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Coherent Backscattering from Multiple Scattering Systems - KOPS ...

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5 Experiments<br />

space with the energy inside an absorbing cut-out of the half-space at the position of the<br />

sample:<br />

j with losses (⃗r ⊥ , t) = A(t) · j lossless (⃗r ⊥ , t) = j lossless (⃗r ⊥ , t) · ∫<br />

∫<br />

finite sample<br />

infinite half-space<br />

ρ τ (⃗r, t) d⃗r<br />

ρ τ→∞ (⃗r, t) d⃗r<br />

This ignores the fact that the photon density distribution is altered by the sample boundaries,<br />

but if the sample is large enough, only a few photons reach those boundaries anyway, so that<br />

the presence of the boundaries is of nearly no consequence for the density distribution.<br />

As solving eqns. 5.5 and 5.3 for the photon density distribution of the infinite half-space raises<br />

considerable algebraic and numeric difficulties, we fall back to the density distribution in free<br />

space, where the solution is easier to obtain. Fig. 5.2 shows that the albedos A(t) are similar<br />

enough to make this assumption, although the actual photon density distributions look quite<br />

different (fig. 5.3). The only difference in the albedos occurs when the photon cloud reaches<br />

the boundaries, which for the teflon sample in the figure happens at photon travel times<br />

around 10 to 100 ns. Even at this point the error is only a few percent, which presumably is<br />

not larger than the error that is already made by ignoring the altered density distribution.<br />

(5.5)<br />

Evaluating eqn. 5.5 gives the albedo<br />

∫ L<br />

1<br />

A(τ, L, R) =<br />

π(l ∗ +z 0 )<br />

0<br />

(√<br />

− K 0<br />

K 0<br />

(√<br />

4(l ∗ +z 0 ) 2 +z 2<br />

Dτ<br />

z 2<br />

Dτ<br />

)<br />

− 2K 0<br />

(√<br />

)<br />

+ 2K 0<br />

(√<br />

) (√<br />

R 2 +z 2<br />

Dτ<br />

+ K 0<br />

R 2 +4(l ∗ +z 0 ) 2 +z 2<br />

Dτ<br />

)<br />

− K 0<br />

(√<br />

)<br />

2R 2 +z 2<br />

Dτ<br />

−<br />

2R 2 +4(l ∗ +z 0 ) 2 +z 2<br />

Dτ<br />

)<br />

dz (5.6)<br />

where the K n (x) are modified Bessel functions of the second kind. The last step of integration<br />

is performed numerically.<br />

The transport mean free path l ∗ is the result of the evaluation of the backscattering data, for<br />

which the albedo is an input parameter. Therefore the correct value for l ∗ is not yet known<br />

when the albedo is calculated. Instead, we use l ∗ = 3D v<br />

≈ 3n effD<br />

c 0<br />

(see sec. 2.3), which should at<br />

least have the right order of magnitude.<br />

The resulting albedos for the samples examined in the backscattering experiments are given in<br />

tab. 5.1. One immediately observes the striking difference between the albedos of the titania<br />

samples, which are in excess of 99%, and the albedo of teflon, which is about 90%. The<br />

accuracy of the experiments therefore depends strongly on the accuracy of the teflon albedo.<br />

It is however nearly impossible to give an error for the calculated albedos, as the validity of the<br />

various assumptions is not known. Altogether, the error of the albedo mismatch is probably<br />

of the order of one or two percent.<br />

5.1.3 The correct theory of coherent backscattering<br />

The first steps towards a theoretical description of coherent backscattering have already been<br />

taken in sec. 2.1, where the intensity in a multiple scattering medium is presented as the<br />

48

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