Optical Spectroscopy
• Source of radiant energy for:
• Visible region: tungsten filament lamp • UV region: deuterium discharge lamp (D2)
(a) A tungsten lamp.
(a) A deuterium lamp.
[Picture taken from Analytical Chemistry
by Gary D. Christian Page 530 and 531]
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Components of Instrumentation for Optical Spectroscopy
Wavelength selector
• Monochromator (Monochrome = “one colour”)
to spread out or disperse light into its component wavelengths and select the required wavelength for analysis.
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Components of Instrumentation for Optical Spectroscopy
• Function of monochromator • Restricts the wavelength that is to be used to a narrow band
• Enhance the selectivity and sensitivity of an instrument
• Narrow bandwidth => better adherence to Beer’s law
• Not possible to produce radiation of a single wavelength
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Components of Instrumentation for Optical Spectroscopy
• Components of a monochromator: • Entrance slit (restrict unwanted radiation)
• Dispersing element (separate the wavelengths of the polychromatic radiation)
• prism • reflection grating
• Exit slit – adjustable (control the width of the band of wavelengths)
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Components of Instrumentation for Optical Spectroscopy
Bunsen prism monochromator
[Picture taken from Fundamentals of Analytical Chemistry by Douglas A. Skoog, Donald M. West
and F. James Holler Page 536]
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Components of Instrumentation for Optical Spectroscopy
Grating
Monchromator
[Pcture taken from Modern
Analytical Chemistry by
David Harvey, pg 378]
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Components of Instrumentation for Optical
Spectroscopy
Sample container
• Must be transparent in the wavelength region being measured
• UV-VIS spectroscopy
– UV region: cell or cuvette of quartz
– VIS region: cell or cuvette of quartz/glass/plastic
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Components of Instrumentation for Optical Spectroscopy
• Cells should be optically matched (in pair).
• Selection of cells depends on:
- wavelength of radiation used
- amount of sample available
- nature of sample liquid (aqueous / organic) or gas
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Components of Instrumentation for Optical Spectroscopy • Size of curvette = 1cm x 1cm (square base)
• Volume used= 0.5ml to 2ml depending on the sample size.
Some typical UV and visible absorption cells
[Picture taken from
Analytical Chemistry
by Gary D. Christian
Page 427]
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Components of Instrumentation for Optical Spectroscopy
Detector
• Photons are detected by: • Photoemission or
• Photoconduction
All photon detectors are based on the interaction of
radiation with a reactive surface to produce electrons
(photoemission) or to promote electrons to energy states in
which they can conduct electricity (photoconduction). Only
UV, visible and near-IR radiation have sufficient energy to
cause these processes to occur.
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Components of Instrumentation for Optical Spectroscopy
Photomultiplier tubes
A photomultiplier contains a photo-emissive cathode and several anodes (dynodes) in a vacuum. The cathode is coated with an easily ionized material such as alloys of alkali metals (K, Na, Ca, Mg) with Sb, Bi and / or Ag.
A photon falling on the surface of the cathode causes the emission of an electron, provided the photon is sufficiently energetic to ionize the material. The signal is amplified by the process of secondary emission (as shown on next slide). The electron amplification depends on the voltage.
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Components of Instrumentation for Optical Spectroscopy
• Photomultiplier Tube
Quartz Window
Light Photocathode
Dynode 2
e-
current
Dynode 1
anode
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• The emitted electrons accelerate towards the dynode 1, which has higher voltage than cathode.
• Upon striking the dynode 1, each accelerated photoelectron produces more electrons. These electrons again accelerated to dynode 2, which again has a higher voltage than dynode 1. This results in electron amplification where it is finally collected at anode to measure the current electronically.
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Components of Instrumentation for Optical Spectroscopy
• Photomultiplier Tube
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Optical Instruments
• Single Beam - • Sample and reference cells are read at different time.
• Recalibration with the blank is necessary periodically due to fluctuations and wavelength changes from the radiation source.
• Double Beam - • Monochromatic beam is split into two components. (one beam for sample,
one beam for reference)
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[Picture taken from Fundamentals of Analytical Chemistry by Douglas A. Skoog, Donald M. West and F. James Holler Page
553]
Single-Beam Instruments
2.4 Type of Optical Instruments
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Double-beam Instrument
[Picture taken from Fundamentals of Analytical Chemistry by Douglas A. Skoog, Donald M. West and F. James Holler Page
553]
Optical Instruments
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Advantages of double - beam spectrophotometer:
1. Sample and reference cells can be read simultaneously.
2. Compensate the fluctuations and wavelength changes from the radiation source.
3. Allows continuous recording of spectra (absorbance as a function of wavelength).
Optical Instruments
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2.5 UV-VIS absorption spectrometry
Introduction
• Visible and UV Spectroscopic regions & associated energy levels :
Near-ultraviolet Visible
200nm 380nm 780nm
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Absorption in the UV-VIS Region
The UV region extends from about 10 – 380nm, but the most analytically useful region is from 200 – 380nm, called the near-UV region. Below 200nm, the air absorbs substantially and the instruments are operated under vacuum conditions (vacuum-UV region).
Absorption in the UV and visible region result in electronic transition.
The visible region is the wavelength that can be seen by the human eyes. It extends from the near-UV region (380nm) to about 780 nm.
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Absorption in the UV-VIS Region
Absorbing Species (Chromophores) • The wavelength at which an organic molecule absorbs
depends upon how tightly its electrons are bound. • Shared electrons in single bonds of organic compounds are
very firmly held => absorption at wavelengths in the vacuum UV region (<180 nm) => not used for analytical purposes.
• Electrons in double and triple bonds are not as strongly held => useful absorption peaks in the UV region.
• The absorbing groups (unsaturated organic groups) in a molecule are called chromophores but a molecule containing a chromophore is called a chromogen.
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Absorption in the UV-VIS Region
What can be analysed?
Chemical species that can absorb UV-VIS radiation
Chemical species that can form soluble complexes with chromophoric reagents
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Absorption in the UV-VIS Region
•Chemical species that can absorb UV-VIS radiation
• Organic chromophoric groups: unsaturated bonds • Saturated organic cpds with heteroatoms such as O, N, S or halogens
• Containing non-bonding electrons that can be excited within 170 – 250 nm for absorption.
• Ions of the transition metals • Transition between filled and unfilled d-orbitals • First two rows of transition metals - coloured
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Absorbing species
• Electronic transitions
p, s, and n (non-bonding) electrons
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Sigma and Pi orbitals
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Chromophore Example Excitation λmax, nm ε Solvent
C=C Ethene π __> π* 171 15,000 hexane
C≡C 1-Hexyne π __> π* 180 10,000 hexane
C=O Ethanal n __> π*
π __> π*
290
180
15
10,000
hexane
hexane
N=O Nitromethane n __> π*
π __> π*
275
200
17
5,000
ethanol
ethanol
C-X X=Br
X=I
Methyl bromide
Methyl Iodide
n __> σ*
n __> σ*
205
255
200
360
hexane
hexane
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Absorption in the UV-VIS Region
•Chemical species that can form soluble complexes with chromophoric reagents.
Examples
thiocyanate ion for iron, cobalt, & molybdenum;
diethyldithiocarbamate for copper; diphenylthiocarbazone for lead; 1,10-phenanthroline for iron.
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2.5.1 Absorption in the UV-VIS Region
In spectrometric analysis, there are two major approaches: One is to measure the radiant energy absorbed by the ions or molecule itself.
Most organic species and some inorganic species absorb ultraviolet or visible radiation and can be used for spectrophotometric analysis.
The other approach is used on species that do not absorb significant amounts of light through the formation of Complex Formation. A suitable chemical reagent is added to convert them to a new species that absorbs light strongly.
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Qualitative and Quantitative Analysis by UV-VIS Spectroscopy
• The application of UV-VIS spectroscopy in qualitative analysis is limited due to:
- the absorption bands tend to be broad and hence lacking in details
- several absorbing compounds might absorb over similar wavelength ranges and the absorption spectra might overlap considerably.
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Quantitative Analysis
Standard Curve Method
(External Standard Method)
Standard Addition Method
Qualitative and Quantitative Analysis by UV-VIS Spectroscopy
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Standard Curve Method
(External Standard Method)
The standard curve method is carried out as follows:
1. Ensure only the analyte in solution will absorb UV-VIS radiation strongly and not other substances in the sample.
2. Select the measurement wavelength, max, which is most sensitive to the analyte (i.e. maximum absorbance)
3. Select an appropriate range of standard solutions.
2.5.2 Qualitative and Quantitative Analysis by UV-VIS Spectroscopy
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4. Prepare standard solutions and sample.
5. Take absorbance readings of standard solutions and plot absorbance vs. concentrations.
6. Take absorbance of sample and read off from calibration graph.
Absorbance of unknown solution must be
within linear line. If it is outside range,
dilution must be carried out.
Qualitative and Quantitative Analysis by UV-VIS Spectroscopy
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0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0 2 4 6 8 10
Concentration
Ab
so
rb
an
ce
Qualitative and Quantitative Analysis by UV-VIS Spectroscopy
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• Ideally, calibration standards should be similar to the composition of the sample to minimize effects of various other components (matrix effect/interference).
Qualitative and Quantitative Analysis by UV-VIS Spectroscopy
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Example:
Testing of phosphate content in cola samples
PO43- + Reagent Yellow colour complex
The cola colour itself will impart a darker colour as compared to the standard solutions. This background colour from the sample causes matrix (or background) interference. Thus it actually gives a higher absorbance reading.
Qualitative and Quantitative Analysis by UV-VIS Spectroscopy
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• To overcome this matrix interference • Include a “sample blank” in the standard curve method.
• Sample Blank = contains solvent + sample (same dilution as the sample solution) except the reagent for complex reaction.
• Use Standard-Addition method.
Qualitative and Quantitative Analysis by UV-VIS Spectroscopy
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Standard Addition Method
This method is used when:
1. The solid or liquid matrix of a sample is either unknown or so complex that an external standard cannot be used with confidence.
2. The chemistry of the preparation or of the experimental method is complex or highly variable.
Qualitative and Quantitative Analysis by UV-VIS Spectroscopy
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The standard addition method is carried out as follows:
1. Fixed amounts of the unknown are added to each of the standard solutions.
Example:
2. Measurement is taken for each solution.
3. The absorbance is plotted against concentration.
4. The concentration of the unknown is obtained by extrapolation to zero-absorbance.
Standard solution 0 mL 1 mL 2 mL 3 mL
Sample 1 mL 1 mL 1 mL 1 mL
Qualitative and Quantitative Analysis by UV-VIS Spectroscopy
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4 0
0.2
0.4
0.6
0.8
1
-1 1 2 3
Conc.
Ab
so
rb
an
ce
Conc of
analyte in
the sample
Qualitative and Quantitative Analysis by UV-VIS Spectroscopy
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Qualitative and Quantitative Analysis by UV-VIS Spectroscopy
[Picture taken from Contemporary Chemical Analysis by Judith F. Rubinson and Kenneth A. Rubinson, Pg119]
Example
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• Limitations are= the assay response must be selective enough so that the response only comes from the analyte.
• The concentration range over which the instrument response remains linear tends to be quite narrow (factor of 10)
• Benefit = allow compensation for quite complex effects.
• Disadvantage=tedious as a set of standard solution are to be prepared for each sample. Imagine that you have a lot of samples. How?
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Applications of UV-VIS Spectroscopy
Selection of Wavelength
• Absorbance measurement are usually made at the max of the analyte change in absorbance per unit concentration is greatest.
max is usually determined experimentally by
measuring the spectrum (absorbance vs.
wavelength) of the analyte in the selected solvent.
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Applications of UV-VIS Spectroscopy
Applications
UV-VIS spectroscopy is commonly used for quantitative analysis.
Examples:
• Environmental • Phenol, chlorine, fluoride in water and wastewater
• Pharmaceuticals • Antibiotics, hormones, vitamins and analgesics • E.g., determine purity of aspirin tablets