CHAPTER – I Introduction
1
1. Introduction:
Present work is based on photoinduced electron transfer (PET) between
electron donor-acceptor systems. The process involves absorption of UV-
visible photon by one of the component which is specifically fluorescent and
has capability either to donate or accept electron with the molecule of other
component present within the approach of 10 Ao in suitable solvent
environment to get binded. The binding between two molecules of different
components in the excited state results into decrease in fluorescence of excited
molecule. Hence such process involving electron transfer on absorption of UV
-visible photon called PET can be studied by measuring the quenching of
fluorescence of photosensitive component as a function of concentration of
other component which may be an analyte of significance as pharmaceutical,
biological and environmental molecule. The systematic measurement on
intelligently selected appropriate electron donor-acceptor molecules of two
different components helped to develop new analytical methods for detection
as well as to understand molecular interactions. Therefore the subject
fluorescence, PET processes and their applications are reviewed in this chapter.
1.1 Luminescence:
Luminescence is the emission of light from any substance that occurs
from electrically excited state. Stokes (1852) formulated the first law in the
history of luminescence, which states that the wavelength of the luminescence
is greater than the wavelength of the exciting radiation [1]. The term
“Luminescence” was introduced into the literature by Wiedemann (1888). He
also offered the first, although not entirely accurate, defination of luminescence
as the excess emission over and above the thermal emission background [2].
This definition reflected an important property, but it did not distinguish
luminescence from other type of glow that is also excess emission over and
above thermal emission background. Vavilov (1951-52) suggested
complimenting Wiedemann‟s definition by addition the correction of duration
and using the term luminescence for the excess emission over and above the
CHAPTER – I Introduction
2
thermal emission of a body, if this emission has a duration considerably
exceeding period of light oscillations [1-3]. Thus luminescence is the emission
of cold light in which all or part of absorbed energy is re-emitted in the form of
electromagnetic radiation in the visible or near visible region of the spectrum.
It involves two main steps, the excitation of the electronic system of the
material and the subsequent emission of photons. The examples of
luminescence are the light or glow emitted by a luminous watch dial, fireflies,
glowworms, the lantern fish (Lucerna piscis), Nile fish (dilyxnos), bacteria,
rotten wood, fungus, mushrooms, mollusc, squid, etc. Luminescence contrasts
with incandescence, which is the production of light by heated materials [1-5].
The processes of luminescence are detailed as,
1. Absorption of energy by the electron of the atoms of the absorbing
materials causes the excitation of electron and it jumps from the inner orbits of
the atoms to the outer orbits.
2. When the electrons fall to their original state, a photon of light is
emitted. The interval between the steps may be short (less than 1/10, 000 of a
sec.) or long (many hours). If the interval is short, the process is called
fluorescence and if the interval is long, the process is called phosphorescence.
In either case the light produced is almost always of lesser energy and of longer
wavelength than the exciting light [1, 3-4].
Present studies involve monomer fluorescence and it‟s quenching by
electron transfer hence fluorescence and its aspects are revised.
1.2 Photoluminescence:
Generating luminescence through excitation of a molecule by ultraviolet
or visible light photons is a phenomenon termed photoluminescence. It is
formally divided into two categories as fluorescence and phosphorescence,
depending upon the electronic configuration of the excited state and emission
pathway [6].
CHAPTER – I Introduction
3
Fig. 1.1.a: Spin configuration of singlet and triplet excited states.
The electronic states of most organic molecules can be divided into singlet state
and triplet state. In singlet state, all electrons in the molecules are spin-paired
while in triplet state, one set of electron spins is unpaired as shown in Fig.1.1.a.
1.3 Fluorescence:
Fluorescence is emission of light from singlet-excited states, in which
the electron in the excited orbital return to the ground state and this spin-
allowed transition occurs rapidly by emission of a photon [4, 7-8]. With a few
rare exceptions, molecules in condensed phase rapidly relax to the lowest
vibrational level of S1. This process, called internal conversion, is nonradiative
and takes place in 10-12
seconds or less. Return to the ground state occurs to a
higher excited vibrational ground-state level, which then quickly reaches
thermal equilibrium. An interesting consequences of emission to a higher
vibrational ground state is that the emission spectrum is typically a mirror
image of the absorption spectrum of the 10 SS . This emission rates of
fluorescence are 108
s-1
, so that a typically fluorescence lifetime is near 10
nanoseconds. Fluorescence spectral data are generally presented as emission
spectra. Emission spectra vary widely and are dependant upon the chemical
structure of the fluorophore and the solvent in which it is dissolved.
CHAPTER – I Introduction
4
1.3.1 Mechanism of Fluorescence:
On absorption of light the molecule is raised from the ground state G to
the excited state E, the resulting electronic transition is shown in Fig.1.1.b as
per the Frank- Condon principle [9].
A Absorption F Fluorescence T Triplet state
P Phosphorescence
Fig.1.1.b: Electronic transitions
The molecule returns to the ground state by emitting some of its absorbed
energy as fluorescence. An electronic transition due to light absorption is
almost instantaneous (10-15
second) whereas the lifetime of the excited state is
about 10-8
second and therefore the whole process of light absorption and
fluorescence emission takes place in about 10-8
second. Now some of the
absorbed energy is lost partly by collisions with other molecules so that the
emitted energy is less than the energy absorbed from the exciting light.
Fluorescence is thus an emission from a singlet excited state (electrons spin
paired) to ground state where as phosphorescence is emission from a triplet
excited state (electrons unpaired) to ground state. Phosphorescence persists
longer than fluorescence and this persistence are prolonged and the intensity
enhanced by low temperature [7].
1.3.2 Jablonski diagram:
Processes, which occur between the absorption and emission of light,
are usually illustrated by Jablonski diagram shown in Fig. 1.2. The ground, first
and second electronic states are depicted by S0, S1 and S2, respectively. At each
E
G
Excited state
(Singlet)
CHAPTER – I Introduction
5
electronic energy level, the fluorophores can exist in a number of vibrational
energy levels. Transitions between states are depicted as vertical lines to
illustrate the instantaneous nature of light absorption. According to the Franck-
Condon principle, transitions occur in about 10-15
seconds, a time is too short
for significant displacement of nuclei [5]. The highest probability of the
transition corresponds to the largest overlap between the ground state and
excited-state vibrational wavefunctions.
Fig.1.2: A simplified diagram with absorbance, internal conversion,
fluorescence, intersystem crossing and phosphorescence
1.3.3 Types of Fluorescence: ,
The fluorescence which is observed as long as excitation is in process is
known as steady state or prompt fluorescence. When excitation is cut off, this
fluorescence ceases. However, in some case even after cutting of source of
excitation, the emission of light persists as a glow and is known as delayed
fluorescence.
1. Steady State Fluorescence:
2. Delayed Fluorescence
CHAPTER – I Introduction
6
1.4 Processes competing with Fluorescence:
1.4.1 Vibrational Relaxation (VR):
Emission spectra are typically independent of the excitation wavelength.
Upon excitation to higher electronic and vibrational levels, the excess energy is
quickly dissipated, leaving the fluorophore in the lowest vibrational levels of
S0. As a consequence, fluorescence from solution, when it occurs, always
involves a transition from the lowest vibrational level of an excited state S1 [4,
10]. Due to vibrational relaxation the fluorescence band for a given electronic
transition is displaced toward lower frequencies or longer wavelengths from the
absorption bands (Stoke‟s effect).
1.4.2 Internal Conversion (IC):
Internal conversion is a non-radiative transition between two electronic
states of the same spin multiplicity. In solution, this process is followed by a
vibrational relaxation towards the lowest vibrational level of the final electronic
state. The excess vibrational energy can be indeed transferred to the solvent
during collisions of the excited molecule with the surrounding solvent
molecules. Thermally relaxed excited molecules transfer energy into
isoenergetic vibrational level of ground state level which follows vibrational
relaxation [11]. Internal conversion from S1 to S0 is also possible but is less
efficient than conversion from S2 to S1, because of the much larger energy gap
between S1 and S0. Therefore, internal conversion from S1 to S0 can compete
with emission of photons (fluorescence) and intersystem crossing to the triplet
state from which emission of photons (phosphorescence) can possibly be
observed.
1.4.3 Intersystem Crossing (ISC):
Intersystem crossing is a non-radiative transition between two
isoenergetic vibrational levels belonging to electronic states of different
multiplicities. For example, an excited molecule in the 0 vibrational level of the
S1 state can move to the isoenergetic vibrational level of the Tn triplet state;
CHAPTER – I Introduction
7
then vibrational relaxation brings it in to the lowest vibrational level of T1.
Intersystem crossing may be fast enough (10-7
–10-9
s) to compete with other
pathways of de-excitation from S1 (fluorescence and internal conversion
S1 S0) Crossing between states of different multiplicity is forbidden, but spin–
orbit coupling (i.e. coupling between the orbital magnetic moment and the spin
magnetic moment) can be large enough to make it possible. The probability of
intersystem crossing depends on the singlet and triplet states involved. If the
transition S0 S1 is of *n type for instance, intersystem crossing is often
efficient. It should also be noted that the presence of heavy atoms (i.e. whose
atomic number is large, for example Br, Pb) increases spin–orbit coupling and
thus favors intersystem crossing [12].
Once ISC has occurred, the molecule undergoes the usual IC process
and falls to the lowest vibrational level of the first excited triplet state.
Therefore, ISC can compete with fluorescence and thus it decreases the
quantum efficiency of fluorescence. The population of triplet state has
significance in producing delayed fluorescence and phosphorescence, which is
a radiative decay of triplet state molecule to the ground state. Different
pathways for de-excitation of excited molecules are exhibited in Fig. 1.3.
Fig.1.3: De-excitation pathways of excited molecules
CHAPTER – I Introduction
8
1.5 Structural factors on Fluorescence Measurements:
1.5. a. Effect of electron-withdrawing substituents: (carbonyl and nitro
compounds)
The fluorescence properties of aromatic carbonyl compounds are
complex and often difficult to predict. Many aromatic aldehydes and ketones
(e.g. benzophenone, anthrone, 1- and 2- naphthaldehyde) have a low-lying n–p
excited state and thus exhibits low fluorescence quantum yields, as explained
above and the dominant de-excitation pathway is intersystem crossing.
O O
OO
O O
H
4a,9a-dihydroanthracene-9,10-dione anthracene-9-carboxylic acid 9H-fluoren-9-onediphenylmethanone
Some aromatic carbonyl compounds have a low-lying * excited
state and thus have a reasonable quantum yield (e.g. 0.12 for fluorenone in
ethanol at 77 K and 0.01 at room temperature). However, if a *n state lies
only slightly higher in energy, the fluorescence quantum yield strongly depends
on the polarity of the solvent. In fact, in some solvents, the energy of the
*n state can become lower than that of the * state. When the
polarity and the hydrogen bonding power of the solvent increases, the
*n state shifts to higher energy whereas the *state shifts to lower
energy. Therefore, intense fluorescence can be observed in polar solvents and
weak fluorescence in nonpolar solvents (e.g. xanthone). When an aromatic
molecule has a carboxylic group as a substituent, photophysical effects due to
conformational changes can be observed. For instance, anthracene-9-carboxylic
acid exhibits a broad fluorescence spectrum deprived of apparent vibronic
bands, in contrast to its absorption spectrum and to both absorption and
fluorescence spectra of the conjugate base. Such a difference between the
fluorescence spectra of the acidic and basic forms can be explained in terms of
CHAPTER – I Introduction
9
conformation of the carboxylate group a -COO-, which should be almost
perpendicular to the ring so that the p system of the anthracene ring is only
slightly perturbed. On the contrary, the carboxylic group a -COOH may be in a
position close to the coplanarity of the ring; the resulting interaction induces an
intramolecular charge-transfer character to the *transition. Charge-
transfer fluorescence bands are indeed usually broad and structureless.
However, because the absorption spectrum of the acidic form exhibits vibronic
bands, the rotation of the -COOH is likely to be photoinduced. In general, the
fluorescence of aromatic hydrocarbons possessing a -NO2 substituent is not
detectable. The existence of a low-lying *n transition explains the
efficient intersystem crossing process (e.g. for 2-nitronaphthalene, the quantum
yield for intersystem crossing is 0.83 in benzene solvent at room temperature).
Many nitroaromatics are indeed phosphorescent. However, in some cases, the
quantum yield for intersystem crossing is significantly less than 1. Therefore,
the absence of detectable fluorescence is likely to be due to a high rate of
01 SS internal conversion, which may be related to the considerable charge-
transfer character of the excited state, as a result of the strong electron-
withdrawing power of the -NO2 group. It should be mentioned that many
nitroaromatics undergo photodegradation. For instance, 9-nitroanthracene is
transformed into anthraquinone upon illumination.
1.5.b. Electron-donating substituents: ( COH, COR, CNH2, CNHR,
CNR2)
In general, substitution with electron-donating groups induces an
increase in the molar absorption coefficient and a shift in both absorption and
fluorescence spectra. Moreover, these spectra are broad and often structureless
compared to the parent aromatic hydrocarbons (e.g. 1- and 2-naphthol
compared to naphthalene). The presence of lone pairs of electrons on the
oxygen and nitrogen atoms does not change the *nature of the
transitions of the parent molecule. These lone pairs are indeed involved directly
in p bonding with the aromatic system, in contrast to the lone pairs of electrons
CHAPTER – I Introduction
10
of carbonyl substituents or heterocyclic nitrogen. To make the distinction
between the two types of lone pairs, Kasha and Rawls suggested using the term
“l orbital” for the lone pair orbital of aromatic amines and phenols. A
significant intramolecular charge transfer character of the relevant transitions is
expected for planar aromatic amines and phenol; this is confirmed by the fact
that the fluorescence spectra are broad and structureless. If, for steric reasons,
the -NH2 group is twisted out of the plane of the aromatic ring, the degree of
conjugation of the “l orbital” is decreased, but the transitions corresponding to
the promotion of an electron from an “l orbital to a p orbital” are still different
(in particular more intense) to the *n transitions involving the lone pairs
of a carbonyl or nitro group. Departure from coplanarity with the aromatic ring
is also pronounced with -OR substituents, whereas an -OH group is nearly
coplanar [13].
1.5.1 Fluorescence Intensity:
The height of emission peak at maximum emission wavelength gives,
intensity of fluorescence (F). The intensity of fluorescent light is directly
related with the concentration of fluorescent solute in solution as given by
following relation.
F = (I0 – I) f --------------------- (1)
If f is constant in the measured excitation range, then the shape of the
fluorescence excitation spectrum is determined solely by the extinction
coefficient of the molecule [14].
1.5.2 Factors affecting on Fluorescence Intensity:
1.5.3 Concentration of fluorescent solution:
The intensity of fluorescence is proportional to the concentration of the
fluorescent compound only in highly dilute solutions and therefore the
concentration of the compound to be assayed is a very important consideration
CHAPTER – I Introduction
11
in quantitative work [15]. Fluorophor exists as an isolated molecule when
solution is dilute and emission is monomer fluorescence. However, increase the
concentration results into aggregation called excimer or photodimer which
automatically quenches monomer fluorescence. The complexation of
fluorophor with solvent or impurity leads into fluorescence quenching.
Increase in concentration of fluorescent solutions usually results in quenching
at high concentrations and this is often accompanied by wavelength shifts.
Concentration effects can be ascribed to various phenomena including
reabsorption of emitted light, “true” concentration quenching, dimerization or
aggregation, and miscellaneous experimental and instrumental factors. The
examination of concentration effects is of importance because of the
information obtained in this manner about solute-solute and solute-solvent
interactions. Furthermore, the effects of concentration have to be taken into
account in the measurement of quantum yields of fluorescence and relative
fluorescence intensities [16].
1.5.4 Solvent effect:
Fluorescence intensity and wavelength are affected by change of
solvent. For solvent effect it will be convenient to consider three aspects.
a) Purity of the Solvent:
Since fluorescence is highly sensitive technique, it is important that the
solvents used, should themselves be non-fluorescent and free from fluorescent
impurities. These solvents may be used either for extracting the desired
material or for the actual fluorescence measurement. All solvents should be
checked that they do not contain any undesirable fluorescence and otherwise
vigorously purified. Purification of solvents must be carried out before its use
in fluorescence study [17]. The attention should be paid to the cleaning agents
used to clean glassware. The chromic acid absorbs ultraviolet light and it is
preferable to clean cuvettes in nitric acid rather than in chromic acid. Some
CHAPTER – I Introduction
12
solvents also absorb specific wavelengths of light and therefore care to be taken
by avoiding the fluorescence in the region of their absorption.
b) Aqueous buffer solutions:
The constituents of the buffer also affect the fluorescence. Commercial
buffer solutions contain constituents, which are not always disclosed by the
manufactures [14]. These constituents could have a fluorescence of their own
or they could be quenching agents. In the case of phosphate buffers, an increase
of phosphate concentration frequently leads to a decrease in fluorescence
intensity.
c) Non-aqueous Solvents:
Fluorescence often varies with solvent and several reasons have been
put forth to explain this alternation in fluorescence [18], on the basis of
dielectric constants of the solvent, the association of solvent and solute by
hydrogen bonding , quenching by solvent molecules and ionization. Report on
Indole indicates the same maximum excitation of 285 nm in solvents, but the
wavelength of maximum fluorescence is 297 nm in cyclohexane, 305 nm in
benzene, 310 nm in water. The fluorescence wavelength thus increases with the
dielectric constant of the solvent due to an effect on the -electrons.
1.5.5 Effect of pH:
The effect of pH upon the fluorescence of a compound is of
considerable importance and knowledge of fluorescence brought about by pH
changes in the medium can be valuable from several aspects. The basicity or
acidity of molecules is determined by its electronic structure and this may
undergo detailed changes during excitation from the ground state by the
absorption of light due to changes in the basicity or acidity of a compound
during excitation. A difference in the basicity or acidity of the ground and
excited states will be reflected in differences between the absorption and
fluorescence spectra with change in pH. The nature of the changes will depend
CHAPTER – I Introduction
13
on whether the basicity is increased or decreased during ionization. Thus a
compound may be fluorescent only over a short range of pH, as in the case of
sulphapypridine, which is practically non-fluorescent above pH 4 and is
maximally fluorescent at pH 0.5 to 1.0 [19]. Again a compound may be
fluorescent over a considerable range of pH, but over a certain section of that
range it may be much more fluorescent than over the rest, similarly mono
methyl aniline which has a replaceable hydrogen atom behaves exactly like
aniline but dimethylaniline which does not have such a hydrogen, does not lose
it‟s fluorescence at high pH values [20].
1.6 Experimental Parameters:
The experimental parameters generally used to measure the properties of
any luminescent system are,
1.6.1 Absorption spectra
1.6.2 Emission spectra
1.6.3 Excitation spectra
1.6.4 Fluorescence quantum yields
1.6.5 Fluorescence life time
1.6.1 Absorption spectra:
Einstein relation gives the quantization condition for the absorption or
emission of light by an atom or by molecule
h = hc/ = E2 –E1 --------------- (2)
where, E2 and E1 are the electronic energy levels, h is Planck‟s constant and ,
and c are the frequency, wavelength and velocity of the incident photon.
The Beer-Lambert‟s law governs the absorption of energy by a
molecule. According to this relationship
Log10 (I0/I) = c l ----------------- (3)
Where
I0 = intensity of incident light
CHAPTER – I Introduction
14
I = intensity of transmitted light
= molar extinction coefficient
c = concentration of the solution
l = path length of the absorbing system through which light passes and
Log10 (I0/I) = optical density or absorbance of the material
In practice, the absorption spectrum is plotted in terms of molar
extinction coefficient ( ) against frequency or wavelength.
Figure 1.4 is a typical absorption spectrum for a S0 S1 transition. The
probability of the absorption depends upon the degree of overlap of the wave
function of the lowest vibrational level of the ground state S00 and the wave
function of the vibrational levels of the first excited singlet state S10 S1n.
Fig.1.4: Illustration of the vibrational bands in the absorption and
fluorescence spectra of aromatic hydrocarbons
CHAPTER – I Introduction
15
The positions of the absorption peaks and its nature are of significance
in the spectroscopic studies. The nature of the absorption spectrum indicates
the monomeric or dimeric state of the molecular systems, which is of
importance to explore whether the ground state dimer or a monomer is excited
in the absorption process [21]. In solution the broad absorption band is an
indication of dimeric nature of molecules in the ground state while the
structured spectrum indicates the existence of monomolecular species [22]. The
absorption of solids is not as structured as in solution. The nature of absorption
bands also gives an idea about the lattice structures of molecular systems under
study and suggests the possibility of formation of dimeric species [8].
Extensive work has been carried out to establish exact relationship
between absorption and emission properties of organic crystalline materials
with a view to explore electronic and molecular structure of materials in
condensed state [23]. The position of the absorption bands in the spectra of
aromatic hydrocarbons depends upon the number of benzene rings and the way
by which they are condensed. In linearly condensed molecules, band of
absorption spectrum moves towards longer wavelength of the electromagnetic
spectrum. This effect is mainly due to decrease in energy difference between
lower excited and ground state of the molecule. As the number of condensed
rings increases this energy difference becomes progressively less in the linear
polynuclear aromatic hydrocarbons [24]. But in non-linear hydrocarbons the
situation becomes reverse and the energy difference increases as the number of
bends (angular condensation) in the molecule increases.
1.6.2. Emission spectra:
Emission spectrum is the plot of intensity of fluorescence vs.
wavelength. The fluorescence emission spectrum is obtained by irradiating the
sample by a wavelength of maximum absorption as indicated by absorption
spectrum of the sample. Figure 1.5 reveals the levels of the ground S0 and
excited state S1 associated with the absorption and emission spectra. It is
observed that the absorption spectra gives data about the vibrational levels of
CHAPTER – I Introduction
16
the excited state and the emission spectra yields data about the vibrational
levels of the ground state. In most of the organic materials, the emission
spectrum is the mirror image of the absorption spectrum. This relationship is an
indication of the similarity of the respective vibrational wave functions in the
excited and ground states. Birks and Dyson (1963) [25] reported that this
mirror image relationship is not observed in some molecular systems. In such
systems there is some degree of hindrance to the normal relaxation processes in
the excited or ground state.
1.6.3 Excitation spectra:
Excitation spectroscopy of the fluorescent samples gives a further way
of gaining information about the excited states of organic molecules. An
excitation spectrum is obtained by studying variation in the fluorescence
quantum intensity as a function of excitation wavelength. For most of the
organic molecules the quantum yield is independent of excitation wavelength,
this is due to very efficient process of internal conversion from higher excited
states to the lowest excited singlet states. Even for those molecules for which
quantum intensity is invariant with excitation wavelength, the excitation
spectra provide a powerful tool for measuring the absorption spectra of
molecules, which are at too low concentration for detection by absorption
spectrometry.
The excitation spectrum will be identical to the absorption spectrum
where cd 1. The measurement of quantum intensity is limited by the
sensitivity of the spectrofluorometer and that depends upon the intensity of the
excitation source. Parker (1968) [24] estimated that concentrations as low as
10-12
mol dm-3
can be detected by excitation spectroscopy compared with a
minimum concentration of 10-8
mol dm-3
by absorption spectroscopy.
Excitation spectroscopy is also used to determine the quantum efficiency of
energy transfer between donor and acceptor molecules.
CHAPTER – I Introduction
17
1.6.4 Fluorescence Quantum Yields:
Fluorescence quantum yield is the major characteristics of a
photochemical reaction. The fluorescence efficiency or the quantum yield ( f)
of a fluorophores is defined as the fraction of the incident radiation that is
reemitted as fluorescence. A high quantum yield value near to 1 (100%
efficiency of the emission process) is generally observed with molecules
having large planar conjugated systems that are relatively rigid [11, 26]. More
flexible molecules are more likely to have values of f, while molecules whose
lowest excited state is achieved by n * transition or that contain heavy
atoms such as bromine or iodine are usually non fluorescent. Quantum yield is
characteristic for each fluorescent compound and is independent of the
excitation and emission wavelength.
Determination of relative quantum efficiency at room temperature of the
two substances is practically simple [13]. The measurement with modern light
sensitive spectrofluorometers involves negligible errors due to excessive
absorption of incident light or due to self-absorption. Under such conditions the
rate of fluorescence emission is proportional to the product I0 cl f.
The integrated area under the corrected fluorescence spectrum is
proportional to the rate of emission of fluorescence and thus, if the
fluorescence emission spectra of two solutions or systems are measured with
the same experimental conditions like same instrumental geometry and at the
same intensity of exciting light then the ratio of the two fluorescence intensities
is given by,
)(10
20
1
2
area
area
clI
lcI
F
F
11
22
)(
)(
densityoptical
densityoptical ---------------------- (4)
CHAPTER – I Introduction
18
1.6.5 Fluorescence life time:
When an electron is promoted to the higher energy state by absorption
of one quantum of radiation, the question is that to how long it will remain in
the excited state before returning to the ground state. The time spent by an
electronically excited molecule in the higher energy state is known as the
natural radiative life time of the atom or molecule. After this time, the system
reverts spontaneously to its original state by emission of radiation of an
appropriate energy. The fluorescence lifetime of most organic molecules is in
the nanosecond region. The fluorescence life time refers to the mean lifetime of
the excited state i.e. the probability of finding a given molecule that has been
excited still in the excited state after time t is e-t/τ
. The general equation relating
the fluorescence intensity I and the lifetime τ is
I = I0 e-t /τ
where I is the fluorescence intensity at time t, I0 is the maximum fluorescence
intensity during excitation, t is the time after removal of the excitating radiation
and τ is the average lifetime of the excited state.
The precise measurement of the observed lifetime is important since it can
be used to calculate the natural lifetime τo or the absolute quantum efficiency,
Фo, if one or the other is known.
τ = Фo τo
The life time measured mostly by Time Resolved Fluorescence Spectroscopy
method.
1.7. Fluorescence Quenching Phenomenon:
The phenomenon of decrease in intensity of fluorescent compound at its
max is known as fluorescence quenching. When one compound diminishes or
abolishes the fluorescence of another, it is said to quench the fluorescence. The
quenching of fluorescence can be brought about in many ways like,
1.7.1 Inner filter effect
1.7.2 Chemical change
1.7.3 Energy degradation
CHAPTER – I Introduction
19
1.7.4 Energy transfer
1.7.5 Electron transfer
1.7.1 Quenching by inner filter effects:
Inner filter effects are instrumental effects. They have no influence on
the primary process of emission from molecule originally excited but simply
reduce the observed intensity of luminescence within the material being tested
[11, 27- 28]. The two kinds of inner filter effects are,
a) Excessive absorption of the exciting light,
b) Absorption of the luminescence emitted (solute quenching).
Therefore, the fluorescence intensity of most dyes increases linearly
with increasing concentration at relatively low dye concentrations. The
measured intensity is usually proportional to the optical density (OD) of the
dye solution. The fluorescence intensities can be approximately corrected for
the inner filter effects as follows,
]2/)log[( emexabscorr ODODAFF ------------ (5)
Many fluorescent dyes form dimer or higher aggregates in solutions of
higher concentrations particularly in non-polar solvents [29-30]. The second
type of inner filter effect is produced by the absorption of the fluorescence light
either by an excessive concentration of the fluorescent dye itself (self
absorption) or by other solutes. Self-absorption mainly affects the lower
wavelength side of the fluorescence emission band because in this region it
overlaps with the first absorption band. Self-absorption reduces the
fluorescence intensity. The presence of a second solute that absorbs strongly in
the region where the first solute fluoresces will also cause distortion in the
emission spectrum of the fluorescing dye.
1.7.2 Quenching by chemical change:
If a fluorescent compound undergoes a chemical change as a result of
presence of a second compound it could be converted into a non-fluorescent
product. Although, the fluorescence of the compound is quenched by the
CHAPTER – I Introduction
20
addition of the second compound, this form of quenching is to be distinguished
from „true‟ quenching during which no net chemical change occur. Quenching
by chemical change can occur in many ways but the end product is usually a
non-fluorescent compound.
Quenching can occur as result of pH changes in the solution. In case of
aniline when acid is added to it, the fluorescence begins to be quenched at pH-6
and at pH-2 the solution is non-fluorescent [11, 31]. This is due to the
conversion of aniline into the non-fluorescent anilinium ion, which is different
chemical species from aniline.
C6H5NH2 C6H5N+H3
Aniline (Fluorescent) Anilinium ion (Non-fluorescent ion)
1.7.3 Quenching by energy degradation:
Such quenching process involves concentration of singlet excited state
molecule into triplet state by energy or electron transfers, so the fluorophores
no longer emits its energy as fluorescence. The quenching affects of oxygen on
certain iodo, bromo and nitro compounds probably may be due to energy
transfer. The quenching of fluorescent molecules by electron donating I-, Br
-,
SCN , and S2O3
and electron accepting anions such as IO3 , NO3 and S4O6
are cases of involving electron transfer between donor-acceptor. In certain
cases energy transfer between the triplet energy level of quencher and excited
singlet level of fluorophore takes place when triplet energy level of quencher
lie below the excited singlet level of fluorophor which is probable in condensed
system, where donor-acceptor are more closer than in solution [32-33].
,
1.7.4 Quenching by energy transfer:
The system of donor – acceptor pair is excited by proper radiation, to
achieve selective excitation of donor molecules. The donor-acceptor pairs are
such that they satisfy the conditions required for efficient transfer of energy.
The acceptor molecule accepts the energy from donor and donor is deactivated
CHAPTER – I Introduction
21
to its ground state and acceptor is raised to singlet excited level. The excited
acceptors so formed de-excite to ground level either radiatively or non-
radiatively. In radiative process the fluorescence characteristics of acceptor
molecule is observed. The systematic variation of acceptor concentration
gradually quenches the fluorescence of donor by ET with simultaneous
sensitization of acceptor fluorescence. Förster (Fluorescence) Resonance
Energy Transfer (FRET) is a physical phenomenon described over 50 years
ago, that is being used more and more in biomedical research and drug
discovery today. It describes a non radiative energy transfer mechanism
between two chromophores. FRET relies on the proximity/ distance dependent
transfer of energy from a donor molecule to an acceptor molecule. This energy
transfer mechanism termed Förster resonance energy transfer named after the
German scientist Theodor Förster. The efficiency of FRET depends on the
following basic parameters-
a) the distance between donor and acceptor molecules,
b) the extent of overlap of the emission spectrum of the donor with the
absorption spectrum of the acceptor,
c) the relative orientation of the donor and acceptor transition dipoles,
d) the quantum yield of the donor.
FRET is the radiationless transmission of energy from a donor molecule, which
initially absorbs the energy, to acceptor molecule. The transfer of energy leads
to reduction in donor‟s fluorescence intensity and excited state lifetime and
increase in the acceptor‟s emission intensity. A pair of molecules that interacts
in such manner that FRETS occurs is referred as donor-acceptor pair. As
mentioned above, there should be proximity between donor and acceptor (10-
100 Å) and absorption/ excitation of acceptor must overlap with emission
spectrum of the donor as shown in Fig.1.5. The research group of our
fluorescence spectroscopy laboratory has also contributed on FRET and
analytical relations are established successfully to develop methods for
quantitative estimations of biomolecules such as vitamin B2 and norfloxacin
[35-36].
CHAPTER – I Introduction
22
Fig.1.5: Spectral overlap of excitation of acceptor with emission of donor.
1.7.5 Fluorescence quenching by electron transfer:
D+ + A D + A + Hole transfer
D - + A D + A- Electron transfer
D * + A D + A* Energy transfer
Scheme-I: Quenching mechanisms in energy transfer and electron
transfer processes
The quenching resulting from collisional encounters between the
fluorophore and quencher is called collisional or dynamic quenching. In this
type, the quencher must diffuse to the fluorophor during the life time of the
excited state. Upon contact, the fluorophore returns to the ground state, without
emission of a photon. This is a time dependent process. One experimentally
useful type of quenching is due to collisions between quenching agents and
CHAPTER – I Introduction
23
fluorophores, and is called collisional or dynamic quenching. A second type of
quenching is static quenching, in which the quenching agent forms a non-
fluorescent complex with the quenching agent. A final type of quenching,
discussed below, is resonance energy transfer. Static and dynamic quenching
requires direct contact between the fluorophore and the quencher. For dynamic
quenching, the result of this contact is loss of the fluorescence pathway for
return to the ground state, although the mechanism can vary significantly with
the quenchers. Some quenchers act by inducing intersystem crossing (oxygen
and iodide are thought to quench by this method). Others, such as aromatic
amines, appear to donate electrons to the excited state. In the case of dynamic
quenching, contact must occur while the fluorophore is in excited state.
Dynamic quenching is exhibits a concentration-dependence that is described by
the Stern-Volmer equation [37],
][11 0
0 QKQkF
FDq ----------------- (6)
where τ0 is the lifetime of the fluorescent state in the absence of the quenching
agent. If the quenching is not known to be due to dynamic quenching, KD is
replaced by KSV.
For dynamic quenching,
00
F
F ----------------- (7)
because the quenching agent decreases the lifetime of the excited state.
Dynamic quenching increases with temperature, because temperature increases
diffusion rates. The term kq is the second order rate constant that describes the
quenching process. It is proportional to the effectiveness of the quencher and
the accessibility of the fluorophore to collisions with the quencher. The
quenching rate constant is actually comprised of two terms,
f0= fQ k0
where fQ is the fraction of collisions that result in quenching, and k0 is the
diffusion controlled bimolecular rate constant which is given by,
CHAPTER – I Introduction
24
))((
1000
43
0
0 qfqf DDrr
L
cm
Nk -------------- (8)
where N0 is Avogadro‟s number, rf and rq are the radii of the fluorophore and
quencher, and Df and Dq are the diffusion coefficients of the fluorophore and
quencher. Typical values of k0 for free fluorophores and free quenchers are
~1010
mol-1
dm3sec
-1. If the fluorophore is bound to the surface of a protein, the
k0 will be roughly half of this value due to available surface occupied by the
protein. If the fluorophore is buried within the protein, the value of k0 will be
even smaller, depending on the accessibility of the fluorophore. Static
quenching is the result of the formation of a non-fluorescent complex between
the fluorophore and the quencher. The association constant for the quencher
fluorophore complex describes the effectiveness of a static quencher:
]][[
][
QF
FQK s ---------------------- (9)
where [FQ] is the complex concentration, [F] and [Q] are the concentrations of
free fluorophore and free quencher. The total fluorophore concentration F0, is
given by
[F]0 = [F] + [FQ] ------------------ (10)
]][[
][]0[
QF
FFK s
By rearranging the above equation,
][
1
]][[
][ 0
QQF
FK s
If it is believed that the all of the decrease in observed fluorescence is due to
complex formation then the equation becomes:
][10 QKF
Fs -------------------- (11)
The above equation is identical to the Stern-Volmer equation for dynamic
quenching. Static and dynamic quenching can be distinguished by lifetime
measurements because dynamic quenching reduces the apparent fluorescent
lifetime, while static quenching merely reduces the apparent concentration of
CHAPTER – I Introduction
25
the fluorophore. Alternatively, temperature effects can be used to distinguish
the two forms of quenching. Diffusion rate and therefore dynamic quenching
rate increases with temperature. In contrast, complex formation strength tends
to be inversely proportional to temperature and therefore static quenching tends
to be higher at lower temperatures. In some cases, the effect of the quencher is
due to a combination of static and dynamic quenching shown in Fig. 1.6. This
result in a modified equation can be written as [38],
20 ][])[(1])[1])([1( QKKQKKQKQKF
Fssds DD
------- (12)
Fig.1.6: Distinction between dynamic and static quenching
At high quencher concentrations, a dynamic quencher will appear to exhibit
combined quenching. This is thought to be due to the fact that, at high
concentrations, a significant amount of the quencher molecules are already in
close proximity to the fluorophore. Assuming that any quencher within a
sphere surrounding the fluorophore will quench the fluorescence, a modified
Stern-Volmer equation can be derived [39],
1000
][
00
])[1(
VNQ
d eQKF
F --------------- (13)
in which V is the volume of the sphere (V is usually slightly larger than the sum
of the quencher and fluorophore radii). In proteins, more than one population of
fluorophore may be present. This is especially true for tryptophan residues,
where some may be readily solvent accessible, and others may be buried.
Stern-Volmer plots for these proteins frequently curve downward, reflecting
the quenching of the accessible fluorophores. Assuming the buried fluorophore
is not quenched, and fluorescence will be,
CHAPTER – I Introduction
26
b
a
a FQK
FF 0
0
][1 ------------------- (14)
where Ka is the Stern-Volmer constant for the accessible quencher. In practice,
it is likely that the buried fluorophore will exhibit some quenching also, and
therefore the curve would be expected to be more complex than is described by
this equation. In quenching experiments with proteins, the quenching agent
may interact with the protein in ways that alter the protein structure or that
affect the degree of quenching observed. One method for examining this is the
use of several quenchers with different properties. Differential quenching by
positively and negatively charged quenchers suggests a charged environment.
Small KD values typically reflect the steric hindrance of quencher-fluorophore
collisions. Quenching studies may allow isolation of signals from different
fluorophores. They may also allow characterization of conformational changes
that alter the accessibility of the fluorophores to the quenching agent.
Fluorescence quenching by electron transfer (ET) is a one electron
reaction in which an electron jumps from an occupied (HOMO) orbital of one
reactant to an unoccupied (LUMO) orbital of the other as shown in Scheme II.
Scheme II: Photoinduced electron transfer mechanism between donor and
acceptor molecules
CHAPTER – I Introduction
27
Fig.1.7: The potential energy curves for PET system
Excited state intermolecular electron transfer between donor-acceptor pair
brought about by the absorption of UV or vis. photon are known as PET
reactions. Electron transfer reaction involves the crossing of the surface free
energy of the reactant to the product at transition state which is shown in Fig.
1.7. The excited state of sensitizer can be an electron donor or acceptor. In
either case, quenching by ET between uncharged species leads to a radical ion
pair or a charge-transfer complex. Electron transfer and energy transfer by
electron exchange require a close approach for effective orbital overlap [40-
41]. As a result the “range of effectiveness” of these mechanisms is usually
limited to distances of less than 10 A0. In contrast coulombic energy transfer
does not involve orbital overlap and can be effective from collision distances of
less than 10 A0 and up to separation distances as large as 100 A
0 [42].
Spin conversion is normally observed in both electron and energy
transfer i.e. the overall spin of the radical ion pair (electron transfer) and the
spin of the excited state of acceptor (energy transfer) match the excited state of
CHAPTER – I Introduction
28
sensitizer. Triplet-triplet energy transfer is forbidden by the dipole-dipole
mechanism and takes place by electron exchange [40]. This pathway can be
used to generate reactive triplet states that normally cannot be formed by direct
excitation [43]. Singlet-singlet energy transfer, which proceeds by spin-allowed
electron exchange and dipole-dipole interactions, has been used to probe the
structure of biological macromolecules [44].
In 1963 Leonhardt and Weller reported the emission of complexes
between perylene and dimethyl aniline [45]. These stoichiometric complexes
were postulated as forming by electron transfer between the excited singlet
state of perylene and the ground state of the amine. The term exciplex was
eventually coined to describe these complexes [46]. Today, an exciplex is
defined as two-component system in which charge and electronic excitation are
shared by the components. Many quenching reactions that proceed by electron
transfer involve exciplexes. This is particularly true for planer organic
molecules. Exciplex formation involving these molecules correlates with their
redox potentials and dipole measurements to confirm their charge-transfer
nature.
The primary electron transfer involves a transfer of an electron between
an excited-state and ground state molecules to generate a charge transfer
species, while secondary electron transfer refers to the electron-transfer
pathways which follows formation of the charge-transfer complex. These may
include reversible electron transfer to give the ground state reactants, ionic
dissociation into free ions, triplet recombination to generate an excited state of
one of the reactants, the formation of other charge transfer intermediates and
stable products. The ET can involve either electron transfer or an electron
exchange.
1.8 Fluorescence quenching pathways:
The dynamics of quenching electron transfer must take into account the
positions and motions of the reactants in a given molecular environment. The
processes in solutions classify the reaction pathways into two types.
CHAPTER – I Introduction
29
i) The reactants are the mobile and free to approach to close distances
within the lifetime of the excited partner.
ii) Structural factors keep the reactants separated at a fixed distance
during the lifetime of the excited partner.
1.8.1 Fluorescence quenching via encounter complex:
In a fluid medium, reactant molecules which are mobile and
unrestrained by structure or environment may form an encounter complex prior
to quenching. An encounter complex can be visualized as an intermolecular
resemble of an excited-state and ground-state molecule usually separated by a
small distance (7A0) and surrounded by several shells of solvent molecules
termed as the innermost shell solvent cage [40,47-48]. The structure of
encounter complex is affected by the size, shape and charges of the reactants
and by their interactions with the solvent cage. Excitation of the sensitizer
usually takes place before formation of the encounter complex. The events for
proceeding of formation of the encounter complex can be described by the
random walk hypothesis. According to this motion, molecules diffuse in
solution by a series of one-dimensional random steps [40]. If we apply this
concept to the formation of encounter complexes, we can envisage reactant
partners approaching one another in series of randomized zig-zag steps.
Eventually the molecules collide, separate and undergo further collisions.
A typical collision for an uncharged small organic molecule has duration
of about = 10-9
-10-10
second. Quenching pathways may take place within the
encounter complex depending upon the driving force of these reactions. During
the lifetime of an encounter complex, the reactants undergo structural (nuclear)
and electronic (orbital) changes. The vibrational fluctuations, which determine
the nuclear barrier of the pathway, have frequencies of 1012
s-1
.Thus the lifetime
of a typical encounter complex is usually of sufficient duration for rate-
determing nuclear changes to take place. Nuclear reorganization is a critical
aspect of electron transfer and must be considered when evaluation of the rate
limiting barriers of this quenching pathway is carried out.
CHAPTER – I Introduction
30
In quenching by electron transfer, if the transfer of an electron occurs
during the lifetime of the collision complex (i.e. when the reactant partners are
in contact), the charge-transfer species immediately formed in a “contact ion
pair” (CIP). The collision complex can also separate slightly, undergo electron
transfer and generate a “solvent-separated” ion pair (SSIP). Following electron
transfer solvent molecules rapidly stabilize contact ion pairs and solvent-
separated ion pairs. Thus, a contact ion pair may be “pried apart” by a solvent
molecule and be converted into a solvent-separated ion pair or vice-versa.
Contact ion pairs and solvent separated ion pairs are sometime described as
“germinate” ion pairs provided that each ionic partner is descendant of the
same parental pair. If solvent-separated ions dissociate into the bulk of the fluid
medium where they become separated by a large distance, they are classified as
free and solvated ions. These ionic species are completely independent of one
another analogous to stable free radical and can exist as distinct, randomized,
solvated and long-lived species.
1.8.2 Fluorescence quenching via exciplex:
Fluorescence quenching via exciplex is a particularly important pathway
when the reactants are planar organic molecules capable of forming
“sandwiched” complexes. If the interaction between the reactants, one of which
is electronically excited, is strong, and encounter complex can rapidly form an
intermediate which may have a sufficiently long life time to undergo light
emission. Such intermediates are termed exciplexes and are characterized by
strong binding energies (5.20 Kcal mol-1
), partial charge character on each
reactant molecules and large dipole moments which reflect the degree of
charge transfer [49-50]. Typically, an exciplex is a long-lived, relatively stable
and structured electronically excited species. Experimental support for
exciplexes is provided by the appearance of broad, structure less and long lived
emission, although absorption and chemical reactions may also be used for
characterization.
CHAPTER – I Introduction
31
A molecular orbital wave function representation is used to express the
electronic interaction in an exciplex as a summation of possible states
(wavefuntion) [51].
= C1 (D*A) + C2 (DA*) + C3 (D+ A
-) + C4 (D
- A
+) + C5 (DA)
where the coefficients pertain to the relative contribution of each state. If „A‟ is
exclusively an electron acceptor and if ground-state interactions are neglected,
equation 1.5 simplifies to
C1 (D*A) + C2 (DA*) + C3 (D+ A
-) ---------- (15)
If C3>>C2, the exciplex has pronounced charge-transfer character and will have
a tendency to dissociate into radical ion pairs, especially in polar solvents. In
the extreme case, an exciplex is more accurately described as a contact ion-
pair. Emission from exciplexes proceeds by a vertical, Franck-Condon allowed
transitions from a minimum on an excited state surface to a low-lying ground
state surface involve a significant nuclear change, the emission may not be
observed. Other decay processes, such as ionic dissociation into solvent-
separated radical ions or chemical reactions may prevail. Such a non-emitting
charge-transfer species is described as a “non-emitting” exciplex and has
properties similar to those of a contact ion-pair. For C3>>C2, exciplex
formation leads to energy transfer. In such a case, exciplexes tend to emit light
or undergo separation to form the excited state of the acceptor and ground state
of the donor.
1.9 Surfactants:
Surfactants are characterized by a hydrophilic charged „head‟ and a
hydrophobic hydrocarbon „tail‟. The most outstanding property of surfactants is
their tendency to form aggregates, the micelles, at sharply defined critical
micelle concentration (CMC). The micelles formed by ionic amphiphilic
molecules in aqueous solutions are dynamic association of surfactant molecules
that achieve segregation of their hydrophobic proteins from the solvent via self
assembly [52].
CHAPTER – I Introduction
32
The aggregation of single molecules of a certain type when dissolved in
water, to form a particle of colloid dimension called a micelle which is shown
in Fig.1.8. The molecules or monomers, which can take part in these processes,
are characterized by possessing two regions in their chemical structure. One is
hydrocarbon chain, the hydrophobic region of the molecule, and other is an
ionized group or water soluble group, the hydrophilic region of the molecules
e.g. Sodium lauryl sulphate.
Fig.1.8: Structure of micelle
The existence in one compound of two moieties, one of which has affinity for
the solvent and other is antipathetic to it, has been called amphipathy by Hartlet
[52]. This dual nature is responsible for the properties of micellization, surface
activity and solubilization. As a class, these substances, which include soaps
and detergents, can be called associate in solution forming particles of colloidal
dimensions. Due to their tendency to become adsorbed at interfaces, they are
often called surface-active agents or colloidal surfactants.
CHAPTER – I Introduction
33
1.9.1 Classification of surfactants:
From the commercial point of view surfactants are often classified
according to their use. The most accepted and scientifically sound classification
of surfactants is based on their dissociation in water.
1.9.2 Anionic surfactants:
Anionic surfactants are dissociated in water in an amphiphilic anion, and
a cation, which is in general an alkaline metal (Na+, K
+) or a quaternary
ammonium ion. They are the most commonly used surfactants. They include
alkylbenzene sulfonates (detergents), (fatty acid) soaps, lauryl sulfate (foaming
agent), di-alkyl sulfosuccinate (wetting agent), lignosulfonates (dispersants)
etc. Anionic surfactants account for about 50 % of the world production.
Sr. No Name Structure
1 Potassium laurate CH3(CH2)10COO- K+
2 Sodium dodecyl (lauryl)
sulphate
3 Hexadecylsulphonic acid CH3(CH2)15SO-3 H
+
4 Sodium
dioctylsulphosuccinate
1.9.3 Cationic surfactants:
Cationic surfactants are dissociated in water into an amphiphilic cation
and an anion, most often of the halogen type. A very large proportion of this
class corresponds to nitrogen compounds such as fatty amine salts and
quaternary ammonium salts with one or several long chain of the alkyl type,
often coming from natural fatty acids. These surfactants are in general more
expensive than anionic surfactants, because of the high-pressure hydrogenation
reaction to be carried out during their synthesis. As a consequence, they are
only used in two cases in which there is no cheaper substitute, i.e. (1) as
CH3(CH2)11SO-4 Na+
C8H17OOCHSO-3 Na+
C8H17OOCCH2
CHAPTER – I Introduction
34
bactericide, (2) as positively charged substance which is able to adsorb on
negatively charged substrates to produce antistatic and hydrophobic effect,
often of great commercial importance such as in corrosion inhibition.
Sr.
No
Name of Surfactant Structure
1 Hexadecyl (cetyl)trimethylammonium
bromide
CH3 (CH2) 13N+(CH3) 3 Br
-
2
Dodecylpyridium chloride N
+
C12H25Cl-
3
Dodecyl hydrochloride CH3(CH2)11NH3
+
1.9.4 Nonionic surfactants:
Nonionic surfactants account about 45% of the overall industrial
production. They do not ionize in aqueous solution, because their hydrophilic
group is of a nondissociable type, such as alcohol, phenol, ether, ester, or
amide. A large proportion of these nonionic surfactants are made hydrophilic
by the presence of a polyethylene glycol chain, obtained by the
polycondensation of ethylene oxide and they are called polyethoxylated
nonionics. In the past decade glucoside (sugar based) head groups, have been
introduced in the market, because of their low toxicity. As far as the lipophilic
group is concerned, it is often of the alkyl or alkylbenzene type, the former
coming from fatty acids of natural origin. The polycondensation of propylene
oxide produce a polyether which (in opposition to polyethylene oxide) is
slightly hydrophobic.
CHAPTER – I Introduction
35
Sr.
No.
Name of the surfactant Structure
1 Polyoxyethylene p-tertoctylphenyl
ether
C8H17C6H4O(CH2CH2O)10H
2. Polyoxyethylene monohexadecyl
ether
CH3(CH2)15(OCH2CH2)21OH
1.9.5 Zweterionic or Ampholytic surfactant:
This type can behave either as an ionic, non-ionic, or cationic species,
depending on the pH of the solution. When a single surfactant molecule
exhibits both anionic and cationic dissociations it is called amphoteric or
zwitterionic. This is the case of synthetic products like betaines or sulfobetaines
and natural substances such as amino acids and phospholipids.
1.9.6 The micellization process:
The most important property of amphipathic molecules or ions
characterized by a polar hydrophilic head and non-polar hydrocarbon tail is
their tendency to form large aggregates, the micelles, above a certain rather
sharply defined concentration. So micelle is defined as “a colloidal particle
together with its surrounding stabilizing agent” [50]. Surfactant molecules (e.g.
CTAB, SDS, Triton X-100, Brij – 35 etc.) self-aggregate into supramolecular
structure when dissolved in water or oil. The simplest aggregate of these
surfactant molecules is called a micelle, and dispersion of the aggregates in
water or oil is referred to as micellar solution [53-55]. A typical micelle has
size of 50 Å and is made of about 100 surfactant molecules [56]. The self-
association gives rise to rich variety of phase structure shown in Figure1.9.
Aggregation is not only limited to aqueous solution but also it is some time
observed in non-aqueous polar solvents such as ethylene glycol and non-polar
solvents such as hexane [57].
CHAPTER – I Introduction
36
1.9.7 Solubilization of organic compounds:
Self-association property of surfactants to form self-assembled
aggregates, the micelles, in an aqueous medium has a profound effect on the
solubility of the some organic substances (additives) which are otherwise
sparingly soluble in water [58-59]. Solubilization by micelles is of importance
in many industrial processes such as detergency, emulsion polymerization, oil
recovery, etc. and in a variety of fundamental research oriented polymerization
like micellar modeling of biological membranes [60].
The solubilization can be ascribed to incorporation of hydrophobic
substance in to micelle in solution of surfactant. Solubilization has been treated
as partitioning of additive molecules (solubilizates) between a micellar phase
and intermicellar bulk phase [61-63]. The partitioning behavior of
solubilization between intermicelle bulk phase and micellar phase is an
indication of the hydrophilic – lyophilic balance of the molecule. It has been
discussed that the affinity of water for the solubilizates is important in
partitioning [64] due to water dragging effect where the water is carried as a
shell around the solubilizate. The partition coefficient is dependent on the
structure of solubilizate and the surfactant that constitutes the micelles.
In addition to the solubilization equilibrium, the micro viscosity of the
micellar interior and location of the solubilizate within the micelles is also
important in many applications of micellar solubilization. The physical
behavior of the surfactant micelles can be visualized as the construction of
model membrane to biological surface with the solubilizate, drug carrier and
drug release [65-66].
1.9.8 Mechanism of solubilization:
Solubilization is believed to occur at five sites in the micelle as shown in
Scheme-III.
1. the surface of the micelle at the micelle solvents interface
2. between the hydrophilic head group
CHAPTER – I Introduction
37
3. palisade layer of the micelle between the hydrophilic ground and the
first few carbon atoms of the hydrophobic groups that comprise the
outer core of the micellar interior.
4. more deeply in the palisade layer
5. in the inner core of the micelle
Ionic micelles ordinarily have an extensive hydrophobic core region,
which can interact strongly with hydrocarbon and halogenated hydrocarbons of
solutes. Hydrophobic effects have often been considered to be dominating in
determining the locus of solubilization [67-68]. Surfactant micelles can be
pictured as having a highly nonpolar interior and a relatively polar interfacial
region. Therefore nonpolarized or easily polarizable compounds are solubilized
in aqueous medium in the inner core of the micelle between the ends of the
hydrophobic groups of the surfactant molecules. Polarized hydrocarbons are
solubilized by absorption at the micelle-water interface and by replacing water
molecules that may penetrate the core of the micelle close to the polar heads,
but solubilization of additional material is deep in the palisade layer as located
in the inner core of micelle [59]. The polarizability of the π electron cloud of
the aromatic nucleus and its consequent ability to interact with the positively
charged groups at the micelle water interface may account for the initial
adsorption of these hydrocarbons in that location [69].
Scheme-III
CHAPTER – I Introduction
38
1.10 Applications:
1.10.1 PET in synthetic organic chemistry:
The photoinduced electron transfer reactions are of interest to
photochemists to understand the generation of charge transfer intermediates
and stable products when donor and acceptor molecules are placed close in
suitable solvents. Many reactions photosynthesized by electron transfer were
investigated and studied thoroughly to know mechanism and probable
products.
1.10.1.a Reaction of alkanes:
The most clear cut examples of electron transfer phtosensitizers are
those involving electron deficient sensitizers and electron rich olefins. The
radical cations generated from these reactions have been shown to undergo
polymerization, dimerizations, cross cycloaddition, nucleophilic substitution
and isomerization [70-72].
1.10.1.b Bond cleavages, ring opening’s elimination and isomerization:
Strained cyclic organic molecules are efficient quenchers of excited
states. These reactions frequently involve electron transfer. Some examples are
photolysis of methanolic solutions of tricyclo heptanes and 1-cyanonaphthalene
leads to CH3OH addition [73]. Sensitized bond cleavage reactions of 1,2-diaryl
ethanes and aryl pinacols have been reported [74].
1.10.1.c Valence isomerization:
The rearrangement of n-bornadiene to the richer quadricyclane and the
reverse reaction can take place on photolysis in polar solvents in the presence
of electron deficient photosensitizers [75]. Electron transfer from valence
isomer to the excited states of electron deficient senzitizer is supported by
thermodynamic consideration. In the presence of singlet and triplet sensitizer,
the ring opening of quadricyclane displays a significant solvent dependence
[76].
CHAPTER – I Introduction
39
1.10.1.d Photo-oxygenations:
Photo-oxygenations have been considered to proceed via energy transfer
quenching, involving sensitization of oxygen by sensitizer triplet to form
excited singlet oxygen, which is reactive intermediate. A typical example
involves the oxygenation of electron rich olefins conjugated to aromatic
moieties with electron deficient sensitizers for example 9,10-dicyanoanthracene
[77]. The search for new photosensitizer would be always of novel applications
to synthetic organic chemistry.
1.10.1.e Photo-reduction of dyes by electron transfer processes:
Photo reduction is observed for some dyes in which the dye appears to
be bleached in light. In such reduction processes two „H‟ atoms (two electrons
and two protons) are added to the dye molecule D.
D + RH2 DH2 + R
The photo-reaction goes against the thermochemical gradient and
reverses spontaneously in the dark. The most important example of such
reactions is the photosynthesis in the plants. The light absorbed by the
chlorophyll molecules promotes an electron energetically to excited state.
Thus, provides the driving force for the primary processes. Such a
photosynthetic process occurring in the plants can be developed in the
laboratories. The operation of artificial photosynthetic devices depends mainly
on photoinduced electron transfer processes (PET) and hence PET reactions are
of immense importance in this context [78].
1.10.1.f Photo-oxidation reactions by electron transfer:
Photo-oxidation reactions in absence of molecular O2 are better
described as photochemical oxidation-reduction reaction in which an electron
transfer will occur between donor and acceptor. Photo redox reactions can be
mediated by an intermediate, which is called as sensitizer acts as photo catalyst
h
CHAPTER – I Introduction
40
in more generation sense. Thus, the photoinduced electron transfer reactions
are significantly broadened the scope of organic photochemistry.
1.10.2 PET systems as sensors:
Upon excitation the luminophores, especially those with groups held
outside but close to the -electron systems of the luminophore, show an
increased susceptibility to redox reactions. Knowledge of the redox potential of
their reactions can be used to tailor PET processes that can be switched on or
off. In the off state, the excited state energy must be bigger than that require to
oxidize the receptor and to reduce the fluorophore. Thus, allowing PET from
receptor to fluorophore. In the on state, a cation in the receptor cavity raises to
oxidation potential, causing the thermodynamic condition for PET to be
removed and fluorophores to undergo emission. A sensor molecule when
subjected to light energy, an electron is transferred from the receptor to
fluorophore, taking energy from its excited state and rendering the system non-
luminescent. However, if the receptor traps a guest, its lone pair of electrons
becomes bound up, electron transfer does not occur and the excited state
energy of the system is released as emission from the fluorophore [79].
1.10.3 Molecular Information Processors:
Molecular information processor is an interesting device based on PET
and consists YES, NOT AND or XOR and other logic gates. The use of
chemical input and photonic output is developing field of research. For
example, a YES gate molecule is one that fluoresces in the presence of H+ and
a NOT gate molecule is one whose fluorescent emission disappears when H+
is
added. This is an important area of research and it is now obvious that this type
of work hold out the potential for molecular computers and neutral networks
using photon mode input.
CHAPTER – I Introduction
41
1.10.4 Qualitative and quantitative applications of PET:
PET reactions are of significance in the fields of chemistry and biology.
Extensive theoretical and experimental studies in homogeneous media and
organized assemblies have been done for more than a couple of decades for the
better understanding of PET reactions. PET is used for spectroscopic detection
of biomolecules, drugs and nucleic acids and also to understand molecular
interactions between them. The detection methods involved use of fluorescent
probe whose intensity is quenched regularly by photoinduced electron transfer
between ground state quencher to excited fluorescent probe. The gradual
quenching of fluorescence of probe as a function of concentration of quencher
enabled to establish quantitative relation between extent of quenching of
fluorescence and concentration of quencher that is an analyte. The earlier
spectroscopic methods involved separation of an analyte from other
components or impurities and its detection based on Beer‟s law in direct
absorption methods and in direct fluorimetric methods. These methods are
laborious and require that the analyte should be fluorescent. The electron
donor-acceptor pair should be such that donor should be capable to donate
electron i.e. easily oxidisable and other reducible by accepting the electron
from donor.
1.11 Literature survey on PET process:
Photoinduced intermolecular electron transfer interaction between
coumarin dyes and aromatic amines has been investigated in sodium dodecyl
sulphate micellar solutions using steady state and time resolved fluorescence
quenching measurements [80]. In the time-resolved fluorescence
measurements, the analysis of the fluorescence decays following a micellar
quenching kinetics model assuming a unified quenching constants (kq) per
quencher occupancy does not give satisfactory results especially for the higher
quencher concentrations used. The correlation of the observed kq values in the
micellar solutions with the free-energy changes ( G0) for electron transfer
CHAPTER – I Introduction
42
reactions show an inversion in the observed rates as predicted by Marcus outer
sphere electron transfer at exergonicities more than 0.65eV are discussed [80].
Photoinduced electron transfer between octadecyl-rhodamine B (a hole donor)
and N, N-dimethyl -l-naphthylamine (hole acceptor), located in the head group
region of sodium dodecyl sulfonate micelles, has been examined for different
acceptor concentrations using time resolved fluorescence. The experimental
results were analysed using the Marcus distance-dependent transfer rate
modified to take into account the heterogeneous nature of micelles. Diffusion
of the donor or acceptor is included in the theoretical analysis and the results
are compared with earlier experiments involving the same donor-acceptor
combination but in a different type of micelles [81].
Torimura et al. studied the fluorescence quenching by photoinduced
electron transfer between various fluorescent dyes and nucleobases. In these
systems nucleobases are used as electron donors. Appropriate donor-acceptor
pair was selected from electrochemical data obtained by cyclic voltammetry.
The quenching experiments were performed by keeping concentration of
acceptor to some constant value and varying that of donor in aqueous solutions
[82].
S.P.Wu et al. studied the fluorescence quenching study on the
interaction of bases of nucleic acid with electron accepting sensitizer and serum
albumin containing electron rich tryptophan residue. The fluorescence
quenching data shows that nitrogen bases act as effective electron donors to
quench the fluorescence of electron-accepting sensitizers. The quenching by
diffusion-controlled rate coincided well with the static and dynamic Stern-
Volmer correlation. The free energy changes for photo induced electron
transfer process were also investigated [83].
Z.P. Du et al. reported the experimental study on the photo interaction
between sanguinarine and guanosine by using UV-visible and fluorescence
spectroscopy. The binding of sanguinarine to guanosine was substantiated by
the hypochromism and bathochromism in the absorption spectra and the
emission quenching in fluorescence spectra. These spectral features strongly
CHAPTER – I Introduction
43
support the interactions of sanguinarine with guanosine. The thermodynamic
data for the sanguinarine binding to guanosine were also calculated .The results
show that the binding of sanguinarine to guanosine is not only exothermic but
entropy driven [84]. Similarly X.Zhang et al. reported a spectral study of the
interaction between chelerythrine chloride and adenosine by UV-visible
spectrophotometric and spectrofluorimetric measurements and calculated the
thermodynamic parameters [85].
B. Chakraborty et al. studied the interaction of proflvin with
triethylamine in homogeneous and micellar media and photoinduced electron
transfer probed by magnetic field effect. The two prime phenomena were
explored in this study are photoinduced electron transfer (PET) and ground –
state complex formation. The experimental result shows that it is the medium,
which determines the reaction pathways to be followed. Magnetic field effect
helps to elucidate the reaction mechanism involved in this system [86].
Neeti Singh et al. reported spectrophotometric study of the charge
transfer complexation of picric acid as an electron acceptor with p-nitroaniline
as an electron donor in three different organic solvents. The results were
discussed in terms of association constant (kct), molar extinction coefficient
( ct), standard free energy ( G0), oscillator strength (f), and transition dipole
moment ( EN). The results reveal that the interaction between the donor and
acceptor is due to - * transitions. The stoichiometry of the complexes was
found to be 1:1 due to linear relationship between donor and acceptor [87].
A. Chakraborty et al. investigated the PET between different coumarin
dyes and N, N-dimethyl aniline in AOT reverse micelle using steady state and
time resolved fluorescence spectroscopy. The fluorescence quenching data
shows that slower electron transfer rate in reverse micelle in comparison to that
in the neat solvent. It was observed that the retardation in the ET rate in the
correlation of the free energy change with the ET rate [88].
F. Yu et al. developed a new spectrofluorimetric method for
determination of adenosine disodium triphosphate (ATP). The interactions
between prulifloxacin (PUFX)-Tb3+
complex and ATP has been studied by
CHAPTER – I Introduction
44
using UV-visible absorption and fluorescence spectra using these pairs as
fluorescence probe, under the optimum conditions. ATP can remarkably
enhance the fluorescence intensity of the complex and enhanced fluorescence
intensity is in proportion to the concentration of ATP. The dynamic range and
detection limit of ATP was investigated [89].
1.12 Aim and scope of the present work:
The fluorescence quenching phenomenon first described over 50 years
ago and since then being used more and more in biomedical research. It is well
established that physico-chemical interactions between the components of
nucleic acids such as nitrogen bases, nucleosides, nucleotides and fluorescent
probe resulting into the strong fluorescence quenching of the latter, have been
the focus of extensive recent research. Several mechanisms appear to operate in
such systems namely quenching due to chemical reaction, quenching involving
electronic energy transfer, quenching due to the heavy atom and quenching
processes proceeding via charge transfer interaction. Photoinduced electron
transfer (PET) appears to be the most likely mechanism of quenching since the
redox potentials are of the appropriate magnitudes for polycyclic aromatic
fluorescent probe and nucleic acid couples. This mechanism is of intrinsic
interest because it takes place in aqueous or partially aqueous environment and
thus providing opportunities for studying the effects of hydrophobic
interactions, hydrogen bonding, and proton transfer coupled to PET
fluorescence quenching phenomenon.
The components of nucleic acids have an important function in life
process, so study on them has become an important research field of life
science. Quantitative determination of nucleic acid is required in many fields,
such as molecular biology, biotechnology and medical diagnosis. The natural
fluorescence intensity of nucleic acids is so weak that the direct use of their
fluorescence emission properties is limited. Therefore, to study the components
of deoxyribonucleic acid (DNA) and ribonucleic acid (RNA) using the
fluorescence method an extrinsic fluorescent probe should be introduced.
CHAPTER – I Introduction
45
Different probes react with nitrogen bases, nucleosides and nucleotides in
different ways, DNA and RNA molecules are known to enhance the
fluorescence intensity and also to quench the fluorescence of some of the
probes such as Ethidium bromide, sanguinarine, chelerythrine chloride,
proflavine, pyrene, coumarine etc. which are reported in literature. DNA and
RNA are composed of the components like nitrogen bases, nucleosides and
nucleotides. Adenine, guanine, uracil, thymine and cytosine are the nitrogen
bases. Adenosine, guanosine, uridine and cytidine are nucleosides while
adenosine 5‟ monophosphate (AMP), guanosine 5‟ monophosphate (GMP) and
uridine 5‟ monophosphate (UMP) are the nucleotides. Many of these
biomolecules constituting nucleic acids are of pharmaceutical importance.
Uracil is used for drug delivery and in the body it helps to carry out the
synthesis of many enzymes necessary for cell functions. Its derivatives 5-fluoro
uracil and 5-methyl uracil are known to be antiviral, anticancer drugs. These
materials are weakly photosensitive and fluoresce too low to detect in direct
methods of analysis. Therefore in present work attempts were made to have
systems in which uracil and its derivatives bind with fluorescent 9-anthracene
carboxylic acid (9-ANCA) probe and form charged pairs in aqueous medium.
Such pairing was expected to form charge transfer state upon excitation and
may results in quenching of fluorescence of probe molecule. The possibility of
binding between these molecules was examined by electrochemical studies of
such pairs which helped further to consider photoinduced electron transfer
(PET) from nitrogen base molecules to the fluorescent probe.
Similarly, AMP, GMP and UMP are the structural units of the nucleic
acids used as drugs. AMP is an intermediary substance formed during the
body‟s process of creating energy in the form of adenosine triphosphate (ATP)
from food. The body creates AMP within cells during normal metabolic
processes. It has medicinal importance and its injection available commercially
is used in post therapeutic neuralgia treatment. In brain research studies UMP
is used as a convenient delivery compound for uridine. The present work aimed
to develop fluorimetric method for analysis of these molecules by using 9-
CHAPTER – I Introduction
46
ANCA. The direct molecular interaction between 9-ANCA and nucleotides is
not possible as both being isoelectronic. The cationic surfactant such as cetyl-
trimethyl ammonium bromide (CTAB) is known to solubilize, stabilize the
drugs and DNA, RNA molecules of opposite charges and may result in several
desirable or undesirable interactions. Hence possible electrostatic interactions
between the pairs of 9-ANCA-CTAB and CTAB-nucleotides are used to
develop a new fluorimetric method for analysis of nucleotides from aqueous
solution and applied successfully for pharmaceutical samples containing
nucleotides. The possible electrostatic interactions between these pairs were
examined by conductometric studies. In addition to 9-ANCA, perylene
solubilised in CTAB was found to be suitable probe for detection of these
biomolecules by using PET.
The nucleoside like adenosine used as anti-inflammatory agent also
undertaken in PET studies with proflavine hemi sulphate (PF). The ground
state charge transfer complex formation was observed by absorption and
fluorescence studies.
Studies on photophysical properties of fluorescent organic materials in
aqueous solution were performed. The materials such as 9-ANCA, perylene
and PF were tested for photoabsorption and emission performance with a view
to use as probe and to develop analytical techniques for determination and to
understand the molecular interaction with DNA and RNA molecules. The
spectral data obtained would found useful in deciding the donor (components
of DNA and RNA) and acceptor (fluorescent probe) pairs for PET studies
which are satisfying basic condition required for the electron transfer process.
The PET experiments are planned in aqueous and micellar solutions to examine
optimum conditions. Attempts were made to verify Stern-Volmer relation and
thus to determine the binding parameters to understand molecular interaction
between donor and acceptor. Thus, studies carried on different electron donor –
acceptor pairs would found useful in developing new analytical methods for
detection as well as to understand the molecular interaction based on PET.
CHAPTER – I Introduction
47
1.13 References:
1. D. R. Vij, Luminescence of solids, Plenum Press, New York, (1998)
2. E. Widemann and G. C. Schmidt, Ann. Physik, 56 (1895) 18.
3. H.V. Laverenz, An introduction to Luminescence of Solids, Dover
Publications, Inc. New York, (1968) 90.
4. C.A. Parker, in Photoluminescence of Solution, Elsevier Publication,
Amsterdam, (1968) 21.
5. J. B. Coon, R. E. Wames and C. M. Loyd, Journal of Molecular
Spectroscopy, 8 (1-6) (1962) 285.
6. L. Earl, Wehry, Handbook of Instrumental Techniques for Analytical
Chemistry, University of Tennesses Department of Chemistry
7. R. T. Williams and J. W. Bridjes, J. Clin. Path, 17 (1964) 371.
8. K. K. Rhohatgi-Mukharjee, Fundamental‟s of Photochemistry, (1988)
9. A.Albert, J.Chem. Soc., (1960) 1020.
10 J. R. Lakowiez, Principles of Fluorescence Spectroscopy, 3rd
Edition
(2006).
11. S. S. Deshpande, Critical Reviews in Food Science and Nutrition, 41 (3)
(2001) 155
12. J. Andersson, F. Puntoriero, S. Serroni, A. Yartsev, T. Pascher, T Polı,
S. Campagna and V. Sundström, Chemical Physics Letters, 386 (4-6)
(2004) 336.
13. B. Valeur, Molecular Fluorescence: Principles and Applications,
WILEY –VCH, (2001)
14. J. W. Bridges, Ph.D. Thesis, University of London (1963).
15. Analytical letters, 38 (2005) 1367.
16. S. Quan, F. Teng, Z. Xu, L. Qiun, Y. Hou, Y. Wang and X. Xi,
European Polymer Journal, 42 (1) (2006) 228.
17 S. Undenfriend, Fluorescence Assay in Biology and Medicine Academic
press, New York, (1962)
18. B. L.Van Duuren, Chem. Rev, 63 (1963) 325.
19. J. W. Bridges, P. J. Creavan and R. T. Williams, Published data (1963)
CHAPTER – I Introduction
48
20. K. T. Williams, J. Roy, Insti. Chem. 83 (1959) 611
21. J. R. Platt, J. Chem. Phys. 17 (1949) 484.
22. T. Forster and K. Kasper, Z. Electrochem. 1 (1954) 275.
23. H. Kuhn, D. Mobius and H. Bucher, in Techniques in Chemistry, Vol.I,
Part IIIB, Wiley Interscience, New York (1972) 577.
24. I. B. Berlman, Handbook of Fluorescence of Aromatic Molecules,
Academic Press, New York and London, (1971)
25. J. B. Birks and J. E. Dyson, Proc. Roy. Soc. 275 A (1963) 135.
26. D. Chris, M. Geddes, Sci. Tenchnol. 12 (2001) 53.
26. G. C. Pimentel, J. Am. Chem. Soc.79 (1957) 3323.
27. G. C. Pimentel, and A. L. Meclellan, “The Hydrogen Bond‟‟,
W. H. Freeman and Company, San Francisco and London (1960)
29. T. Lasson, M. Wedborg and D.Turner, Analytical Chemica Acta, 583
(2007) 357.
30. H. M. Zhang, X. Q. Guo, Yi. B. Zhao, D. Y. Wang and J. G. Xu,
Analytical Chemica Acta, 361(1-2) (1998) 9.
31. E. J. Bawen and F. Wokes, Fluorescence of Solutions, Longmans,
Green, London (1953).
32. T. Effio, U. P. Trociewitz, X. Wang and J. Schwartz, Superconductor,
Sci. Technology, 21 (2008) 1.
33. M. Kastantin, B. Ananthanarayanan, P. Karmali, E. Ruoslahti and M.
Tirrell, Langmuir, 25 (13) (2009) 7279.
34. H. Lu, O. Schops, U. Woggon, and C. M. Niemeyer, J. Am. Chem. Soc.
130 (2008) 4815.
35. S. L. Bhatter, G. B. Kolekar, S. R. Patil, J. of Luminescence, 128 (2008)
306.
36. V. R. More, U. S. Mote, S. R. Patil, G. B. Kolekar, Spectrochimica Acta
Part A, 74 (2009) 771.
37. P. Hartmann, J. P. Leiner. M. E. Lippitsch, Journal of Fluorescence,
4 (4) (2005) 327.
CHAPTER – I Introduction
49
38. P. K. Behera, T. Mukherjee and A. K. Mishra, Journal of Luminescence,
(3) (1995) 131.
39. B. Valeur, Molecular Fluorescence, Principles and Applications,
WILEY-VCH, (2001).
40. N. J. Turro, “Modern Molecular Photochemistry”, Benjamin/Cummings,
Menlo Park, Chapter 9, (1978).
41. D. L. J. Dexter, Chem. Phys, 21 (1953) 836.
42. T. Forster, Faraday Discuss, Chem. Soc. 7 (1959) 27.
43. N. J. Turro, J. C. Dalton and D. C. Weiss, “Organic Photochemistry”,
Chapman, O.L. Ed, Marcel Dekker, New York, 2 (1969) 1.
44. L. Stryer and R. P. Haugland, Proc. Natl, Acad. Sci, U.S.A. 58 (1967)
719.
45. H. Leonhardt and A. Weller, Ber. Bunsenges, Phys. Chem. 67(1963)
791.
46. T. Forster, “The Exciplex”. M. A. Gordon, W. R. Ware, Eds, Academic,
New York (1975) 1.
47. J. W. Moore and R. G. Pearson, “Kinetics and Mechanism, Wiley-New
York (1981) 257.
48. R. D. Cannon, “Electron Transfer Reactions”, Butterworth‟s, London
(1980) 97.
49. Y. Sigintuya and S. Vamamoto, Journal of Photochemistry and
Phtobiology A: Chemisty, 186 (2007) 41-46.
50. W. Baumann, H. Bischof, J. Frohling, J. Lumin. 25 (1981) 555.
51. M. Ottolenghi, Acc. Chem. Res. 6 (1973) 153.
52. a. M. Jayne Lawrence. Chem. Soc. Rev. 23 (1994) 417.
b. www.drdorights.com/science.php
53. C. Tanford, The Hydrophobic Effect: Formation of micelles and
Biological Membranes, Wiley, New York, (1973).
54. V. Degiorgio, and M. Corti, (Eds), Physics of Amphiphiles: Micelles,
Vesicles and Microemulsion, Nort Holland, Amsterdam, (1985).
55. Y. Chevalier and T. Zemb, Rep. Prog. Phys. 53 (1991) 279.
CHAPTER – I Introduction
50
56. S. P. Moulik, Curr. Sci. 71 (1996) 368.
57. Y. Chevalier and T. Zemb, Rep. Prog. Phys.53 (1990) 279.
58. P. Mukherjee, and K. L. Mittal (ED) “Solution Chemistry of
Surfactant”, Vol.1, Plenum press, New York, (1979) 153.
59. P. H. Elworty, A. T. Florence and C. B. Macfarlane, “Solubilization by
Surfactant-Active Agents”, Chapamnn and Hall, Landon (1968).
60. J. H. Fendle, “Membrane Mimetic Chemistry” Wiley-Inter-Science,
New York (1982).
61. E. Lissi, E. Abiun and A. M. Rocha, J. Phys. Chem. 84 (1980) 2406.
62. C. A. Bunton and L. Seppulveda, J. Physical. Chem. 83 (1979) 80.
63. G. A. Smith, S. D. Christian, E. E. Tucker and J. F. Scmhorn, J. Colloid
Interfcae. Sci. 130 (1989) 254.
64. R. S. Tsai, W. Fan, N. El Tayer, P. A. Carrupt, B. Testa and L. B. Kier.,
J. Am. Chem. Sci. 115 (1993) 9632.
65. Y. Kushumoto and H. Sato, Chem. Phys. Lett. 68 (1979) 13.
66. H. Satoh, Y. Kusumoto, N. Nakashima, and K. Yoshihara, Chem.
Phys. Lett, 71 (2) (1980) 326.
67. Y. Moroi, K. Sato, and R. Motuura, J. Phys. Chem. 86 (1982) 2463.
68. R. Zana , Adv. Colloidal Interface. Sci. 57 (1995) 1.
69. T. Nakagawa, and M. J. Schick “Nonionic Surfactants” Dekker, New
York (1967).
70. R. A. Marcus and N. Sutiri, Biochim, Biophys, Acta. 811 (1985) 265.
71. S. L. Mattes and S. Farid, J. Am. Chem. Soc. 105 (1983) 1386.
72. S. L. Mattes, S. Farid, “Organic Photochemistry,” Padwa A. Ed. Marcel
Dekker, New York, 6 (1983) 233.
73. P. G. Gassman, K. D. Olson, L. Water, R. Yamaguchi, J. Am. Chem.
Soc. 103 (1981) 4977.
74. L. W. Reichel, G. W. Griffin, A. J. Muller, P. K. Das, Can. J. Chem.
62 (1984) 424.
75. H. D. Roth, M. L. Schilling, J. Am. Chem. Soc. 103 (1981) 7210.
76. G. I. Jones, S. H. Chiang, W. G. Becker, J. A. Welch, J. Phys. Chem.
CHAPTER – I Introduction
51
86 (1982) 2805.
77. J. Erilseni, C. S. Foote, J. Am. Chem. Soc. 102 (1980) 6083.
78. S. Dileesh and K. R. Gopidas, Journal of Phtochemistry and Phtobiology
A: Chemistry 162 (2004) 115.
79. J. Nicholas Turro, WEN – Sheng Chung and M. O. Kamoto,
Photobiology A: Chemistry, 45 (1988) 17.
80. M. Kumbhakar, S. Nath, H. Pal, A.V. Sapre and T. Mukherjee, Chem.
Phys. 119 (2003) 388.
81. J. Nanda, P.K. Behra, H. L.Tavernier, M. D. Fayer, J. of Luminescence
115 (2005) 138.
82. M. Torimura, S. Kurata, K. Yamada, T. Yokdmuka, R. Kurane, Ana.
Sci.17 (2001) 155
83. S. Wu, B. Ding, J. Wu and Z. Jiang Res. Chem. Intermed. 26 (7, 8)
(2000) 727.
84. Z. P. Du, Q. L. Suo, X. Y. Zhang, L. W. Zhang, X.H. Wei, Chinese
Chemical Letters 19 (2008) 1465.
85. X. Zhang, Q. Suo, Spectroscopy Letters, 40 (2007) 615.
86. B. Chakraborty, S. Basu, Chemical Physics Letters, 477 (2009) 382.
87. N. Singh and A. Ahmad Canadian Journal of Analytical Science and
Spectroscopy, 54 (1) (2009) 11.
88. A. Chakraborty, D. Seth, D. Chakraborty, P. Hazra, N. Sarkar, Chemical
Physics Letters, 405 (2005) 18.
89. F. Yu, L. Li, F. Chen, Analytica Chimica Acta, 610 (2008) 257.