Coherent Backscattering from Multiple Scattering Systems - KOPS ...
Coherent Backscattering from Multiple Scattering Systems - KOPS ...
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 />
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