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Principles of Fluorescence Spectroscopy

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446 ENERGY TRANSFER<br />

wavelength is expressed in nm then F D (λ) is in units <strong>of</strong> M –1<br />

cm –1 (nm) 4 , and the Förster distance in Å is given by<br />

R 0 0.211(κ 2 n 4 Q D J(λ) ) 1/6 (in Å)<br />

R 6 0 8.79 10 5 (κ 2 n 4 Q D J(λ) ) (in Å 6 )<br />

(13.5)<br />

(13.6)<br />

If the wavelength is expressed in cm and J(λ) is in units <strong>of</strong><br />

M -1 cm 3 , the Förster distance is given by<br />

R 6 0 8.79 10 25 (κ 2 n 4 Q D J(λ) ) (in cm 6 )<br />

R 0 9.78 10 3 (κ 2 n 4 Q D J(λ) ) 1/6 (in Å)<br />

R 6 0 8.79 10 23 (κ 2 n 4 Q D J(λ) ) (in Å 6 )<br />

(13.7)<br />

(13.8)<br />

(13.9)<br />

It is important to recognize that the Förster distances are<br />

usually reported for an assumed value <strong>of</strong> κ 2 , typically κ 2 =<br />

2/3. Once the value <strong>of</strong> R 0 is known the rate <strong>of</strong> energy transfer<br />

can be easily calculated using<br />

kT(r) 1 ( τD R 6<br />

0 ) r<br />

(13.10)<br />

If the transfer rate is much faster than the decay rate, then<br />

energy transfer will be efficient. If the transfer rate is slower<br />

than the decay rate, then little transfer will occur during<br />

the excited-state lifetime, and RET will be inefficient.<br />

The efficiency <strong>of</strong> energy transfer (E) is the fraction <strong>of</strong><br />

photons absorbed by the donor which are transferred to the<br />

acceptor. This fraction is given by<br />

E <br />

k T(r)<br />

τ 1<br />

D k T(r)<br />

(13.11)<br />

which is the ratio <strong>of</strong> the transfer rate to the total decay rate<br />

<strong>of</strong> the donor in the presence <strong>of</strong> acceptor. Recalling that k T (r)<br />

= τ D –1(R 0 /r) 6 , one can easily rearrange eq. 13.11 to yield<br />

E R6 0<br />

R 6 0 r 6<br />

(13.12)<br />

This equation shows that the transfer efficiency is strongly<br />

dependent on distance when the D–A distance is near R 0<br />

(Figure 13.2). The efficiency quickly increases to 1.0 as the<br />

Figure 13.2. Dependence <strong>of</strong> the energy transfer efficiency (E) on distance.<br />

R 0 is the Förster distance.<br />

D–A distance decreases below R 0 . For instance, if r = 0.1R 0<br />

one can readily calculate that the transfer efficiency is<br />

0.999999, indicating that the donor emission would not be<br />

observable. Conversely, the transfer efficiency quickly<br />

decreases to zero if r is greater than R 0 . Because E depends<br />

so strongly on distance, measurements <strong>of</strong> the distance (r)<br />

are only reliable when r is within a factor <strong>of</strong> 2 <strong>of</strong> R 0 . If r is<br />

twice the Förster distance (r = 2R 0 ) then the transfer efficiency<br />

is 1.54%, and if r = 0.5R 0 then the efficiency is<br />

98.5%. It is not practical to use RET to measure distances<br />

outside the range <strong>of</strong> r = 0.5R 0 to r = 2R 0 .<br />

The transfer efficiency is typically measured using the<br />

relative fluorescence intensity <strong>of</strong> the donor, in the absence<br />

(F D ) and presence (F DA ) <strong>of</strong> acceptor:<br />

E 1 F DA<br />

F D<br />

(13.13)<br />

The transfer efficiency can also be calculated from the lifetimes<br />

under these respective conditions (τ DA and τ D ):<br />

E 1 τ DA<br />

τ D<br />

(13.14)<br />

It is important to remember the assumptions involved in<br />

using these equations. Equations 13.13 and 13.14 are only<br />

applicable to donor-acceptor pairs that are separated by a<br />

fixed distance, a situation frequently encountered for<br />

labeled proteins. However, a single fixed donor–acceptor<br />

distance is not found for a mixture <strong>of</strong> donors and acceptors<br />

in solution, nor for donors and acceptors dispersed random-

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