Ultraviolet (UV) And Visible Spectroscopy

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Ultraviolet (UV) and Visible Spectroscopy1.1 IntroductionUltravialet and visible spectroscopy deals with the recording of the absorption ofradiations in the ultraviolet and visible regions of the electromagnetic spectrum. The ultavioletregion extends from 10 to 400 nm. It is subdivided into the near ultraviolet (quartz) region (200400 nm) and the far or vacuum ultraviolet region (10-200 nm). The visible region extends from400 to 800 nm. The absorption of electromagnetic radiations in the UV and visible regionsinduces the excitation of an electron from a lower to higher molecular orbital (electronic energyIevel). Since UV and visible spectroscopy involves electronic transitions, it is often calledelectronic spectroscopy. Organic chemists use ultraviolet and visible spectroscopy mainly fordetecting the presence and elucidating the nature of the conjugated multiple bonds or aromaticrings.1.2 Absorption Laws and Molar AbsorptivityA UV-visible spectrophotometer records a UV or visible spectrum (Fig. 1) as a plot ofwavelengths of absorbed radiations versus the intensity of absorption in terms of absorbance(optical density) A or molar absorptivity (molar extinction coefficient) ε as defined by theLambert-Beer law. According to Lambert's law, the fraction of incident monochromatic radiationabsorbed by a homogeneous medium is independent of the intensity of the incident radiationwhile Beer's law states that the absorption of a monochromatic radiation by a homogeneousmedium is proportional to the number of absorbing molecules. From these laws, the remainingvariables give the following equation which expresses the Lambert-Beer law(Fig 1)where I0 is the intensity of incident radiation, I the intensity of radiation transmitted through thesample solution, A the absorbance or optical density, ε the molar absorptivity or molar extinctioncoefficient, c the concentration of solute (mole/litre) and l the path length of the sample (cm).The molar absorptivity of an organic compound is constant at a given wavelength. The intensity

of an absorption band in the UV or visible spectrum is usually expressed as the molarabsorptivity at maximum absorption, εmax or log10 εmax· The wavelength of the maximumabsorption is denoted by λmax·When the molecular weight of a sample is unknown, or when a mixture is beingexamined, the intensity of absorption is expressed as E1%1 cm(or A1%1 cm)value, i.e. theabsorbance of a 1% solution of the sample in a 1 cm cellwhere c is the concentration in g/ 100 ml and l the path length of the sample in cm. This value iseasily related to ε by the expression1.3 Theory (Origin) of UV-Visible SpectroscopyUV-visible absorption spectra originate from electronic transitions within a molecule.These transitions involving promotion of valence electrons from the ground state to the higherenergy state (excited state) are called electronic excitations and are caused by the absorption ofradiation energy in the UVvisible regions of the electromagnetic spectrum. Since various energylevels of molecules are quantized, a particular electronic excitation occurs only by the absorptionof specific wavelength of radiation corresponding to the required quantum of energy.1.4 Electronic TransitionsAccording to molecular orbital theory, the excitation of a molecule by the absorption ofradiation in the UV-visible regions involves promotion of its electrons from a bonding, or nonbonding (n) orbital to an antibonding orbital. There are σ and π bonding orbitals associated withσ* and π* antibonding orbitals, respectively. Non-bonding (n or p) orbitals are not associated withantibonding orbitals because non-bonding or lone pair of electrons present in them do not formbonds. Following electronic transitions are involved in the UV-visible region (Fig. 2.2):

The usual order of energy required for various electronic transitions is1.5 Transition Probability: Allowed and Forbidden TransitionsOn exposure to UV or visible radiation, a molecule may or may not absorb the radiation,i.e. it may or may not undergo electronic excitation. The molar absorptivity at maximumabsorptionwhere P is the transition probability with values from 0 to 1 and a the target area of the absorbingsystem, i.e. a chromophore.A chromophore with a length of the order of 10 Å or 10-7 cm and with unit probability will haveεmax value of 105. Thus, there is a direct relationship between the area of a chromophore and itsabsorption intensity (εmax). Transitions with εmax values 104 are called allowed transitions andare generally caused by ππ* transitions, e.g. in 1, 3-butadiene, the absorption at 217 nm, εmax21,000 results from the allowed transition. Transitions with εmax values 104 are calledforbidden transitions. These are generally caused by nπ* transitions, e.g. in carbonylcompounds, the absorption near 300 nm with εmax values 10-100 results from the forbiddentransition.In addition to the area of a chromophore, there are also some other factors which govern thetransition probability. However, the prediction of their effects on the transition probability iscomplicated because they involve geometries of the lower and higher energy molecular orbitals

as well as the symmetry of the molecule as a whole. Symmetrical molecules have morerestrictions on their transitions than comparatively less symmetrical molecules. Consequently,symmetrical molecules like benzene have simple electronic absorption spectra as compared toless symmetrical molecules. There are very less symmetry restrictions for a highlyunsymmetrical molecule, thus it will exhibit a complex electronic absorption spectrum.1.6 Certain Terms Used in Electronic Spectroscopy: DefinitionsChromophoreA covalently unsaturated group responsible for absorption in the UV or visible region isknown as a chromophore. For example, C C, CC, C O, CN, N N, NO2 etc. If acompound absorbs light in the visible region (400-800 nm), only then it appears coloured. Thus,a chromophore may or may not impart colour to a compound depending on whether thechromophore absorbs radiation in the visible or UV region. Chromophores like C C or Chaving π electrons undergo πelectrons, e.g. C O, CC*π transitions and those having both π and non-bondingN or N N, undergo ππ*, nπ* and nσ* transitions.Since the wavelength and intensity of absorption depend on a number of factors, there are no setrules for the identification of a chromophore.AuxochromeA covalently saturated group which, when attached to a chromophore, changes both thewavelength and the intensity of the absorption maximum is known as auxochrome, e.g. NH2 ,OH, SH, halogens etc. Auxochromes generally increase the value of λmax as well as εmax byextending the conjugation through resonance. These are also called colour enhancing groups. Anauxochrome itself does not show absorption above 200 nm. Actually, the combination ofchromophore and auxochrome behaves as a new chromophore having different values of λmaxand εmax · For example, benzene shows λmax 256 nm, εmax 200, whereas aniline shows λmax 280nm, εmax 1430 (both increased). Hence, NH2 group is an auxochrome which extends theconjugation involving the lone pair of electrons on the nitrogen atom resulting in the increasedvalues of λmax and εmax ·

1.7 Absorption and Intensity ShiftsBathochramie Shift or Effect.The shift of an absorption maximum to a Ionger wavelength (Fig. 2.5) due to thepresence of an auxochrome, or solvent effect is called a bathochromic shift or red shift. Forexample, benzene shows λmax 256 nm and aniline shows λmax 280 nm. Thus, there is abathochromic shift of 24 nm in the λmax of benzene due to the presence of the auxochrome NH2.Similarly, a bathochromic shift of nπ* band is observed in carbonyl compounds on decreasingsolvent polarity, e.g. λmax of acetone is at 264.5 nm in water as compared to 279 nm in hexane.Hypsochromic Shift or EffectThe shift of an absorption maximum to a shorter wavelength is called hypsochromic orblue shift (Fig. 2.5). This is caused by the removal of conjugation or change in the solventpolarity. For example, aniline shows λmax 280 nm, whereas anilinium ion (acidic solution ofaniline) shows λmax 254 nm. This hypsochromic shift is due to the removal of nπ conjugationof the lone pair of electrons of the nitrogen atom of aniline with the π-bonded system ofthebenzene ring on protonation because the protonated aniline (anilinium ion) has no lone pair ofelectrons for conjugation. Similarly, there is a hypsochromic shift of 10-20 nm in the λmax ofππ*bands of carbonyl compounds on going from ethanol as solvent to hexane, i.e.on decreasing solvent polarity.

Hyperchromic Effect.An effect which leads to an increase in absorption intensity εmax is called hyperchromiceffect (Fig. 2.5). The introduction of an auxochrome usually causes hyperchromic shift. Forexample, benzene shows B-band at 256 nm, εmax 200, whereas aniline shows B-band at 280 nm,εmax 1430. The increase of 1230 in the value εmax of aniline compared to that of benzene is due tothe hyperchromic effect of the auxochrome NH2.Hypochromic EffectAn effect which Ieads to a decrease in absorption intensity εmax is called hypochromiceffect (Fig. 2.5). This is caused by the introduction of a group which distorts the chromophore.For example, biphenyl shows λmax 252 nm, εmax 19,000, whereas 2,2'-dimethylbiphenyl showsλmax 270 nm, εmax 800. The decrease of 18,200 in the value of εmax of 2,2'-dimethylbiphenyl isdue to the hypochromic effect of the methyl groups which distort the chromophore by forcing therings out of coplanarity resulting in the loss of conjugation.1.8 Solvent EffectsSince the polarity of a molecule usually changes with electronic transition, the positionand the intensity of absorption maxima may be shifted by changing solvent polarity.π*(i) πTransitions (K-Bands)Owing to the non-polar nature of hydrocarbon double bonds, the ππ * transitions ofalkenes, dienes and polyenes arenot appreciably affected by changing solvent polarity. Theππ*transitions of polar compounds, e-.g. saturated as well as a, α, ß-unsaturatedcarbonyl compounds are shifted to longer wavelengths and generally towards higher intensitywith increasing solvent polarity. The excited state in this transition is more polar than the groundstate, thus, dipole-dipole interaction with a polar solvent lowers the energy of the excited statemore than that of the ground state. Thus, there is a bathochromic shift of 10-20 nm in going fromhexane as a solvent to ethanol, i.e. on increasing solvent polarity.

(ii) B-BandsThese bands also originate from ππ * transitions, and their position and intensityare not shifted by changing solvent polarity except in case of heteroaromatic compounds whichshow a marked hyperchromic shift on increasing solvent polarity.(iii) nπ * Transitions (R-Bands)It has been found that an increase in solvent polarity usually shifts nπ* transitions toshorter wavelengths (higher energy). For example, acetone shows λmax 279 nm in hexane,whereas in water it shows λmax 264.5 nm. This can be explained on the basis that the carbonylgroup is more polar in the ground statethan in the excited stateThus, dipole-dipole interaction or hydrogen bonding with a polar solvent lowers the energy ofthe ground state more than that of the excited state resulting in the hypsochromic shift in case ofunconjugated as well as conjugated carbonyl compounds with increasing solvent polarity.(iv) nα* TransitionsThese transitions are affected by solvent polarity, especially by solvents capable offorming hydrogen bond. Alcohols and amines form hydrogen bonds with protic solvents. Suchassociations involve non-bonding electrons of the heteroatom. The involvement of non-bondingelectrons in hydrogen bonding lowers the energy of the n orbital, and thus the excitation of theseelectrons requires greater energy resulting in the hypsochromic shift with increasing polarity. Ithas been found that an increase in solvent polarity usually shifts nshorter wavelengths, and ππ* and nα*bands to*π bands of polar compounds to longer wavelengths.1.9 Woodward-Fieser Rules for Calculating λmax in Conjugated Dienes andTrienesWoodward (1941) formulated a set of empirical rules for calculating or predicting ilmaxin conjugated acyclic and six-membered ring dienes. These rules, modifiedby Fieser and Scott on

the basis of wide experience with dienes and trienes, are called Woodward-Fieser rules and aresummarized in Table 2.3. First, we discuss the following terms used in Woodward-Fieser rules.(i) Homoannular DienesIn homoannular dienes, conjugated double bonds are present in the same ring and havings-cis (cisoid) configuration (s single bond joining the two doubly bonded carbon atoms):The s-cis configuration causes strain which raises the ground state energy Ievel of the moleculeleaving the high energy excited state relatively unchanged. Thus, the transition energy is loweredresulting in the shift of absorption position to a Ionger wavelength. Acyclic dienes exist mostlyin the strainless s-trans (transoid) conformation with relatively lower ground state energy Ievel.Thus, their absorptions appear at shorter wavelengths. For example, 1, 3-cyclohexadiene (I)shows λmax 256 nm, whereas 1, 3-butadiene shows λmax 217 nm. Also, due to the shorter distance

between the two ends of the chromophore, s-cis dienes give lower εmax ( 1 0,000) than that ofthe s-trans dienes ( 20,000).(ii) Heteroannular DienesIn heteroannular dienes, conjugated double bonds are not present in the same ring andthese have s-trans (transoid) configurations:(iii) Exocyclic Conjugated Double BondsThe carbon-carbon double bonds projecting outside a ring are called exocyclic doublebonds. For exampleNote that the same double bond may be exocyclic to one ring, while endocyclic to the other andsometimes the same double bond may be exocyclic to two rings simultaneously.(iv) Alkyl Substituents and Ring ResiduesOnly the alkyl substituents and ring residues attached to the carbon atoms constituting theconjugated system of the compound are taken into account. Following examples indicate suchcarbon atoms by numbers and the alkyl substituents and ring residues by dotted lines:

In compounds containing both homoanular and heteroannular diene systems, the calculations arebased on the longer wavelength (253 nm), i.e. the homoannular diene system. The calculated andobserved values of λmax usually match within 5 nm as shown in the following examplesillustrating the applications of Woodward Fieser rules (Table 2.3).

2.0 Woodward-Fieser Rules for Calculating λmax in α,β Unsaturated CarbonylCompoundsCompounds containing a carbonyl group (C 0) in conjugation with an ethylenic groups(C C) are called enones. UV spectra of enones are characterized by an intense absorption band

(K-band) due to πweak R-band due to nπ * transition in the range 215-250 nm (εmax usually 10,000-20,000) and aπ * transition in 310-330 nm region (εmax usually 10-100). Similar todienes and trienes, there are set rules called Woodward-Fieser rules for calculating or predictingλmax in α,β -unsaturated carbonyl compounds (enones). These rules first framed by Woodwardand modified by Fieser and by Scott are given in Table 2.4.

For calculated Amax in other solvents, a solvent correction given in Table 2.5 must be carriedout.Since carbonyl compounds are polar, the positions of the K- and R-bands of enones aredependent on the solvent. Hence, solvent corrections are required (Table 2.5) to obtain thecalculated values of λmax in a particular solvent. The εmax for cisoid enones are usually 10,000,while that of transoid are 10,000. The calculated values of λmax are usually within 5 nm of theobserved values as shown in the following examples illustrating the applications of WoodwardFieser rules (Table 2.4).

Ultraviolet (UV) and Visible Spectroscopy 1.1 Introduction Ultravialet and visible spectroscopy deals with the recording of the absorption of radiations in the ultraviolet and visible regions of the electromagnetic spectrum. The ultaviolet region extends from 10 to 400 nm. It is subdivided into the near ultraviolet (quartz) region (200-

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