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Principles of Fluorescence Spectroscopy

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PRINCIPLES OF FLUORESCENCE SPECTROSCOPY 901<br />

ation is occurring at a rate comparable to the intensity<br />

decay rate.<br />

A7.3. The lifetime <strong>of</strong> the R state (τ OR ) can be calculated<br />

from the phase angle difference ∆φ = φ R – φ F . At 100<br />

MHz this difference is 58E, which corresponds to a<br />

lifetime <strong>of</strong> 16 ns.<br />

A7.4. A. Acridine and acridinium may be reasonably<br />

expected to display distinct absorption spectra.<br />

The emission spectrum in 0.2 M NH 4 NO 3 (Figure<br />

7.49) shows evidence for emission from both<br />

acridine and acridinium. Hence if both species<br />

were present in ground state, the absorption<br />

spectrum should be a composite <strong>of</strong> the absorption<br />

spectra <strong>of</strong> acridine and acridinium. In contrast,<br />

if the acridinium is formed only in the<br />

excited state, then the absorption spectrum in 0.2<br />

M NH 4 NO 3 should be almost identical to that <strong>of</strong><br />

neutral acridine.<br />

B. Examination <strong>of</strong> the data (Table 7.6) reveals two<br />

decay times that are independent <strong>of</strong> emission<br />

wavelength. This indicates that there are two<br />

emitting species and that their decay rates are<br />

independent <strong>of</strong> emission wavelength. On the<br />

short-wavelength side <strong>of</strong> the emission the decay<br />

is a single exponential. This result indicates the<br />

reaction is irreversible and that the measured<br />

decay times at other wavelengths contain contributions<br />

from both acridine and acridinium.<br />

Pro<strong>of</strong> <strong>of</strong> an excited-state reaction is provided by<br />

observation <strong>of</strong> negative pre-exponential factors.<br />

As the observation wavelength is increased this<br />

term becomes more predominant. At the longest<br />

observation wavelengths one finds that the preexponential<br />

factors are nearly equal in magnitude<br />

and opposite in sign. This near equality <strong>of</strong><br />

the pre-exponential factors indicates that at 560<br />

nm the emission is predominantly from the<br />

relaxed species. The fact that α 2 is slightly larger<br />

than α 1 indicates that there is still some emission<br />

from neutral acridine at 560 nm.<br />

A7.5. Red-edge excitation selects for fluorophores that are<br />

most strongly interacting with the solvent. The solvent<br />

configuration around these selected fluorophores is<br />

similar to that in a solvent-relaxed state. The TRES<br />

with 416-nm excitation do not show a time-dependent<br />

CHAPTER 8<br />

shift because the fluorophore is already in the relaxed<br />

state.<br />

A8.1. The apparent bimolecular quenching <strong>of</strong> 2-AP by Cu 2+<br />

can be found by noting that F 0 /F = 1.10 at 2 x 10 –6 M<br />

Cu 2+. Hence K = 50,000 M –1 and k q = 5 x 10 12 M –1 s –1.<br />

Similarly, F 0/F = 1.7 at 0.001 M DMA, yielding K =<br />

700 M –1 and k q = 7 x 10 10 M –1 s –1 . Both values are<br />

larger than the maximum value possible for diffusive<br />

quenching in water, near 1 x 10 10 M –1 s –1. This implies<br />

some binding or localization <strong>of</strong> the quenchers near the<br />

fluorophores.<br />

A8.2. The data in Figure 8.72 can be used to calculate the<br />

lifetimes <strong>of</strong> pyrene, which are 200, 119, and 56 ns in<br />

the presence <strong>of</strong> N 2, air or O 2, respectively. Assuming<br />

the oxygen solubility in DMPC vesicles is fivefold<br />

larger than in water (0.001275 M/atm in water), the<br />

oxygen bimolecular quenching constant is k q = 2 x 10 9<br />

M –1 s –1 . This value is about 20% <strong>of</strong> the value expected<br />

for a fluorophore dissolved in water.<br />

A8.3. The data in the absence <strong>of</strong> benzyl alcohol (Figure<br />

8.73) can be used to calculate a bimolecular quenching<br />

constant <strong>of</strong> 6 x 10 9 M –1 s –1 . This indicates that the<br />

naphthalene is mostly accessible to iodide and probably<br />

not bound to the cyclodextrin. This conclusion is<br />

supported by the data in the presence <strong>of</strong> benzyl alcohol.<br />

In the presence <strong>of</strong> benzyl alcohol the Stern-<br />

Volmer plots curve downward in the presence <strong>of</strong> β-CD<br />

(Figure 8.74). This suggests the presence <strong>of</strong> two naphthalene<br />

populations, one <strong>of</strong> which is less accessible to<br />

iodide quenching. In the presence <strong>of</strong> benzyl alcohol<br />

and 5.1 mM β-CD the Stern-Volmer plot is still<br />

curved, and the apparent value <strong>of</strong> k q decreases, which<br />

indicates shielding from iodide quenching. Under<br />

these conditions it seems that naphthalene binds to β-<br />

CD only in the presence <strong>of</strong> benzyl alcohol.<br />

A8.4. Figure 8.77 shows a plot <strong>of</strong> F 0 /F versus [I –]. From the<br />

upward curvature <strong>of</strong> this plot it is apparent that both<br />

static and dynamic quenching occur for the same population<br />

<strong>of</strong> fluorophores. The dynamic (K D ) and static<br />

(K S ) quenching constants can be calculated by a plot<br />

<strong>of</strong> the apparent quenching constant (K app ) versus the

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