22.07.2013 Views

Principles of Fluorescence Spectroscopy

Principles of Fluorescence Spectroscopy

Principles of Fluorescence Spectroscopy

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

420 ADVANCED ANISOTROPY CONCEPTS<br />

→<br />

→<br />

Figure 12.12. Prolate ellipsoid <strong>of</strong> revolution. A and E are the<br />

directions <strong>of</strong> the absorption and emission transition moments, respectively.<br />

Revised and reprinted with permission from [4]. Copyright ©<br />

1985, Academic Press, Inc.<br />

tions <strong>of</strong> the two rotational rates (D || and D ⊥ ). The amplitudes<br />

<strong>of</strong> the anisotropy decay depend on the orientation <strong>of</strong> the<br />

transition moments. If one <strong>of</strong> the transition moments is<br />

directed along any <strong>of</strong> the symmetry axes <strong>of</strong> the ellipsoid,<br />

then the anisotropy decay becomes a double exponential.<br />

Hence, one can expect double-exponential anisotropy<br />

decays for molecules like DPH or perylene, where the longwavelength<br />

absorption and emission moments are directed<br />

along the long axis <strong>of</strong> the molecules.<br />

12.4. ELLIPSOIDS OF REVOLUTION<br />

We now describe the theory for the anisotropy decays <strong>of</strong><br />

ellipsoids <strong>of</strong> revolution. It is important to remember that<br />

this theory assumes the ellipsoid to be rigid. In the case <strong>of</strong><br />

a labeled protein this assumption implies no independent<br />

motion <strong>of</strong> the fluorophore within the protein. For prolate or<br />

oblate ellipsoids the anisotropy decay is expected to display<br />

three correlation times:<br />

r(t) r 1 exp(t/θ 1) r 2 exp(t/θ 2)<br />

r 3 exp(t/θ 3 )<br />

(12.11)<br />

The amplitudes decaying with each correlation time depend<br />

on the angles <strong>of</strong> the absorption (β A ) and emission (β E )<br />

dipoles with the symmetry axis. Using the notation defined<br />

in Figure 12.12 these anisotropy amplitudes are<br />

r 1 0.3 sin 2β A sin 2β E cos ξ<br />

r 2 0.3 sin 2 β A sin 2 β E cos 2ξ<br />

r 3 0.1(3 cos 2 β A 1)(3 cos 2 β E 1)<br />

(12.12)<br />

(12.13)<br />

(12.14)<br />

Occasionally one finds alternative forms 37–38 for r 1 and r 2 :<br />

r 1 1.2 sin β A cos β A sin β E cos β E cos ξ<br />

r 2 0.3 sin 2 β A sin 2 β E cos 2ξ<br />

The fundamental anisotropy is given as usual by<br />

r 0 r 1 r 2 r 3 0.2(3 cos 2 β 1)<br />

(12.15)<br />

(12.16)<br />

(12.17)<br />

where β is the angle between the absorption and emission<br />

transition moments. The three correlation times are determined<br />

by the two different rotational rates:<br />

θ 1 (D || 5D ) 1<br />

θ 2 (4D || 2D ) 1<br />

θ 3 (6D ) 1<br />

(12.18)<br />

(12.19)<br />

(12.20)<br />

Depending upon the shape <strong>of</strong> the ellipsoid <strong>of</strong> rotation, and<br />

the orientation <strong>of</strong> the transition moments, a variety <strong>of</strong> complex<br />

anisotropy decays can be predicted. 4,37<br />

In the previous chapter we saw that one can calculate<br />

these rotational correlation times for a spherical molecule<br />

(θ S ) based on its volume and the solution viscosity. Similar

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!