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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2.3 Random walk and diffusion<br />
of propagation. The difference between transport mean free path and scattering mean free<br />
path is the larger the more anisotropic the scattering is. For completely isotropic scattering<br />
both mean free paths are equal.<br />
The product M ∗ l ∗ gives the length s of the photon paths that contribute to the mean square<br />
displacement. As there is no reason to assume that the speed of the photons will change<br />
along their path, the length of a photon path is proportional to time. The size of the photon<br />
cloud 〈r 2 (t)〉 at a certain time is therefore linearly proportional to both the length s of the<br />
contributing photon paths and the time t the photons have spent traveling along these paths.<br />
On top of everything, the mean square displacement of eqn. 2.4 is structurally equivalent to<br />
the variance<br />
〈r 2 (t)〉 = 6Dt (2.5)<br />
of a gaussian distribution in three dimensions<br />
ρ(⃗r, t) =<br />
1<br />
r2<br />
√ e− 4Dt (2.6)<br />
3<br />
4πDt<br />
where ρ is the density distribution of photons that started off at the origin of the coordinate<br />
system at time t = 0 in an infinitely extended medium, and D is the diffusion coefficient. So<br />
obviously multiple scattering in the limit of large M(t) can also be described as diffusion of<br />
light energy through the medium with the diffusion equation ∂ρ<br />
∂t − D∇2 ρ = δ(t)δ(⃗r), whose<br />
solution is given by eqn. 2.6<br />
Comparing eqns. 2.4 and 2.5 one can give the diffusion coefficient as<br />
D = sl∗<br />
3t = vl∗<br />
3<br />
(2.7)<br />
where v is the velocity of energy transport. Using this, the photon density distribution can<br />
also be given as a function of the path length s:<br />
ρ(⃗r, s) =<br />
√<br />
3<br />
4πsl ∗ 3<br />
e − 4<br />
r2<br />
3 sl∗ (2.8)<br />
However, the photon density distribution in a multiply scattering sample is not purely determined<br />
by the scattering properties of the scattering particles, but also by energy losses due to<br />
absorption in the material. According to Lambert-Beer’s law, absorption weakens the intensity<br />
of a light wave exponentially along the traveled path, so that its effect can be included<br />
in the photon density distribution by an additional factor e − la<br />
s<br />
or e − τ t , respectively. The absorption<br />
length l a and the absorption time τ are inversely proportional to the number density<br />
ρ abs of absorbing particles on the path and their absorption cross section σ abs : l a = 1<br />
ρ abs σ abs<br />
and<br />
τ = t s l 1<br />
a =<br />
v ρ abs σ abs<br />
.<br />
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