pranita kore
TRANSCRIPT
JSPM’s Charak College of Pharmacy & Research,
GAT No.720/1&2,WAGHOLI, Pune-NAGAR ROAD,PUNE-412 207
Theory of U.V Spectrophotometry
Presented By, Guided By, Miss. Pranita Kore Dr. Rajesh J Oswal
Prof.Sandip Kshirsagar
Department Of Pharmaceutical Chemistry
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Introdution
Electronic Transition’s
Chromophores
Auxochromes
Beer’s-Lambert Law
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Content’s of U.V Spectrophotometry
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I.IntroductionA.UV radiation and Electronic Excitations:
1.The difference in energy between molecular bonding, non-bonding and anti-bonding orbitals ranges from 125-650 kJ/mole
2.This energy corresponds to EM radiation in the ultraviolet (UV) region, 100-350 nm, and visible (VIS) regions 350-700 nm of the spectrum
3.For comparison, recall the EM spectrum:
4.Using IR we observed vibrational transitions with energies of 8-40 kJ/mol at wavelengths of 2500-15,000 nm
5.For purposes of our discussion, we will refer to UV and VIS spectroscopy as UV
g-rays X-rays UV IR Microwave Radio
Visible
Introduction B. Band Structure
6. When these energy levels are superimposed, the effect can be readily explained – any transition has the possibility of being observed
Energy
Vo
V4
V3
V2
V1
Disassociation
R1 - Rn
R1 - Rn
R1 - Rn
R1 - Rn
R1 - Rn
Vo
V4
V3
V2
V1
Disassociation
R1 - Rn
R1 - Rn
R1 - Rn
R1 - Rn
R1 - Rn
E1
E0
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II. Electronic transitions
The absorption of UV or visible radiation corresponds to the excitation of outer electrons.
There are two types of electronic transition which can be considered; 1.Transitions involving p, s, and n electrons 2.Transitions involving charge-transfer electrons
When an atom or molecule absorbs energy, electrons are promoted from their ground state to an excited state. In a molecule, the atoms can rotate and vibrate with respect to each other. These vibrations and rotations also have discrete energy levels, which can be considered as being packed on top of each electronic level.
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Absorbing species containing p, s, and n electrons
Absorption of ultraviolet and visible radiation in organic molecules is restricted to certain functional groups (chromophores) that contain valence electrons of low excitation energy.
The spectrum of a molecule containing these chromophores is complex.
This is because the superposition of rotational and vibrational transitions on the electronic transitions gives a combination of overlapping lines.
This appears as a continuous absorption band.
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Possible electronic transitios of p, s, and n electrons are;
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s -s* Transitions
An electron in a bonding s orbital is excited to the corresponding antibonding orbital. The energy required is large.
For example, methane (which has only C-H bonds, and can only undergo s -s* transitions) shows an absorbance maximum at 125 nm. Absorption maxima due to s - s* transitions are not seen in typical UV-Vis. spectra (200 - 700 nm)
n -s* Transitions
Saturated compounds containing atoms with lone pairs (non-bonding electrons) are capable of n - s* transitions.
These transitions usually need less energy than s - s * transitions. They can be initiated by light whose wavelength is in the range 150 - 250 nm. The number of organic functional groups with n - s* peaks in the UV region is small.
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n - p* and p - p* Transitions
Most absorption spectroscopy of organic compounds is based on transitions of n or p electrons to the p* excited state.
This is because the absorption peaks for these transitions fall in an experimentally convenient region of the spectrum (200 - 700 nm).
These transitions need an unsaturated group in the molecule to provide the p electrons.
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III. ChromophoresA. Definition
1. Remember the electrons present in organic molecules are involved in covalent bonds or lone pairs of electrons on atoms such as O or N
2. Since similar functional groups will have electrons capable of discrete classes of transitions, the characteristic energy of these energies is more representative of the functional group than the electrons themselves
3. A functional group capable of having characteristic electronic transitions is called a chromophore (color loving)
4. Structural or electronic changes in the chromophore can be quantified and used to predict shifts in the observed electronic transitions
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III. Chromophores
B. Substituent Effects:
General – from our brief study of these general chromophores, only the weak n p* transition occurs in the routinely observed UV
The attachment of substituent groups (other than H) can shift the energy of the transition
Substituents that increase the intensity and often wavelength of an absorption are called auxochromes
Common auxochromes include alkyl, hydroxyl, alkoxy and amino groups and the halogens
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III. Chromophores
C. Substituent Effects
General – Substituents may have any of four effects on a chromophore
i. Bathochromic shift (red shift) – a shift to longer l; lower energy
ii. Hypsochromic shift (blue shift) – shift to shorter l; higher energy
iii. Hyperchromic effect – an increase in intensity
iv. Hypochromic effect – a decrease in intensity
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Hyperc
hro
mic
Bathochromic
Hypoch
rom
ic
Hypsochromic
700 nm200 nm
e
Fig: Absorption & intensity shifts04/13/2023 13
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IV. Auxochromes
The color of a molecule may be intensified by groups called auxochromes which generally do not absorb significantly in the 200-800nm region, but will affect the spectrum of the chromophore to which it is attached.
The most important auxochromic groups are OH, NH2, CH3 and NO2 and their properties are acidic (phenolic) or basic.
The actual effect of an auxochrome on a chromophore depends on the polarity of the auxochrome, e.g. groups like CH3-,CH3CH2- and Cl- have very little effect, usually a small red shift of 5-10nm. Other groups such as -NH2 and -NO2
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cuvette
source
slit
detector
V. Beer-Lambert law
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The method is most often used in a quantitative way to determine concentrations of an absorbing species in solution, using the Beer-Lambert law:
A=log10 (I0/I)=ε.C.L
Where, A is the measured absorbance,
I0 is the intensity of the incident light at a given wavelength,
I is the transmitted intensity, L the pathlength through the sample, and
c the concentration of the absorbing species.
For each species and wavelength, ε is a constant known as the molar absorptivity or extinction coefficient.
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