Page 326 - Instant notes
P. 326

Physical Chemistry     312


        i.e. the Beer-Lambert law for the intensity, I, of transmitted radiation is:
           I=I 0exp(−σ[X]l)

        The constant σ is called the absorption coefficient or extinction coefficient.
           The Beer-Lambert law is often written in terms of logarithms to the base 10, in which
        case, by writing σ=ε ln10:



        The constant ε is another form of the absorption (extinction) coefficient. The constants σ
        and ε are related directly to the transition probability f or the spectral transition. The
                                                −1
        dimensions of σ and ε are (concentration×length)  but the exact units depend on the units
        used for the species concentration (e.g. molar or molecular units) and path length. Care
        must  be  taken to determine whether values of absorption coefficient are referenced to
        logarithms of absorption intensity ratios to base e or to base 10. The convention is as
        written here. In either form, it can be seen that transmitted intensity  decreases
        exponentially with the length of sample through which the radiation passes.
           The ratio of the transmitted intensity to the  incident  intensity,  I/I 0, is called the
        transmittance, T, so log
           log T=−ε[X]l

        The absorbance (or optical density) of the species,



                                         −A
        is related to transmittance through, T=10 .


                                       Linewidths
        Spectral lines are not infinitely narrow since that would violate a variant of  the
        Heisenberg uncertainty principle (Topic G4) which states that  the  energy of a state
        existing for a time, τ, is subject to an uncertainty, δE, of magnitude:



        Since no excited state has an infinite lifetime, the spectral transition corresponding to the
        energy separation between two states is spread over a finite width of energy. The energy
        uncertainty  inherent  to  states  that have finite lifetimes is called  lifetime broadening.
        Two processes contribute to the finite lifetime of excited states:
        (i) The rate of spontaneous emission of radiation as an excited state collapses to a lower
           state (a fundamental property of the molecule) establishes an intrinsic minimum
           natural linewidth to the transition, δE nat≈ћ/τ nat where τ nat is the natural lifetime to
           spontaneous decay.
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