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SPECTROFLOURIMETRY
Modern Pharmaceutical Analytical Techniques
1
CONTENTS
οƒ˜ Introduction
οƒ˜ Definition
οƒ˜ Theory
οƒ˜ Factors affecting fluorescence
οƒ˜ Instrumentation
οƒ˜ Application
οƒ˜ Conclusion
οƒ˜ Reference
2
INTRODUCTION
οƒ˜ Absorption of UV-VIS radiation causes transition of
electrons from ground state to excited state.
οƒ˜ As excited state is not stable so, excess energy is released
by
οƒΌ Collisional deactivation
οƒΌ photoluminescence
οƒ˜ This study or measurement of this emitted radiation is the
principle of Flourimetry.
οƒ˜ Phosphorescence is also related phenomena, which is
study of emitted radiation when electron undergoes
transition from triplet state to singlet ground state .
3
DEFINITION
οƒ˜ Singlet ground state: a state in which all the electrons in a
molecule are paired (↑↓)
οƒ˜ Doublet state: a state in which an unpaired electron is
present e.g., free radical ↑ or ↓
οƒ˜ Triplet state: a state in which unpaired electrons of same
spin present ↑ ↑ (unpaired and same spin)
οƒ˜ Singlet excited state: a state in which electrons are
unpaired but of opposite spin like ↑ ↓ (unpaired and
opposite )
4
οƒ˜ Collisional deactivation: in which entire energy is lost due
to collisional deactivation and no radiation is emitted.
οƒ˜ Fluorescence: a part of energy is lost due to vibrational
transitions and remaining energy is emitted as UV-VIS
radiation of longer wavelength.
οƒ˜ Fluorescence is the phenomena of emission of radiation
when the is transition from single excited state to singlet
ground state.
οƒ˜ The wavelength of absorbed radiation is called excitation
wavelength.
οƒ˜ The wavelength of emitted radiation is called emission
wavelength.
5
οƒ˜ Phosphorescence: at favourable conditions like low temp.
and absence of oxygen there is transition from excited
singlet state to triplet state which is called as inter
system crossing. The emission of radiation when electrons
undergoes transition from triplet state to singlet ground
state is called as phosphorescence .
6
Fig:- Phenomena of fluorescence and phosphorescence.
7
THEORY
οƒ˜ Both fluorescence and phosphorescence are types of
photoluminescence (luminescence)
οƒ˜ Luminescence is described by using a molecular-energy
interpretation.
οƒ˜ Fluorescence of organic molecules means emission of radiant
energy during a transition from the lowest excited singlet state
𝑆1 to the singlet ground state 𝑆0 .
οƒ˜ Phosphorescence of organic molecules means emission of
radiant energy during a transition from the lowest excited
triplet state 𝑇1 to the singlet ground state 𝑆0 .
8
 In phosphorescence, an intersystem crossing can take
place readily from 𝑆1 to one of the vibrational levels of 𝑇1
state that has very nearly the same energy level (process
III). This is followed by non radiative decay (process IV) to
the 𝑇1 level.
9
Fig; Partial energy diagram for a photo luminescent system
10
οƒ˜ Intersystem crossing process involves a change in the spin of
the excited electron and thus a change in spin multiplicity.
οƒ˜ The triplet state 𝑇1 is metastable, and molecules populating
it have excess energy. This energy can be lost by
οƒΌ Phosphorescence (process V)
οƒΌ Oxygen quenching:
οƒΌ By collision
11
Differences between fluorescence and
phosphorescence
οƒ˜ Phosphorescence may sometimes persist for many seconds after
the excitation source is removed.
οƒ˜ Fluorescence emission is always at shorter wavelength than that
of phosphorescence.
οƒ˜ Fluorescence is usually observed at room temperature in liquid
solution, while phosphorescence is observed in rigid medium at
very low temperature.
οƒ˜ Fluorescence life time is usually in the range 10-7-10-9 sec, while
phosphorescence lifetime is usually in the range 10-4 -10 sec.
12
οƒ˜ Half life time: It is the time required for half of the
molecules to emit photons and thus return to the ground
states.
οƒ˜ Effect of molecular structure on luminescence properties
13
Fluorescence may be expected
generally in;
οƒΌ Aromatic molecules that contain conjugated double
bonds
οƒΌ Polycyclic aromatic compounds (with great number of Ο€
electrons)
οƒΌ Substituents strongly affect on the fluorescence;
substituents such as NH2, NHCH3, N(CH3)2, OH and OCH3
groups enhance the fluorescence, while electron with
drawing group such as NO2 Cl-, Br-, I- and COOH groups
decrease the fluorescence
οƒΌ Formation of metal chelates promotes the fluorescence.
14
Phosphorescence may be expected
generally in
οƒΌ Aromatic hydrocarbons
οƒΌ Introduction of substituents such as NH2, SH, OH to
aromatic hydrocarbon enhance the phosphorescence
and also aromatic nitro compounds
οƒΌ Majority of aromatic aldehydes and ketones show
phosphorescence.
15
Fluorescence Spectra
Instruments that measure the intensity of fluorescence are called
fluorimeter. Those that measure the fluorescence intensity at
variable wavelengths of excitation and emission, and are able to
produce fluorescence spectra are called spectrofluorimeters
In the recording the fluorescence spectra, the limitations of light
sources and measuring devices assume real significance. These
limitations are:
οƒΌ Variation of the intensity of available energy with Ξ».
οƒΌ Variation in the response of the detector to light of
different wavelengths
16
.
Excitation Spectra:
Before a compound can fluoresce, energy must be observed, and
with an ideal light source, of constant intensity at different
wavelengths, the most intense fluorescence is produced by
radiation corresponding in wavelength to that of the absorption
peak of the substance. Therefore, if the intensity of the
fluorescence is plotted as a function of the wavelength of the
radiation used to excite the fluorescence, an activation or
excitation spectrum will, result. This will be identical to the
absorption spectrum when corrected for instrumental effect,
because the fluorescence efficiency is greatly independent of Ξ» .
17
Fig; Fluorescence excitation and emission spectra for a solution of
quinine
18
Emission Spectra (Fluorescence)
When a monochromator source of constant light intensity is
used to irradiate a sample, the fluorescence may be
analysed in a monochromator at constant slit width to give
apparent emission spectrum.
The true spectrum is obtained by applying a correction for
change in detector sensitivity with wavelength and for
changes due to fluorescence monochromator i.e., half band
width of emergent light and light losses.
Fluorescence emission spectra arise because of transition
from the first excited state and their shapes are therefore
independent of the light used to excite fluorescence.
19
FACTORS AFFECTING FLUORESCENCE
INTENSITY;
οƒ˜ Concentration
οƒ˜ Quantam yield
οƒ˜ Intensity of incident light I0
οƒ˜ Pathlength (b)
οƒ˜ Adsorption
οƒ˜ Oxygen
οƒ˜ pH
οƒ˜ Temperature and viscosity
οƒ˜ Scatter
20
Concentration:
The fluorescence intensity of a substance is proportional to
concentration only when the absorbance in a 1 cm cell is less than
0.02.
If the concentration of the fluorescent substance is so great that all
incident radiation is absorbed, the equation will be:
F = I0
Ο•
That is the fluorescence is independent of concentration, and
proportional to the intensity of incident radiation only, a property that
may be utilized to determine the approximate emission characteristics
of a light source
21
Diagrammatic representation of the variation of fluorescence intensity
with concentration.
Region (a): Proportional relationship
Region (b): Negative deviation from linearity.
Region (c): Fluorescence independent of concentration
Region (d): Reabsorption of fluorescence 22
Quantum yield of fluorescence (Ο•)
This is the ratio:
Ο• =
π‘›π‘œ.π‘œπ‘“ π‘β„Žπ‘œπ‘‘π‘œπ‘›π‘  π‘’π‘šπ‘–π‘‘π‘‘π‘’π‘‘
π‘›π‘œ.π‘œπ‘“ π‘β„Žπ‘œπ‘‘π‘œπ‘›π‘  π‘Žπ‘π‘ π‘œπ‘Ÿπ‘π‘’π‘‘
Since some absorbed energy is lost by radiation less pathways,
the quantum efficiency is less than 1.
Highly fluorescent substances take Ο• value near 1, which
shows that most of the absorbed energy is re-emitted as
fluorescence.
For e.g.; fluorescein in 0.1 M NaOH and quinine in 0.05 M
H2SO4 have, Ο• values of 0.85 and 0.54 respectively at 23Β°C.
Non-fluorescent substances have Ο• = 0.
23
Intensity of incident light 𝐈 𝟎
:
An increase in the intensity of light incident on the sample
produces a proportional increase in the fluorescence
intensity. The intensity of incident light depends on the
intensity of light emitted from the lamp.
24
Pathlength (b)
The effective pathlength viewed by the detector depends on
both the excitation and emission slit widths.
25
Adsorption:
The extreme sensitivity of the method requires very dilute
solution, 10-100 times, weaker than those employed in absorption
spectrophotometry.
Adsorption of the fluorescent substance on the container walls
may therefore presents serious problems and strong stock solutions
must be kept and diluted as required. Quinine is a typical example
of a substance which is adsorbed onto cell walls.
26
Oxygen
The presence of oxygen may interfere in two ways:
οƒΌ By direct oxidation of the fluorescent substance to non-
fluorescent products.
οƒΌ By quenching of fluorescence.
27
pH
 It is to be expected that alteration of the pH of a solution will
have a significant effect on fluorescence if the absorption
spectrum of the solute is changed.
28
Temperature and viscosity
Variation in temperature and viscosity will cause variations
in the frequency of collision between molecules. Thus, an
increase in the temperature or the decrease in the viscosity
is likely to decrease the fluorescence by deactivation of the
excited molecules by collision.
29
Quenchers
Quenching is the reduction of the fluorescence intensity by
the presence of substances in the sample other than the
fluorescent analyte.
οƒΌ Static Quenchers:
Form a chemical complex with the fluorescent substance
and alter its fluorescence characteristics. Certain xanthine
derivatives e.g. caffeine, reduce the fluorescence of
riboflavin by static quenching.
30
Scatter
The excitation and emission monochromators are at the
same wavelengths, scattered light of the same wavelength
as the incident light will be detected by the photomultiplier
arising from colloidal particles in the sample (Tyndall
scatter) and from the molecules (Rayleigh scatter)
31
.
Raman Scatter:
Arises from the conversion of some of the incident radiation
into vibrational and rotational energy by the solvent
molecules. The resultant scattered light is of lower energy
and, consequently of longer wavelength.
32
INSTRUMENTATION
When both the excitation and emission spectra are to be
recorded, two monochromator are essential, one for the light source
(excitation monochromator) and one for the fluorescence (emission
monochromator). The light source must provided a high level of UV
and Visible radiation and a compact high pressure Zenon arc lamp is
used.
The production of ozone by the photochemical conversion of
atmospheric oxygen in the lamp compartment presents a toxic
hazard unless the ozone is thermally decomposed or removed by
adsorption onto charcoal. As many experiments will almost certainly
entail the measurement of very weak fluorescence. The detector
must be a highly sensitive photomultiplier tube of low dark current.
If the main interest lies in the fluorescence emission spectra, one
monochromator may be dispensed with a suitable light source33
and filter used instead. The rather poor luminosity
associated with the monochromator even with a xenon arc
lamp is replaced by the much more intense light from a
source such as a mercury vapour lamp, from which a suitable
activation beam is isolated by means of the filter. This
arrangement partially overcome, one of the difficulties
inherent in spectrofluorimetry, i.e., that so much of the
available light is lost.
34
Fig; simple fluorometer 35
ADVANTAGES OF SPECTROFLUORIMETRY
οƒ˜ High sensitivity
οƒ˜ Selectivity
οƒ˜ Quantitative Aspects
36
Quantitative Aspects:
Many of the quantitative aspects of spectrofluorimetry may be
understood by reference to the fundamental equation for the
intensity of the fluorescence emitted. This equation may be
derived from that of the
Beer-Lambert law:
A = Log 𝑰 𝟎/𝑰 𝒕 = abC
Or 𝑰 𝟎/𝑰 𝒕 = 𝟏𝟎 𝒂𝒃𝒄
∴ 𝑰 𝒕= 𝑰 𝟎 x πŸπŸŽβˆ’π’‚π’ƒπ’„
37
but fluorescence (F) = (𝑰 𝟎- 𝑰 𝒕)Ο•
where Ο• is the quantum yield of the fluorescence
At very low absorbance (< 0.02), the equation will be
F= 2.3 𝑰 𝟎 abC Ο•
For a fixed set of instrumental (𝐼0 and b) and sample (a
andΟ•) parameters, the fluorescence is proportional to the
concentration.
F= K C where K = 2.3 𝑰 𝟎 a b Ο•
38
APPLICATIONS OF SPECTROFLUORIMETRY
οƒ˜ Compounds which are fluorescent are readily determined with
simple instruments as the solution for examination is normally
obtained by dissolution of the sample in a suitable solvent
(table 1)
39
οƒ˜ Single substances which are in themselves, non-
fluorescent may be determined as a result of chemical
change.
e.g.;
Determination of primary amines, amino acids, peptides
etc. through:
40
Reaction with fluorescamine reagent
41
οƒ˜ Determination of primary and secondary aliphatic amines
through:
a- reaction with 4-chloro-7-nitrobenzo-2-oxa-l,3-diazole (
NBD-CI ) give yellow fluorescence
42
b- reaction with l-dimethylaminonaphthalene-5-sulphonyl
chloride (Dansyl, chloride)
43
Thiamine HCI in pharmaceutical preparations such as tablets
and elixirs and in food stuffs such as flour is relatively easily
determined by oxidation to highly fluorescent thiochrome.
The product is soluble in 2-methyl-propan-1-ol and hence is
easily extracted from the reaction mixture for
measurements
44
For mixture of two components, it may be possible to select
the exciting radiation of appropriate wavelengths, such that
only one compound fluoresces at any time. Even if there is
not possible, measurements of the fluorescence at two
wavelengths may be sufficient to determine the composition
of the mixture.
45
CONCLUSION
οƒ˜ Fluorescence is most sensitive analytical techniques.
οƒ˜ Detection studies will increase the development of
fluorescence field.
οƒ˜ Flurometric method are much useful in qualitative
analysis as compared to quantitative analysis.
46
REFERENCES
1. Douglas a, Skoog , Holler, PRINCIPLE OF INSTRUMENTAL
ANALYSIS, 5th edition , Saunders college, west Washington
square, Philidhepia
2. Dr Ravishankar , A TEXTBOOK OF PHARAMACEUTICAL
ANALYSIS, 3rd edition, Rx pub., 57, west car street,
Tiruneveli-627006
3. Gr Chatwal , S.K. Anand, INSTRUMENTAL METHOD OF
CHEMICAL ANALYSIS, Himalaya pub. house pvt ltd, Ramdoot',
Dr. Bhaleraomarg, girgaon, Mumbai - 400 004, Maharashtra,
India
47
THANK YOU
48

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Spectroflourimetry

  • 2. CONTENTS οƒ˜ Introduction οƒ˜ Definition οƒ˜ Theory οƒ˜ Factors affecting fluorescence οƒ˜ Instrumentation οƒ˜ Application οƒ˜ Conclusion οƒ˜ Reference 2
  • 3. INTRODUCTION οƒ˜ Absorption of UV-VIS radiation causes transition of electrons from ground state to excited state. οƒ˜ As excited state is not stable so, excess energy is released by οƒΌ Collisional deactivation οƒΌ photoluminescence οƒ˜ This study or measurement of this emitted radiation is the principle of Flourimetry. οƒ˜ Phosphorescence is also related phenomena, which is study of emitted radiation when electron undergoes transition from triplet state to singlet ground state . 3
  • 4. DEFINITION οƒ˜ Singlet ground state: a state in which all the electrons in a molecule are paired (↑↓) οƒ˜ Doublet state: a state in which an unpaired electron is present e.g., free radical ↑ or ↓ οƒ˜ Triplet state: a state in which unpaired electrons of same spin present ↑ ↑ (unpaired and same spin) οƒ˜ Singlet excited state: a state in which electrons are unpaired but of opposite spin like ↑ ↓ (unpaired and opposite ) 4
  • 5. οƒ˜ Collisional deactivation: in which entire energy is lost due to collisional deactivation and no radiation is emitted. οƒ˜ Fluorescence: a part of energy is lost due to vibrational transitions and remaining energy is emitted as UV-VIS radiation of longer wavelength. οƒ˜ Fluorescence is the phenomena of emission of radiation when the is transition from single excited state to singlet ground state. οƒ˜ The wavelength of absorbed radiation is called excitation wavelength. οƒ˜ The wavelength of emitted radiation is called emission wavelength. 5
  • 6. οƒ˜ Phosphorescence: at favourable conditions like low temp. and absence of oxygen there is transition from excited singlet state to triplet state which is called as inter system crossing. The emission of radiation when electrons undergoes transition from triplet state to singlet ground state is called as phosphorescence . 6
  • 7. Fig:- Phenomena of fluorescence and phosphorescence. 7
  • 8. THEORY οƒ˜ Both fluorescence and phosphorescence are types of photoluminescence (luminescence) οƒ˜ Luminescence is described by using a molecular-energy interpretation. οƒ˜ Fluorescence of organic molecules means emission of radiant energy during a transition from the lowest excited singlet state 𝑆1 to the singlet ground state 𝑆0 . οƒ˜ Phosphorescence of organic molecules means emission of radiant energy during a transition from the lowest excited triplet state 𝑇1 to the singlet ground state 𝑆0 . 8
  • 9.  In phosphorescence, an intersystem crossing can take place readily from 𝑆1 to one of the vibrational levels of 𝑇1 state that has very nearly the same energy level (process III). This is followed by non radiative decay (process IV) to the 𝑇1 level. 9
  • 10. Fig; Partial energy diagram for a photo luminescent system 10
  • 11. οƒ˜ Intersystem crossing process involves a change in the spin of the excited electron and thus a change in spin multiplicity. οƒ˜ The triplet state 𝑇1 is metastable, and molecules populating it have excess energy. This energy can be lost by οƒΌ Phosphorescence (process V) οƒΌ Oxygen quenching: οƒΌ By collision 11
  • 12. Differences between fluorescence and phosphorescence οƒ˜ Phosphorescence may sometimes persist for many seconds after the excitation source is removed. οƒ˜ Fluorescence emission is always at shorter wavelength than that of phosphorescence. οƒ˜ Fluorescence is usually observed at room temperature in liquid solution, while phosphorescence is observed in rigid medium at very low temperature. οƒ˜ Fluorescence life time is usually in the range 10-7-10-9 sec, while phosphorescence lifetime is usually in the range 10-4 -10 sec. 12
  • 13. οƒ˜ Half life time: It is the time required for half of the molecules to emit photons and thus return to the ground states. οƒ˜ Effect of molecular structure on luminescence properties 13
  • 14. Fluorescence may be expected generally in; οƒΌ Aromatic molecules that contain conjugated double bonds οƒΌ Polycyclic aromatic compounds (with great number of Ο€ electrons) οƒΌ Substituents strongly affect on the fluorescence; substituents such as NH2, NHCH3, N(CH3)2, OH and OCH3 groups enhance the fluorescence, while electron with drawing group such as NO2 Cl-, Br-, I- and COOH groups decrease the fluorescence οƒΌ Formation of metal chelates promotes the fluorescence. 14
  • 15. Phosphorescence may be expected generally in οƒΌ Aromatic hydrocarbons οƒΌ Introduction of substituents such as NH2, SH, OH to aromatic hydrocarbon enhance the phosphorescence and also aromatic nitro compounds οƒΌ Majority of aromatic aldehydes and ketones show phosphorescence. 15
  • 16. Fluorescence Spectra Instruments that measure the intensity of fluorescence are called fluorimeter. Those that measure the fluorescence intensity at variable wavelengths of excitation and emission, and are able to produce fluorescence spectra are called spectrofluorimeters In the recording the fluorescence spectra, the limitations of light sources and measuring devices assume real significance. These limitations are: οƒΌ Variation of the intensity of available energy with Ξ». οƒΌ Variation in the response of the detector to light of different wavelengths 16
  • 17. . Excitation Spectra: Before a compound can fluoresce, energy must be observed, and with an ideal light source, of constant intensity at different wavelengths, the most intense fluorescence is produced by radiation corresponding in wavelength to that of the absorption peak of the substance. Therefore, if the intensity of the fluorescence is plotted as a function of the wavelength of the radiation used to excite the fluorescence, an activation or excitation spectrum will, result. This will be identical to the absorption spectrum when corrected for instrumental effect, because the fluorescence efficiency is greatly independent of Ξ» . 17
  • 18. Fig; Fluorescence excitation and emission spectra for a solution of quinine 18
  • 19. Emission Spectra (Fluorescence) When a monochromator source of constant light intensity is used to irradiate a sample, the fluorescence may be analysed in a monochromator at constant slit width to give apparent emission spectrum. The true spectrum is obtained by applying a correction for change in detector sensitivity with wavelength and for changes due to fluorescence monochromator i.e., half band width of emergent light and light losses. Fluorescence emission spectra arise because of transition from the first excited state and their shapes are therefore independent of the light used to excite fluorescence. 19
  • 20. FACTORS AFFECTING FLUORESCENCE INTENSITY; οƒ˜ Concentration οƒ˜ Quantam yield οƒ˜ Intensity of incident light I0 οƒ˜ Pathlength (b) οƒ˜ Adsorption οƒ˜ Oxygen οƒ˜ pH οƒ˜ Temperature and viscosity οƒ˜ Scatter 20
  • 21. Concentration: The fluorescence intensity of a substance is proportional to concentration only when the absorbance in a 1 cm cell is less than 0.02. If the concentration of the fluorescent substance is so great that all incident radiation is absorbed, the equation will be: F = I0 Ο• That is the fluorescence is independent of concentration, and proportional to the intensity of incident radiation only, a property that may be utilized to determine the approximate emission characteristics of a light source 21
  • 22. Diagrammatic representation of the variation of fluorescence intensity with concentration. Region (a): Proportional relationship Region (b): Negative deviation from linearity. Region (c): Fluorescence independent of concentration Region (d): Reabsorption of fluorescence 22
  • 23. Quantum yield of fluorescence (Ο•) This is the ratio: Ο• = π‘›π‘œ.π‘œπ‘“ π‘β„Žπ‘œπ‘‘π‘œπ‘›π‘  π‘’π‘šπ‘–π‘‘π‘‘π‘’π‘‘ π‘›π‘œ.π‘œπ‘“ π‘β„Žπ‘œπ‘‘π‘œπ‘›π‘  π‘Žπ‘π‘ π‘œπ‘Ÿπ‘π‘’π‘‘ Since some absorbed energy is lost by radiation less pathways, the quantum efficiency is less than 1. Highly fluorescent substances take Ο• value near 1, which shows that most of the absorbed energy is re-emitted as fluorescence. For e.g.; fluorescein in 0.1 M NaOH and quinine in 0.05 M H2SO4 have, Ο• values of 0.85 and 0.54 respectively at 23Β°C. Non-fluorescent substances have Ο• = 0. 23
  • 24. Intensity of incident light 𝐈 𝟎 : An increase in the intensity of light incident on the sample produces a proportional increase in the fluorescence intensity. The intensity of incident light depends on the intensity of light emitted from the lamp. 24
  • 25. Pathlength (b) The effective pathlength viewed by the detector depends on both the excitation and emission slit widths. 25
  • 26. Adsorption: The extreme sensitivity of the method requires very dilute solution, 10-100 times, weaker than those employed in absorption spectrophotometry. Adsorption of the fluorescent substance on the container walls may therefore presents serious problems and strong stock solutions must be kept and diluted as required. Quinine is a typical example of a substance which is adsorbed onto cell walls. 26
  • 27. Oxygen The presence of oxygen may interfere in two ways: οƒΌ By direct oxidation of the fluorescent substance to non- fluorescent products. οƒΌ By quenching of fluorescence. 27
  • 28. pH  It is to be expected that alteration of the pH of a solution will have a significant effect on fluorescence if the absorption spectrum of the solute is changed. 28
  • 29. Temperature and viscosity Variation in temperature and viscosity will cause variations in the frequency of collision between molecules. Thus, an increase in the temperature or the decrease in the viscosity is likely to decrease the fluorescence by deactivation of the excited molecules by collision. 29
  • 30. Quenchers Quenching is the reduction of the fluorescence intensity by the presence of substances in the sample other than the fluorescent analyte. οƒΌ Static Quenchers: Form a chemical complex with the fluorescent substance and alter its fluorescence characteristics. Certain xanthine derivatives e.g. caffeine, reduce the fluorescence of riboflavin by static quenching. 30
  • 31. Scatter The excitation and emission monochromators are at the same wavelengths, scattered light of the same wavelength as the incident light will be detected by the photomultiplier arising from colloidal particles in the sample (Tyndall scatter) and from the molecules (Rayleigh scatter) 31
  • 32. . Raman Scatter: Arises from the conversion of some of the incident radiation into vibrational and rotational energy by the solvent molecules. The resultant scattered light is of lower energy and, consequently of longer wavelength. 32
  • 33. INSTRUMENTATION When both the excitation and emission spectra are to be recorded, two monochromator are essential, one for the light source (excitation monochromator) and one for the fluorescence (emission monochromator). The light source must provided a high level of UV and Visible radiation and a compact high pressure Zenon arc lamp is used. The production of ozone by the photochemical conversion of atmospheric oxygen in the lamp compartment presents a toxic hazard unless the ozone is thermally decomposed or removed by adsorption onto charcoal. As many experiments will almost certainly entail the measurement of very weak fluorescence. The detector must be a highly sensitive photomultiplier tube of low dark current. If the main interest lies in the fluorescence emission spectra, one monochromator may be dispensed with a suitable light source33
  • 34. and filter used instead. The rather poor luminosity associated with the monochromator even with a xenon arc lamp is replaced by the much more intense light from a source such as a mercury vapour lamp, from which a suitable activation beam is isolated by means of the filter. This arrangement partially overcome, one of the difficulties inherent in spectrofluorimetry, i.e., that so much of the available light is lost. 34
  • 36. ADVANTAGES OF SPECTROFLUORIMETRY οƒ˜ High sensitivity οƒ˜ Selectivity οƒ˜ Quantitative Aspects 36
  • 37. Quantitative Aspects: Many of the quantitative aspects of spectrofluorimetry may be understood by reference to the fundamental equation for the intensity of the fluorescence emitted. This equation may be derived from that of the Beer-Lambert law: A = Log 𝑰 𝟎/𝑰 𝒕 = abC Or 𝑰 𝟎/𝑰 𝒕 = 𝟏𝟎 𝒂𝒃𝒄 ∴ 𝑰 𝒕= 𝑰 𝟎 x πŸπŸŽβˆ’π’‚π’ƒπ’„ 37
  • 38. but fluorescence (F) = (𝑰 𝟎- 𝑰 𝒕)Ο• where Ο• is the quantum yield of the fluorescence At very low absorbance (< 0.02), the equation will be F= 2.3 𝑰 𝟎 abC Ο• For a fixed set of instrumental (𝐼0 and b) and sample (a andΟ•) parameters, the fluorescence is proportional to the concentration. F= K C where K = 2.3 𝑰 𝟎 a b Ο• 38
  • 39. APPLICATIONS OF SPECTROFLUORIMETRY οƒ˜ Compounds which are fluorescent are readily determined with simple instruments as the solution for examination is normally obtained by dissolution of the sample in a suitable solvent (table 1) 39
  • 40. οƒ˜ Single substances which are in themselves, non- fluorescent may be determined as a result of chemical change. e.g.; Determination of primary amines, amino acids, peptides etc. through: 40
  • 42. οƒ˜ Determination of primary and secondary aliphatic amines through: a- reaction with 4-chloro-7-nitrobenzo-2-oxa-l,3-diazole ( NBD-CI ) give yellow fluorescence 42
  • 43. b- reaction with l-dimethylaminonaphthalene-5-sulphonyl chloride (Dansyl, chloride) 43
  • 44. Thiamine HCI in pharmaceutical preparations such as tablets and elixirs and in food stuffs such as flour is relatively easily determined by oxidation to highly fluorescent thiochrome. The product is soluble in 2-methyl-propan-1-ol and hence is easily extracted from the reaction mixture for measurements 44
  • 45. For mixture of two components, it may be possible to select the exciting radiation of appropriate wavelengths, such that only one compound fluoresces at any time. Even if there is not possible, measurements of the fluorescence at two wavelengths may be sufficient to determine the composition of the mixture. 45
  • 46. CONCLUSION οƒ˜ Fluorescence is most sensitive analytical techniques. οƒ˜ Detection studies will increase the development of fluorescence field. οƒ˜ Flurometric method are much useful in qualitative analysis as compared to quantitative analysis. 46
  • 47. REFERENCES 1. Douglas a, Skoog , Holler, PRINCIPLE OF INSTRUMENTAL ANALYSIS, 5th edition , Saunders college, west Washington square, Philidhepia 2. Dr Ravishankar , A TEXTBOOK OF PHARAMACEUTICAL ANALYSIS, 3rd edition, Rx pub., 57, west car street, Tiruneveli-627006 3. Gr Chatwal , S.K. Anand, INSTRUMENTAL METHOD OF CHEMICAL ANALYSIS, Himalaya pub. house pvt ltd, Ramdoot', Dr. Bhaleraomarg, girgaon, Mumbai - 400 004, Maharashtra, India 47