Uv spectroscopy

24,262 views 37 slides May 18, 2018
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About This Presentation

PRINCIPLE, INSTRUMENTATION AND SPECTRAL CHARACTERIZATION BY UV SPECTROSCOPY


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UV-VISIBLE spectroscopy T.Y.B.Pharm

Spectroscopy   is the study of the interaction between matter and electromagnetic radiation.  spectroscopy originated through the study of  visible light dispersed according to its wavelength, by a prism. Later the concept was expanded greatly to include any interaction with irradiative energy as a function of its wavelength or frequency. 

The word spectroscopy implies that we will use the electromagnetic spectrum to gain information about organic molecules. The other name of UV (Ultra-Violet) spectroscopy is Electronic spectroscopy as it involves the promotion of the electrons from the ground state to the higher energy or excited state. ultraviolet means that the information will come from a specific region of the electromagnetic spectrum called the ultraviolet region. The electromagnetic spectrum includes all radiation that travels at the speed of light c (3 x 10 10 cm/sec). The electromagnetic spectrum includes radio waves, which have long wavelengths, x-rays , which have short wavelengths, and visible light, which has wavelengths between those of radio waves and x-rays.

x-rays are most energetic , visible light next, and radio waves least energetic . Thus, the shorter the wavelength , the greater the energy of an electromagnetic wave. The heat excites some ground-state electrons to higher energy levels, then when the electrons “fall” back to the ground state, they “emit” energy that corresponds to the energy difference between the energy states ( orbitals ) where the electrons are found

The UV-Vis Spectrometer The basic idea behind  UV-Vis Spectroscopy  is to shine light of varying wavelengths through a sample and to  measure the absorbance at each wavelength . Only the wavelengths corresponding to the ΔE for an electronic transition will be strongly absorbed. A UV-Vis spectrum plots absorbance (or its inverse, transmittance) of the sample versus wavelength 

Here’s the spectrum for ethene . [In this case the wavelength is plotted versus  transmittance , the inverse of absorbance (high absorbance = low transmittance, and vice versa). ] Note that the  wavelength of maximum transmittance  is at 174 nm.  We call this   λ max  ,  pronounced “lambda max”. Very little light passes through the sample at this wavelength, because the wavelength corresponds very closely to ΔE for the π to π* transition. 

For example, knowing that the   λ max   for ethene is at 174 nm allows us to calculate the energy gap ΔE , which turns out to be about 164 kcal/mol .

As the number of conjugated pi bonds increases, the  λ max  increases as well!  Because longer frequency = smaller energy, this means that the  energy gap ΔE  between the highest-occupied molecular orbital (HOMO) and lowest unoccupied molecular orbital (LUMO) decreases  as the number of conjugated pi bonds  increases

The  ultraviolet region  falls in the range between  190-380 nm, t he  visible region  fall between  380-750 nm. The following electronic transitions are possible: π- π*  ( pi to pi star transition) n -  π*  ( n to pi star transition) σ - σ *  ( sigma to sigma star transition) n -  σ * ( n to sigma star transition) and are shown in the below hypothetical energy diagram

The  σ to σ*  transition requires an absorption of a photon with a wavelength which does not fall in the UV- vis range (see table 2 below). Thus, only  π to π*  and  n to π * transitions occur in the UV- vis region are observed.

σ to σ* > n to σ* > π to π* > n to π * highest energy lowest energy (lowest wavelength) (lowest wavelength) σ to σ*= c-c( alkanes ) π to π*= c=c ,or triple bond(alkenes, alkynes) n to π *=c=o(carbonyl compounds)

How Does  λ max   Relate To The Color We Perceive? How does the wavelength of maximum absorbance ( λ max ) relate to the actual  color?  First,  a refresher from the last post. We see the complementary colour of the major color that is absorbed.    A molecule that absorbs in the  blue  will appear  orange , because we perceive the colors that are  reflected , and  orange  is the complementary color of blue. For example, this molecule, Rhodamine B [note 2] absorbs at about 560 nm ( green )  and appears  red  , the complimentary color of green.

Solvent lower limit (nm) Acetonitrile 190 Chloroform 240 Cyclohexane 205 95% Ethanol 205 n-Hexane 195 Methanol 205 Water 190 1. Solvents used in UV-Vis spectroscopy (near UV)

Compound λ( nm) Intensity/ ε transition with lowest energy CH 4 122 intense σ-σ*( C-H) CH 3 CH 3 130 intense σ-σ* ( C-C) CH 3 OH 183 200 n- σ* ( C-O) CH 3 SH 235 180 n- σ* ( C-S) CH 3 NH 2 210 800 n- σ* ( C-N) CH 3 Cl 173 200 n- σ* ( C- Cl ) CH 3 I 258 380 n- σ* ( C-I) CH 2 =CH 2 165 16000 π-π* ( C=C) CH 3 COCH 3 187 950 π-π* ( C=O) 273 14 n- π* ( C=O) CH 3 CSCH 3 460 weak n- π* ( C=S) CH 3 N=NCH 3 347 15 n- π* ( N=N) a. Common functional groups

Introduction to UV spectroscopy- UV spectroscopy is type of absorption spectroscopy in which light of ultra-violet region (200-400 nm.) is absorbed by the molecule . Absorption of the ultra-violet radiations results in the excitation of the electrons from the ground state to higher energy state . The energy of the ultra-violet radiation that are absorbed is equal to the energy difference between the ground state and higher energy states ( deltaE = hf ).

Generally, the most favored transition is from the highest occupied molecular orbital (HOMO) to lowest unoccupied molecular orbital (LUMO).  For most of the molecules, the lowest energy occupied molecular orbitals are s orbital , which correspond to sigma bonds. The p orbitals are at somewhat higher energy levels, the orbitals ( nonbonding orbitals ) with unshared paired of electrons lie at higher energy levels . The unoccupied or antibonding orbitals (pie * and sigma * ) are the highest energy occupied orbitals . Some of the important transitions with increasing energies are: nonbonding to pie * , nonbonding to sigma * , pie to pie * , sigma to pie *  and sigma to sigma * .

Principle of UV spectroscopy UV spectroscopy obeys the Beer-Lambert law , which states that:  when a beam of monochromatic light is passed through a solution of an absorbing substance, the rate of decrease of intensity of radiation with thickness of the absorbing solution is proportional to the incident radiation as well as the concentration of the solution . The expression of Beer-Lambert law is- A = log (I /I) = Ecl Where, A = absorbance I  = intensity of light incident upon sample cell I = intensity of light leaving sample cell C = molar concentration of solute L = length of sample cell (cm.) E = molar absorptivity From the Beer-Lambert law it is clear that greater the number of molecules capable of absorbing light of a given wavelength, the greater the extent of light absorption. This is the basic principle of UV spectroscopy.

Instrumentation and working of UV Light Source - Tungsten filament lamps and Hydrogen-Deuterium lamps are most widely used and suitable light source as they cover the whole UV region. Tungsten filament lamps are rich in red radiations; more specifically they emit the radiations of 375 nm, while the intensity of Hydrogen-Deuterium lamps falls below 375 nm. Monochromator - Monochromators generally composed of prisms and slits. The most of the spectrophotometers are  double beam spectrophotometers . The radiation emitted from the primary source is dispersed with the help of rotating prisms. The various wavelengths of the light source which are separated by the prism are then selected by the slits such the rotation of the prism results in a series of continuously increasing wavelength to pass through the slits for recording purpose. The beam selected by the slit is monochromatic and further divided into two beams with the help of another prism.

Sample and reference cells - One of the two divided beams is passed through the sample solution and second beam is passé through the reference solution. Both sample and reference solution are contained in the cells. These cells are made of either silica or quartz. Glass can't be used for the cells as it also absorbs light in the UV region. Detector - Generally two photocells serve the  purpose of detector in UV spectroscopy . One of the photocell receives the beam from sample cell and second detector receives the beam from the reference. The intensity of the radiation from the reference cell is stronger than the beam of sample cell. This results in the generation of pulsating or alternating currents in the photocells.

Amplifier - The alternating current generated in the photocells is transferred to the amplifier. The amplifier is coupled to a small servometer . Generally current generated in the photocells is of very low intensity, the main purpose of amplifier is to amplify the signals many times so we can get clear and recordable signals. Recording devices - Most of the time amplifier is coupled to a pen recorder which is connected to the computer. Computer stores all the data generated and produces the spectrum of the desired compound

Concept of Chromophore and Auxochrome in the UV  Chromophore - Chromophore is defined as any isolated covalently bonded group that shows a characteristic absorption in the  ultraviolet or visible region (200-800 nm) . Chromophores can be divided into two groups- a) Chromophores which contain p electrons and which undergo pie to pie *  transitions. Ethylenes and acetylenes are the example of such chromophores . b) Chromophores which contain both p and nonbonding electrons. They undergo two types of transitions; pie to pie *  and nonbonding to pie * . Carbonyl, nitriles , azo compounds, nitro compounds etc. are the example of such chromophores . Auxochromes - An auxochrome can be defined as any group which does not itself act as a chromophore but whose presence brings about a shift of the absorption band towards the longer wavelength of the spectrum. –OH,-OR,-NH 2 ,-NHR, -SH etc. are the examples of auxochromic groups.

Absorption and intensity shifts in the UV spectroscopy a)  Bathochromic effect - This type of shift is also known as red shift. Bathochromic shift is an effect by virtue of which the absorption maximum is shifted towards the longer wavelength due to the presence of an auxochrome or change in solvents. The nonbonding to pie *  transition of carbonyl compounds observes bathochromic or red shift. b)  Hypsochromic shift - This effect is also known as blue shift. Hypsochromic shift is an effect by virtue of which absorption maximum is shifted towards the shorter wavelength. Generally it is caused due to the removal of conjugation or by changing the polarity of the solvents. c)  Hyperchromic effect - Hyperchromic shift is an effect by virtue of which absorption maximum increases. The introduction of an auxochrome in the compound generally results in the hyperchromic effect. d)  Hypochromic effect - Hyperchromic effect is defined as the effect by virtue of intensity of absorption maximum decreases. Hyperchromic effect occurs due to the distortion of the geometry of the molecule with an introduction of new group.

Chromophores - unsaturated groups like c= o,c =c Auxochromes - saturated groups contains non bonding electrons to chromophore

Solvent Effect Solvents play an important role in UV spectra. Compound peak could be obscured by the solvent peak. So a most suitable solvent is one that does not itself get absorbed in the region under investigation . A solvent should be transparent in a particular region. A dilute solution of sample is always prepared for analysis. Most commonly used solvents are as follows.

Solvent λ of absorption Water 191 nm Ether 215 nm Methanol 203 nm Ethanol 204 nm Chloroform 237 nm Carbon tetrachloride 265 nm Benzene 280 nm  Tetrahydrofuran 220 nm

Applications of UV spectroscopy 1.  Detection of functional groups - UV spectroscopy is used to detect the presence or absence of chromophore in the compound. This is technique is not useful for the detection of chromophore in complex compounds. The absence of a band at a particular band can be seen as an evidence for the absence of a particular group. If the spectrum of a compound comes out to be transparent above 200 nm than it confirms the absence of – a) Conjugation b) A carbonyl group c) Benzene or aromatic compound d) Bromo or iodo atoms. 2.  Detection of extent of conjugation - The extent of conjugation in the polyenes can be detected with the help of UV spectroscopy. With the increase in double bonds the absorption shifts towards the longer wavelength. If the double bond is increased by 8 in the polyenes then that polyene appears visible to the human eye as the absorption comes in the visible region.

3.  Identification of an unknown compound - An unknown compound can be identified with the help of UV spectroscopy. The spectrum of unknown compound is compared with the spectrum of a reference compound and if both the spectrums coincide then it confirms the identification of the unknown substance. 4.  Determination of configurations of geometrical isomers - It is observed that cis -alkenes absorb at different wavelength than the trans-alkenes. The two isomers can be distinguished with each other when one of the isomers has non-coplanar structure due to steric hindrances. The cis -isomer suffers distortion and absorbs at lower wavelength as compared to trans-isomer. 5.  Determination of the purity of a substance - Purity of a substance can also be determined with the help of UV spectroscopy. The absorption of the sample solution is compared with the absorption of the reference solution. The intensity of the absorption can be used for the relative calculation of the purity of the sample substance.