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 />
E sample<br />
(t) / E half−space<br />
(t)<br />
1<br />
0.8<br />
0.6<br />
0.4<br />
0.2<br />
0<br />
free space distribution<br />
half−space distribution<br />
−9.5 −9 −8.5 −8 −7.5 −7 −6.5 −6<br />
log 10<br />
(t [sec])<br />
Figure 5.2: Comparison of the albedos. The time-dependent albedos A(t) of an<br />
absorbing cut-out of the free space (solid line) and respectively a half-space (dashed<br />
line) at the position of the sample are similar enough to replace the latter by the former<br />
in the calculation of the total albedo. Calculations for teflon sample with radius R =<br />
20 mm, thickness L = 50 mm, diffusion coefficient D = 16500 m2 /s, absorption time<br />
τ = 3.3 ns, transport mean free path l ∗ = 220 µm, refractive index n = 1.35.<br />
be equal to one, meaning that the incoming light power P in is equal to the scattered power<br />
P out of a lossless sample. The albedo can therefore also be defined as<br />
A = P with losses<br />
P lossless<br />
=<br />
∫ ∫<br />
∫ surface ∫<br />
surface<br />
j with losses (⃗r ⊥ , t) d⃗r ⊥ dt<br />
j lossless (⃗r ⊥ , t) d⃗r ⊥ dt<br />
(5.3)<br />
In our multiple scattering samples, most of the loss of light energy is due to absorption. If it<br />
were the only reason for energy loss, the albedo could be easily calculated as<br />
A(τ) = 1 − 2(l∗ +z 0 )<br />
e− √<br />
Dτ<br />
(5.4)<br />
2(l ∗ +z<br />
√ 0 )<br />
Dτ<br />
with diffusion coefficient D, absorption time τ, and penetration depth z 0 .<br />
However, as the samples are not infinitely large, one can not a priori exclude that losses at the<br />
side and rear boundaries have significant influence on the photon distribution in the sample.<br />
Unfortunately there is no expression for the photon density distribution in a 3-dimensionally<br />
confined absorbing medium. Therefore we approximate the losses in a sample with finite<br />
radius R and thickness L by comparing the energy inside the non-absorbing infinite half-<br />
46