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Principles of Fluorescence Spectroscopy

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256 DYNAMICS OF SOLVENT AND SPECTRAL RELAXATION<br />

sion spectra. In some circumstances it is possible to obtain<br />

information about the rate <strong>of</strong> relaxation using only steadystate<br />

measurements. The basic idea is to use collisional<br />

quenching to decrease the lifetime <strong>of</strong> the excited state (τ) to<br />

a value comparable to the relaxation time (τS ). As described<br />

in Section 7.5, the center <strong>of</strong> gravity <strong>of</strong> the emission can be<br />

expected to decay exponentially from ν 0 at t = 0 to ν∞ at t<br />

= 4 according to<br />

ν cg(t) ν ∞ (ν 0 ν ∞) exp(t/τ S)<br />

(7.13)<br />

Suppose the total intensity decays with a single decay time<br />

τ. The center <strong>of</strong> gravity observed in a steady-state emission<br />

spectra is given by the integral average <strong>of</strong> ν cg (t) over the<br />

intensity decay:<br />

ν cg <br />

∞<br />

0 ν cg(t) exp (t/τ) dt<br />

∞<br />

0 ν cg (t)dt<br />

Substitution <strong>of</strong> eq. 7.13 into 7.15 yields<br />

νcg ν∞ (ν0 ν∞) τS τ<br />

(7.14)<br />

(7.15)<br />

This expression connects the center-<strong>of</strong>-gravity observed in<br />

a steady-state experiment, with the relative values <strong>of</strong> the<br />

decay time τ and the spectral relaxation time τ S . From this<br />

expression one can also understand the spectral shifts<br />

observed at low and high temperatures. At low temperature,<br />

τ S >> τ, and the center <strong>of</strong> gravity is ν 0 . At high temperature,<br />

τ S

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