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Physical Chemistry 3: — Chemical Kinetics — - Christian-Albrechts ...

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12.3 The radiative lifetime 0 and the fluorescence quantum yield Φ 243<br />

12.3 The radiative lifetime τ 0 and the fluorescence quantum yield Φ <br />

I Determination of the radiative lifetime τ 0 : Assuming that there are no competing<br />

nonradiative processes, we can determine the radiative lifetime 0 by<br />

(1) time-resolved measurements of the (exponential) fluorescence decay after pulsed<br />

excitation,<br />

(2) high-resolution measurement of the natural (Lorentzian) linewidth according to<br />

∆ ∆ = ~ (12.8)<br />

y<br />

0 =<br />

1<br />

2 ∆ 0<br />

(12.9)<br />

(3) evaluation from the molar absorption coefficient (Lambert-Beer) using the relationship<br />

between the Einstein coefficients 21 and 21 , 51<br />

21 = 83<br />

3 21 (12.10)<br />

(4) calculate the value of ¯¯ ¯¯2 (⇒ 12 21 21 )fromfirst principles.<br />

I Fluorescence quantum yield: Apart from quenching, the fluorescence is reduced by<br />

other radiationless processes (IC, ISC, R, . . . ). The experimentally measured fluorescence<br />

lifetime is therefore smaller (often much smaller) than the radiative lifetime 0 .<br />

The ratio is the fluorescence quantum yield:<br />

Φ =<br />

<br />

+ + + + [Q] + = 0<br />

(12.11)<br />

51 The actual procedure, which involves integration over the absorption band, corrects for the influence<br />

of the refraction index of the solvent, etc., is called the Strickler-Berg analysis.

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