SPECTROPHOTOMETRY
Aqsa Mushtaq
2012
-
ag-765
M-phil Pharmacolo
SPECTROPHOTOMETRY
Spectrophotometry is the study of the reflection or transmission
properties of a substance as a function of wavelength. It is the
quantitative study of electromagnetic spectra of a material
.
2 Spectrophotometer
Spectroscopy is any procedure that uses the interaction of
Electromagnetic Radiation (EMR) with matter to identify and/or to
estimate an analyte.
3
Qualitative
Analysis
Quantitative
Analysis
Electromagnetic radiation
(light)
molecules solid
ions liquid
atoms gas
Mixtures solutions
 EMR can be described in
terms of both particles and
waves (Dual nature of light)
 Light waves consist of
perpendicular and oscillating
electric and magnetic fields
Spectophotometry is historically just spectrometry where the light is UV,visible, or
IR.
4
Wavelength (ïŹ, Greek lambda):
Distance from one wave peak
to the next.
Units: m, cm, m, nm or
Frequency (, Greek nu):
Number of peaks that pass a
given point per second.
Units: Cycles/second or s-1
or
Hertz (Hz)
Wavenumber
Number of waves per cm.
ïŻ
A
λ
υ
1
=
Light waves can be characterized By:
cm-1
Wave nature of light can explain phenomena such as reflection, refraction.
5
 Electromagnetic radiation consists of discrete packets
of
energy, which we call photons.
 Photons are the particles of light or the quanta of light.
 Each photon carries the energy, E (Joule).
where h is the Planck’s constant (=6.626x10-34
J.s)
 The all characteristics of light can be related as follows:
The particle nature can explain phenomena like absorption and
υ
hc
λ
c
h
υ
h
E =
=
=
υ
h
E =
The greater the energy, the higher the frequency and
wavenumber and the shorter the wavelength
6
Regions of electromagnetic radiation
Change
in
nuclear
configuration
Ejection of inner
shell electrons
change
in
the
spin
of
electrons
or
protons
Molecular
processes that
occur when light
is absorbed in
each region
Near
Ultraviole
t
200 nm
200 nm Memorize
Molecular Energy levels
Etotal=Eelec+Evib+Erot
Eelec: electronic energy (UV, X-ray)
Electrons are always in continuous motions & energy is emitted out
because of these motions
.
Evib: vibrational energy (Infrared)
Atoms within molecule are in specific motion so the energy which is emitted
out called vibrational energy
Erot: rotational energy (Microwave)
Electromagnetic radiations which are emitted out or absorbed due to
rotation of molecules along their own axis due to center of gravity is
called rotational energy
.
TECHNIQUE UNDERLYING PRINCIPLE INFORMATION
OBTAINED
UV (200-400 nm)
VIS (400-800 nm)
Quantized absorption of
UV/VIS radiations leading
to electronic excitations
Presence & nature of
unsaturation, particularly
conjugation.
IR (2.5-16 micrometer) Quantized absorption of IR
radiations leading to
vibrational excitations
Presence & environment of
functional group, especially
those containing X-H type
bonds such as C-H, O-H &
N-H or multiple bonds such
as C=C, C=O and C≡N
10
Absorption of light
A molecule that absorbs light photons will end up with increased energy.
The molecule will be promoted to an excited state. Microwave energy
will cause rotation of compounds. IR energy is high enough to promote
bond stretching. UV/Vis energy promotes electrons into higher orbitals.
Short-ïŹ UV and X-rays can ionize molecules or even break bonds.
Most excited molecules relax again to the ground state emitting
the excess energy in the form of heat.
moleculephoto
n
absorbed light is quantized
Principle
11
Electronic transition:
1
2
3
4
12
 When a molecule absorbs light having sufficient energy (e.g. UV-Vis
radiation) to cause an electronic transitions, additional vibration
and rotation transitions also occur
 Molecule can absorb one photon of just the right energy to cause
the following simultaneous changes:
rotational levels
vibrational levels
v2
v1
E0
E1
E = hïź
electronic levels
E
N
E
R
G
Y
Pure electronic
transition
r1
r2
E2
A
ïŹ
ïŹmax
spectrum
Band
Spectrum
v1
v2
Ultraviolet-Visible & IR Spectrophotometry
v0
r1
r2
v0
Eelec >> Evib >> Erot
13
Transmittance and Absorbance
Transmittance, T, is simply defined as “the fraction of light
that reaches a detector after passing through a sample”
The percent transmittance, %T, is simply 100 T
2. Absorbance, defined as:
A=  log T A =  log A =log ( )
ïŻ
P
P
T 
100
x
P
P
T
%
ïŻ

P
PïŻ
ïŹ
106
photons
500 nm
0 < T < 1
0.7x106
photons
0 < %T < 100
T = 0.7, %T = 70%, A = 0.155
ïŻ
P
P
14
Absorbance is directly proportional to:
1. concentration, c, of absorbing species in the sample (Aï€ ïĄ c)
2. path length of light, b, through the sample (Aï€ ïĄ b)
A = bc
For purpose of chemical analysis
The previous equation is the heart of spectrophotometry as applied to
analytical chemistry, it is called Beer-Lambert law or simply Beer’s law
Beer’s law
15
Concentration
A
b
s
o
rb
a
n
c
e
,
A
A=bc
certain ïŹ
constant b
One analyte
Beer’s law is a relation between absorbance and concentration
which is a straight line passes by origin at constant pathlength,
b, and at certain wavelength, ïŹ.
Beer’s law is obeyed for monochromatic light
Slope = b
A spectrophotometer measures either the amount of light reflected
from a sample object or the amount of light that is absorbed by the
sample object.
Types:
UV-visible spectrophotometer
Single beam spectrophotometer
Double beam spectrophotometer(in space instrument & in time
instrument)
IR spectrophotometer
Dispersive IR spectrophotometer (scanning instrument)
Fourier transform-Infrared spectrophotometer (FT-IR)
SPECTROPHOTOMETER
17
1- Sources of light
Sources used in UV-Vis Spectrophotometers are continuous sources.
‱ Continuous sources emit radiation of all wavelengths within
the spectral region for which they are to be used.
‱ Sources of radiation should also be stable and of high intensity.
Continuous Sources
Visible and near IR
radiation
Ultraviolet
radiation
Deuterium Lamp
200-400 nm
Tungsten Lamp
320-2500 nm
Intensity : No. of photons of radiation at a particular point is called
intensity and it is directly proportional to energy.
18
2. Wavelength Selectors
Ideally the output of a wavelength selector would be a radiation of
a single wavelength.
The narrower this bandwidth is , the better performance of the
instrument.
Wavelength
selectors
Filters Monochromators
‱ Filters allows to pass the Narrow Band Width light (20nm – 50 nm) &
NBW also called effective band width.
‱ The simplest kind of filter is absorption filters , the most common of
this type of filters is colored glass filters.
i- Filters
ii- Monochromators
They are used for spectral scanning (varying the wavelength of
radiation over a considerable range ).
They can be used for UV/Vis region.
All monochromators are similar in mechanical construction.
All monochromators employ slits, mirrors, lenses, gratings or
prisms.
19
Reflection grating
1-Grating monochromators
 Polychromatic radiation from
the entrance slit is collimated
(made into beam of parallel
rays) by a concave mirrors
 These rays fall on a reflection
grating, whereupon different
wavelengths are reflected at
different angles.
 The orientation of the
reflection grating directs only
one narrow band wavelengths,
ïŹ2, to the exit slit of the mono-
chromator
 Rotation of the grating allows
different wavelengths, ïŹ1, to
pass through the exit slit
The reflection grating
monochromator
Device consists of entrance
and exit slits, mirrors, and a
grating to disperse the light
20
21
2- Prism monochromators
 Dispersion by prism depends
on refraction of light which
is wavelength dependent
 Violet color with higher
energy (shorter wavelength)
are diffracted or bent most
 While red light with lower
energy (longer wavelength
are diffracted or bent least
 As a result, the poly-
chromatic white light is
dispersed to its individual
colors.
22
Bandwidth Choice The size of the monochromator
exit slit determines the width of
radiation (bandwidth) emitted
from the monochromator.
A wider slit width gives higher
sensitivity because higher
radiation intensity passes to the
sample but on the other hand,
narrow slit width gives better
resolution for the spectrum.
In general, the choice of slit
width to use in an experiment
must be made by compromising
these factors. Still, we can
overcome the problem of low
sensitivity of the small slit by
increasing the sensitivity of the
detector.
What are the advantages and disadvantages of decreasing
monochromator slit width?
23
3- Sample compartment (cells)
 For Visible and UV spectroscopy, a liquid sample is usually
contained in a cell called a cuvette.
 Glass is suitable for visible but not for UV spectroscopy because it
absorbs UV radiation. Quartz can be used in UV as well as in visible
spectroscopy
1 cm 1 cm
Opaque
Face
Transparent
Face
Long pathlength
Short pathlength (b)
1 cm pathlength cuvet
24
4- Detectors
 The detectors are devices that convert radiant energy into electrical
signal.
 A Detector should be sensitive, and has a fast response over a
considerable range of wavelengths.
 In addition, the electrical signal produced by the detector must be
directly proportional to the transmitted intensity (linear response).
hïź
e-
-V
Photosensitive cathode
amplifier
i- Phototube
anode
Phototube emits electrons
from a photosensitive,
negatively charged
cathode when struck by
visible or UV radiation
The electrons flow
through vacuum to an
anode to produce current
which is
proportional to radiation
intensity.
25
ii. Photomultiplier tube
 It is a very sensitive device in which electrons emitted from the
photosensitive cathode strike a second surface called dynode which is
positive with respect to the original cathode.
 Electrons are thus accelerated and can knock out more than one
electrons from the dynode.
 If the above process is repeated several times, so more than 106
electrons are finally collected for each photon striking the first
cathode.
photochathode
anode
high voltage
voltage divider network
dynodes
light
electrons
e-
26
Light source
Grating
Rotating the grating
changes the wavelength
going through the
sample
slits
slits
Sample
Phototube
The components of a single beam
spectrophotometer
When blank is the sample
Po is determined,
otherwise P is measured
Separates white light
into various colors
detects light &
measures intensity
- white light of constant intensity
27
2.Double Beam Spectrophotometer: in it two beams are used.
i. Double Beam Spectrophotometer(in space instrument):
Matched photodetector should be same and both should be present in same
condition
28
ii. Double Beam Spectrophotometer(in time instrument):
By difference of millisecond the light of same intensity pass
first through the reference and then through the sample,both
beams are moved by the millisecond difference so that look
like double beam.
29
Advantages of double beam instruments over single beam
instruments
Single beam spectrophotometer is inconvenient because
1. The sample and blank must be placed alternately in the light path.
2. For measurements at multiple wavelengths, the blank must be run
at each wavelength.
In double beam instruments
1. The absorption in the sample is automatically corrected for the
absorption occurring in the blank.
2. Automatic scanning and continuous recording of spectrum (absorbance
versus wavelength).
30
Applications of Ultraviolet/Visible Molecular
Absorption Spectrophotometry
for identification and estimation of inorganic, organic and
biomedical species.
quantitative analysis.
widely used in chemical and clinical laboratories
throughout the world than any other single method.
Rate of reaction
Analysis of mixture of compounds
Analysis of body fluids
31
Infrared Spectroscopy(vibrational spectroscopy)
The Infrared region is divided into: near, mid and far-infrared.
 Near-infrared refers to the part of the infrared spectrum that is
closest to visible light (10000-400 cm-1
) and
 far-infrared refers to the part that is closer to the microwave
region. (400-10 cm-1
)
 Mid-infrared is the region between these two. For chemical
analysis, we are interested in mid IR region (4000-667 cm-1
).
32
 Radiation in the Mid IR region will cause stretching and bending vibrations of the
bonds in most covalent molecules.
Symmetric stretching
Asymmetric stretching
1- Stretching Vibrations
Modes of Vibration
2- Bending vibrations
A- In-plane bending
Scissoring Rocking
twisting wagging
b- Out-of-plane
bending
Bending
Sym
Asym ïź

ïź

ïź
Detection Electronics
and Computer
Infrared
Source
Determines Frequencies
of Infrared Absorbed and
plots them on a chart
Sample
Simplified Infrared Spectrophotometer
Simplified Infrared Spectrophotometer
NaCl
plates
Absorption
“peaks”
Infrared
Spectrum
frequency
% Transmittance
(decreasing)
focusing
mirror
Instrumentation
Instrumentation
IR spectrophotometer
IR spectrophotometer
34
1. Radiation source
Infrared radiation can be produced by electrically heating
a source, often a Nernst filament or a Globar to 1000-1800 C.
a. Nernst filament is fabricated from oxides of zirconium,
thorium and cerium.
b. The Globar is a small rod of silicon carbide.
IR spectrophotometer (contd.)
IR spectrophotometer (contd.)
35
2. Detector
a. Thermal Detectors : measures IR energy by means of its
thermal effect, the heating effect of IR radiation produces an
electrical signal that can be measured, thermal noise is
always a problem.
b. Pyroelectric detectors : pyroelectric substances are
sandwiched between two electrodes, when IR radiation
reaches the detector , temperature changes producing
current that is proportional to the rate of change of
temperature, they exhibit fast responses so suitable for FT-IR.
36
‱ Types
‱ Dispersion Spectrometers (older technique)
‱ Fourier Transform Infrared (FT-IR) Spectrometers
(Modern technique)
‱ Nearly all IR spectrometers, nowadays, are of the
FT type.
Infrared Instrumentation
Infrared Instrumentation
37
1.Dispersive IR spectrometers
1.Dispersive IR spectrometers
Infrared Dispersion Scanning Instrumentation
‱ Scanning instrument uses a frequency separation device (grating) to
resolve the IR radiation into individual frequencies.
‱ An exit slit isolates a specific frequency for passage to the detector.
‱ The IR spectrum is obtained by moving (scanning) the grating over a
given wavenumber region after passing through the sample.
IR source sample
detector
dispersive
grating
mirror
monochromator
exit slit
38
 Slow Scanning process (time consuming)
Slow Scanning process (time consuming)
 "step-wise" nature of spectral acquisition (Measure one
"step-wise" nature of spectral acquisition (Measure one
frequency at a time-scanning takes about 5 min)
frequency at a time-scanning takes about 5 min)
Disadvantages of Dispersion Infrared
Disadvantages of Dispersion Infrared
Instrumentation
Instrumentation
Noise
Measure
signal
height
 All measurements, especially those we carry
out with instruments, generate Noise.
 Detectors of all sorts generate electrical noise
 Noise limits our ability to even observe very
weak signals or to quantify somewhat weak
signals. The Signal-to-Noise Ratio is an
important parameter is assessing our ability to
interpret data.
 Noise is superimposed on top of peaks
39
 Fourier Transform Infrared (FT-IR) spectrometry was developed
in order to overcome the limitations encountered with dispersive
instruments mainly the slow scanning process.
2.Fourier Transform IR
2.Fourier Transform IR
 A solution was developed which employed a very simple
optical device called an interferometer. The interferometer
produces a unique type of signal which has all of the infrared
frequencies “encoded” into it. The signal can be measured
very quickly, usually on the order of one second or so.
40
FTIR systems
FTIR systems
1. Mechanical operation
‱ Encode (modulate) the spectral information using a
Michelson Interferometer.
2. Mathematical operation
‱ Computer processing of encoded information to
produces the spectrum (Decoding).
Optical Diagram
Optical Diagram
Michelson
Michelson
Interferometer
Interferometer
41
Interferometer
He-Ne gas laser
Fixed mirror
Movable mirror
Sample chamber
Light
source
Detector
DLATGS (deuterated L-
alanine doped triglycene
sulphate)
Beam splitter Interferogram
42
Fourier transform
Fourier transform
(Mathematical Operation)
(Mathematical Operation)
Because the analyst requires a frequency spectrum (a plot of
the intensity at each individual frequency) in order to make
an identification, the measured Interferogram signal can not
be interpreted directly. A means of “decoding” the individual
frequencies is required. This can be accomplished via a well-
known mathematical technique called the Fourier
transformation. This transformation is performed by the
computer which then presents the user with the desired
spectral information for analysis.
43
Time axis
Time domain
decoding
by FFT
Wavenumber
Frequency domain
FT-IR summary
FT-IR summary
44
‱ Speed
‱ Sensitivity is dramatically improved with FT-IR ; detectors are
much more sensitive, the optical throughput is much higher,
higher signal to noise ratio.
‱ Mechanical Simplicity
‱ Internally Calibrated These instruments employ a He-Ne laser
as an internal wavelength calibration standard .These
instruments are self-calibrating and never need to be
calibrated by the user.
FT-IR Advantages
FT-IR Advantages
45
Analytical information obtained using IR techniques
Analytical information obtained using IR techniques
I) Qualitative
a) Structural Elucidation through interpretation of functional group
region ( 4000- 1300 cm-1
) & fingerprint region ( 1300- 910 cm-1
).
b) Compound Identification to find a reference IR spectrum that
matches that of the unknown compound.
II ) Quantitative
The intensity of an absorption band is linearly proportional to
the concentration of analyte of interest at a certain frequency.
46
Applications of Infrared Analysis
Applications of Infrared Analysis
 Analysis of petroleum hydrocarbons , oil and grease content
 Determination of air contaminants.
 Determination of protein, starch, oil , lipids and cellulose in
agricultural products .
Pharmaceutical research.
Forensic investigations.
Polymer analysis.
Quality assurance and control.
Environmental and water quality analysis methods.
Biochemical and biomedical research.
Coatings and surfactants.
47
Textbook: Principles of Instrumental Analysis, Skoog, Holler, Nieman
Textbook: Organic spectroscopy and chromatography by M.Younas
http://www.chemguide.co.uk/analysismenu.html
http://www.wiziq.com/tutorial/91202-QUIZ-Infrared-spectroscopy
Resources and references
48

UV IR Spectroscopy-pathology presentation.ppt

  • 1.
  • 2.
    SPECTROPHOTOMETRY Spectrophotometry is thestudy of the reflection or transmission properties of a substance as a function of wavelength. It is the quantitative study of electromagnetic spectra of a material . 2 Spectrophotometer
  • 3.
    Spectroscopy is anyprocedure that uses the interaction of Electromagnetic Radiation (EMR) with matter to identify and/or to estimate an analyte. 3 Qualitative Analysis Quantitative Analysis Electromagnetic radiation (light) molecules solid ions liquid atoms gas Mixtures solutions  EMR can be described in terms of both particles and waves (Dual nature of light)  Light waves consist of perpendicular and oscillating electric and magnetic fields Spectophotometry is historically just spectrometry where the light is UV,visible, or IR.
  • 4.
    4 Wavelength (ïŹ, Greeklambda): Distance from one wave peak to the next. Units: m, cm, m, nm or Frequency (, Greek nu): Number of peaks that pass a given point per second. Units: Cycles/second or s-1 or Hertz (Hz) Wavenumber Number of waves per cm. ïŻ A λ υ 1 = Light waves can be characterized By: cm-1 Wave nature of light can explain phenomena such as reflection, refraction.
  • 5.
    5  Electromagnetic radiationconsists of discrete packets of energy, which we call photons.  Photons are the particles of light or the quanta of light.  Each photon carries the energy, E (Joule). where h is the Planck’s constant (=6.626x10-34 J.s)  The all characteristics of light can be related as follows: The particle nature can explain phenomena like absorption and υ hc λ c h υ h E = = = υ h E = The greater the energy, the higher the frequency and wavenumber and the shorter the wavelength
  • 6.
  • 7.
    Regions of electromagneticradiation Change in nuclear configuration Ejection of inner shell electrons change in the spin of electrons or protons Molecular processes that occur when light is absorbed in each region Near Ultraviole t 200 nm 200 nm Memorize
  • 8.
    Molecular Energy levels Etotal=Eelec+Evib+Erot Eelec:electronic energy (UV, X-ray) Electrons are always in continuous motions & energy is emitted out because of these motions . Evib: vibrational energy (Infrared) Atoms within molecule are in specific motion so the energy which is emitted out called vibrational energy Erot: rotational energy (Microwave) Electromagnetic radiations which are emitted out or absorbed due to rotation of molecules along their own axis due to center of gravity is called rotational energy .
  • 9.
    TECHNIQUE UNDERLYING PRINCIPLEINFORMATION OBTAINED UV (200-400 nm) VIS (400-800 nm) Quantized absorption of UV/VIS radiations leading to electronic excitations Presence & nature of unsaturation, particularly conjugation. IR (2.5-16 micrometer) Quantized absorption of IR radiations leading to vibrational excitations Presence & environment of functional group, especially those containing X-H type bonds such as C-H, O-H & N-H or multiple bonds such as C=C, C=O and C≡N
  • 10.
    10 Absorption of light Amolecule that absorbs light photons will end up with increased energy. The molecule will be promoted to an excited state. Microwave energy will cause rotation of compounds. IR energy is high enough to promote bond stretching. UV/Vis energy promotes electrons into higher orbitals. Short-ïŹ UV and X-rays can ionize molecules or even break bonds. Most excited molecules relax again to the ground state emitting the excess energy in the form of heat. moleculephoto n absorbed light is quantized Principle
  • 11.
  • 12.
    12  When amolecule absorbs light having sufficient energy (e.g. UV-Vis radiation) to cause an electronic transitions, additional vibration and rotation transitions also occur  Molecule can absorb one photon of just the right energy to cause the following simultaneous changes: rotational levels vibrational levels v2 v1 E0 E1 E = hïź electronic levels E N E R G Y Pure electronic transition r1 r2 E2 A ïŹ ïŹmax spectrum Band Spectrum v1 v2 Ultraviolet-Visible & IR Spectrophotometry v0 r1 r2 v0 Eelec >> Evib >> Erot
  • 13.
    13 Transmittance and Absorbance Transmittance,T, is simply defined as “the fraction of light that reaches a detector after passing through a sample” The percent transmittance, %T, is simply 100 T 2. Absorbance, defined as: A=  log T A =  log A =log ( ) ïŻ P P T  100 x P P T % ïŻ  P PïŻ ïŹ 106 photons 500 nm 0 < T < 1 0.7x106 photons 0 < %T < 100 T = 0.7, %T = 70%, A = 0.155 ïŻ P P
  • 14.
    14 Absorbance is directlyproportional to: 1. concentration, c, of absorbing species in the sample (Aï€ ïĄ c) 2. path length of light, b, through the sample (Aï€ ïĄ b) A = bc For purpose of chemical analysis The previous equation is the heart of spectrophotometry as applied to analytical chemistry, it is called Beer-Lambert law or simply Beer’s law Beer’s law
  • 15.
    15 Concentration A b s o rb a n c e , A A=bc certain ïŹ constant b Oneanalyte Beer’s law is a relation between absorbance and concentration which is a straight line passes by origin at constant pathlength, b, and at certain wavelength, ïŹ. Beer’s law is obeyed for monochromatic light Slope = b
  • 16.
    A spectrophotometer measureseither the amount of light reflected from a sample object or the amount of light that is absorbed by the sample object. Types: UV-visible spectrophotometer Single beam spectrophotometer Double beam spectrophotometer(in space instrument & in time instrument) IR spectrophotometer Dispersive IR spectrophotometer (scanning instrument) Fourier transform-Infrared spectrophotometer (FT-IR) SPECTROPHOTOMETER
  • 17.
    17 1- Sources oflight Sources used in UV-Vis Spectrophotometers are continuous sources. ‱ Continuous sources emit radiation of all wavelengths within the spectral region for which they are to be used. ‱ Sources of radiation should also be stable and of high intensity. Continuous Sources Visible and near IR radiation Ultraviolet radiation Deuterium Lamp 200-400 nm Tungsten Lamp 320-2500 nm Intensity : No. of photons of radiation at a particular point is called intensity and it is directly proportional to energy.
  • 18.
    18 2. Wavelength Selectors Ideallythe output of a wavelength selector would be a radiation of a single wavelength. The narrower this bandwidth is , the better performance of the instrument. Wavelength selectors Filters Monochromators ‱ Filters allows to pass the Narrow Band Width light (20nm – 50 nm) & NBW also called effective band width. ‱ The simplest kind of filter is absorption filters , the most common of this type of filters is colored glass filters. i- Filters
  • 19.
    ii- Monochromators They areused for spectral scanning (varying the wavelength of radiation over a considerable range ). They can be used for UV/Vis region. All monochromators are similar in mechanical construction. All monochromators employ slits, mirrors, lenses, gratings or prisms. 19
  • 20.
    Reflection grating 1-Grating monochromators Polychromatic radiation from the entrance slit is collimated (made into beam of parallel rays) by a concave mirrors  These rays fall on a reflection grating, whereupon different wavelengths are reflected at different angles.  The orientation of the reflection grating directs only one narrow band wavelengths, ïŹ2, to the exit slit of the mono- chromator  Rotation of the grating allows different wavelengths, ïŹ1, to pass through the exit slit The reflection grating monochromator Device consists of entrance and exit slits, mirrors, and a grating to disperse the light 20
  • 21.
    21 2- Prism monochromators Dispersion by prism depends on refraction of light which is wavelength dependent  Violet color with higher energy (shorter wavelength) are diffracted or bent most  While red light with lower energy (longer wavelength are diffracted or bent least  As a result, the poly- chromatic white light is dispersed to its individual colors.
  • 22.
    22 Bandwidth Choice Thesize of the monochromator exit slit determines the width of radiation (bandwidth) emitted from the monochromator. A wider slit width gives higher sensitivity because higher radiation intensity passes to the sample but on the other hand, narrow slit width gives better resolution for the spectrum. In general, the choice of slit width to use in an experiment must be made by compromising these factors. Still, we can overcome the problem of low sensitivity of the small slit by increasing the sensitivity of the detector. What are the advantages and disadvantages of decreasing monochromator slit width?
  • 23.
    23 3- Sample compartment(cells)  For Visible and UV spectroscopy, a liquid sample is usually contained in a cell called a cuvette.  Glass is suitable for visible but not for UV spectroscopy because it absorbs UV radiation. Quartz can be used in UV as well as in visible spectroscopy 1 cm 1 cm Opaque Face Transparent Face Long pathlength Short pathlength (b) 1 cm pathlength cuvet
  • 24.
    24 4- Detectors  Thedetectors are devices that convert radiant energy into electrical signal.  A Detector should be sensitive, and has a fast response over a considerable range of wavelengths.  In addition, the electrical signal produced by the detector must be directly proportional to the transmitted intensity (linear response). hïź e- -V Photosensitive cathode amplifier i- Phototube anode Phototube emits electrons from a photosensitive, negatively charged cathode when struck by visible or UV radiation The electrons flow through vacuum to an anode to produce current which is proportional to radiation intensity.
  • 25.
    25 ii. Photomultiplier tube It is a very sensitive device in which electrons emitted from the photosensitive cathode strike a second surface called dynode which is positive with respect to the original cathode.  Electrons are thus accelerated and can knock out more than one electrons from the dynode.  If the above process is repeated several times, so more than 106 electrons are finally collected for each photon striking the first cathode. photochathode anode high voltage voltage divider network dynodes light electrons e-
  • 26.
    26 Light source Grating Rotating thegrating changes the wavelength going through the sample slits slits Sample Phototube The components of a single beam spectrophotometer When blank is the sample Po is determined, otherwise P is measured Separates white light into various colors detects light & measures intensity - white light of constant intensity
  • 27.
    27 2.Double Beam Spectrophotometer:in it two beams are used. i. Double Beam Spectrophotometer(in space instrument): Matched photodetector should be same and both should be present in same condition
  • 28.
    28 ii. Double BeamSpectrophotometer(in time instrument): By difference of millisecond the light of same intensity pass first through the reference and then through the sample,both beams are moved by the millisecond difference so that look like double beam.
  • 29.
    29 Advantages of doublebeam instruments over single beam instruments Single beam spectrophotometer is inconvenient because 1. The sample and blank must be placed alternately in the light path. 2. For measurements at multiple wavelengths, the blank must be run at each wavelength. In double beam instruments 1. The absorption in the sample is automatically corrected for the absorption occurring in the blank. 2. Automatic scanning and continuous recording of spectrum (absorbance versus wavelength).
  • 30.
    30 Applications of Ultraviolet/VisibleMolecular Absorption Spectrophotometry for identification and estimation of inorganic, organic and biomedical species. quantitative analysis. widely used in chemical and clinical laboratories throughout the world than any other single method. Rate of reaction Analysis of mixture of compounds Analysis of body fluids
  • 31.
    31 Infrared Spectroscopy(vibrational spectroscopy) TheInfrared region is divided into: near, mid and far-infrared.  Near-infrared refers to the part of the infrared spectrum that is closest to visible light (10000-400 cm-1 ) and  far-infrared refers to the part that is closer to the microwave region. (400-10 cm-1 )  Mid-infrared is the region between these two. For chemical analysis, we are interested in mid IR region (4000-667 cm-1 ).
  • 32.
    32  Radiation inthe Mid IR region will cause stretching and bending vibrations of the bonds in most covalent molecules. Symmetric stretching Asymmetric stretching 1- Stretching Vibrations Modes of Vibration 2- Bending vibrations A- In-plane bending Scissoring Rocking twisting wagging b- Out-of-plane bending Bending Sym Asym ïź  ïź  ïź
  • 33.
    Detection Electronics and Computer Infrared Source DeterminesFrequencies of Infrared Absorbed and plots them on a chart Sample Simplified Infrared Spectrophotometer Simplified Infrared Spectrophotometer NaCl plates Absorption “peaks” Infrared Spectrum frequency % Transmittance (decreasing) focusing mirror Instrumentation Instrumentation
  • 34.
    IR spectrophotometer IR spectrophotometer 34 1.Radiation source Infrared radiation can be produced by electrically heating a source, often a Nernst filament or a Globar to 1000-1800 C. a. Nernst filament is fabricated from oxides of zirconium, thorium and cerium. b. The Globar is a small rod of silicon carbide.
  • 35.
    IR spectrophotometer (contd.) IRspectrophotometer (contd.) 35 2. Detector a. Thermal Detectors : measures IR energy by means of its thermal effect, the heating effect of IR radiation produces an electrical signal that can be measured, thermal noise is always a problem. b. Pyroelectric detectors : pyroelectric substances are sandwiched between two electrodes, when IR radiation reaches the detector , temperature changes producing current that is proportional to the rate of change of temperature, they exhibit fast responses so suitable for FT-IR.
  • 36.
    36 ‱ Types ‱ DispersionSpectrometers (older technique) ‱ Fourier Transform Infrared (FT-IR) Spectrometers (Modern technique) ‱ Nearly all IR spectrometers, nowadays, are of the FT type. Infrared Instrumentation Infrared Instrumentation
  • 37.
    37 1.Dispersive IR spectrometers 1.DispersiveIR spectrometers Infrared Dispersion Scanning Instrumentation ‱ Scanning instrument uses a frequency separation device (grating) to resolve the IR radiation into individual frequencies. ‱ An exit slit isolates a specific frequency for passage to the detector. ‱ The IR spectrum is obtained by moving (scanning) the grating over a given wavenumber region after passing through the sample. IR source sample detector dispersive grating mirror monochromator exit slit
  • 38.
    38  Slow Scanningprocess (time consuming) Slow Scanning process (time consuming)  "step-wise" nature of spectral acquisition (Measure one "step-wise" nature of spectral acquisition (Measure one frequency at a time-scanning takes about 5 min) frequency at a time-scanning takes about 5 min) Disadvantages of Dispersion Infrared Disadvantages of Dispersion Infrared Instrumentation Instrumentation Noise Measure signal height  All measurements, especially those we carry out with instruments, generate Noise.  Detectors of all sorts generate electrical noise  Noise limits our ability to even observe very weak signals or to quantify somewhat weak signals. The Signal-to-Noise Ratio is an important parameter is assessing our ability to interpret data.  Noise is superimposed on top of peaks
  • 39.
    39  Fourier TransformInfrared (FT-IR) spectrometry was developed in order to overcome the limitations encountered with dispersive instruments mainly the slow scanning process. 2.Fourier Transform IR 2.Fourier Transform IR  A solution was developed which employed a very simple optical device called an interferometer. The interferometer produces a unique type of signal which has all of the infrared frequencies “encoded” into it. The signal can be measured very quickly, usually on the order of one second or so.
  • 40.
    40 FTIR systems FTIR systems 1.Mechanical operation ‱ Encode (modulate) the spectral information using a Michelson Interferometer. 2. Mathematical operation ‱ Computer processing of encoded information to produces the spectrum (Decoding).
  • 41.
    Optical Diagram Optical Diagram Michelson Michelson Interferometer Interferometer 41 Interferometer He-Negas laser Fixed mirror Movable mirror Sample chamber Light source Detector DLATGS (deuterated L- alanine doped triglycene sulphate) Beam splitter Interferogram
  • 42.
    42 Fourier transform Fourier transform (MathematicalOperation) (Mathematical Operation) Because the analyst requires a frequency spectrum (a plot of the intensity at each individual frequency) in order to make an identification, the measured Interferogram signal can not be interpreted directly. A means of “decoding” the individual frequencies is required. This can be accomplished via a well- known mathematical technique called the Fourier transformation. This transformation is performed by the computer which then presents the user with the desired spectral information for analysis.
  • 43.
    43 Time axis Time domain decoding byFFT Wavenumber Frequency domain FT-IR summary FT-IR summary
  • 44.
    44 ‱ Speed ‱ Sensitivityis dramatically improved with FT-IR ; detectors are much more sensitive, the optical throughput is much higher, higher signal to noise ratio. ‱ Mechanical Simplicity ‱ Internally Calibrated These instruments employ a He-Ne laser as an internal wavelength calibration standard .These instruments are self-calibrating and never need to be calibrated by the user. FT-IR Advantages FT-IR Advantages
  • 45.
    45 Analytical information obtainedusing IR techniques Analytical information obtained using IR techniques I) Qualitative a) Structural Elucidation through interpretation of functional group region ( 4000- 1300 cm-1 ) & fingerprint region ( 1300- 910 cm-1 ). b) Compound Identification to find a reference IR spectrum that matches that of the unknown compound. II ) Quantitative The intensity of an absorption band is linearly proportional to the concentration of analyte of interest at a certain frequency.
  • 46.
    46 Applications of InfraredAnalysis Applications of Infrared Analysis  Analysis of petroleum hydrocarbons , oil and grease content  Determination of air contaminants.  Determination of protein, starch, oil , lipids and cellulose in agricultural products . Pharmaceutical research. Forensic investigations. Polymer analysis. Quality assurance and control. Environmental and water quality analysis methods. Biochemical and biomedical research. Coatings and surfactants.
  • 47.
    47 Textbook: Principles ofInstrumental Analysis, Skoog, Holler, Nieman Textbook: Organic spectroscopy and chromatography by M.Younas http://www.chemguide.co.uk/analysismenu.html http://www.wiziq.com/tutorial/91202-QUIZ-Infrared-spectroscopy Resources and references
  • 48.

Editor's Notes

  • #15  Log 10 X = Y ------ X = 10Y Log 1000 = 3 ------ 1000 = 103
  • #41 Principles of FTIR Structure of an Interferometer Fourier spectroscopy used in FT-IR is the general term for the use of a two-beam interferometer (primarily Michelson interferometers) in spectroscopy. A Michelson interferometer consists of a half-mirror (beam splitter) and two reflecting mirrors. One of the reflecting mirrors is fixed in place (fixed mirror) and the other has a mechanism for moving parallel to the optical axis (movable mirror). Light from the light source is collimated and directed into the interferometer, striking the beam splitter at an angle, thereby separating the light into transmitted light and reflected light. These two beams of light are each reflected by the fixed mirror and movable mirror, and then returned to the beam splitter where they are recombined into a single beam.
  • #46 1- Freon (1,1,2-trichloro-1,2,2-trifluoroethane ) contains no C-H bonds, and thus does not absorb IR radiation in the aforementioned 3100 to 2700 cm–1 where HC, oil and grease absorb. 2- compared to standard sample of air with known contaminants. 3- reflectance mode, each reflected band is characteristic for one of the analytes, the reflectance value is proportional to the conc.