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CERN Program Library Long Writeup W5013 - CERNLIB ...

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We note that in case of photon perpendicular to the surface, the following relations hold:<br />

E ′ 0<br />

E 0<br />

=<br />

2n<br />

n ′ + n<br />

E 0<br />

′′<br />

= n′ − n<br />

E 0 n ′ + n<br />

where the sign convention for the parallel field has been adopted. This means that if n ′ >nthere is a phase<br />

inversion for the reflected wave.<br />

Any incoming wave can be separated into one piece polarised parallel to the plane and one polarised perpendicular,<br />

and the two components treated accordingly.<br />

To mantain the particle description of the photon, the probability to have a refracted (mechanism 107) or<br />

reflected (mechanism 106) photon must be calculated. The constraint is that the number of photons be<br />

conserved, and this can be imposed via the conservation of the energy flux at the boundary, as the number<br />

of photons is proportional to the energy. The energy current is given by the expression:<br />

⃗S = 1 c √ µɛE ⃗ × H ⃗ ∗ = c √ ɛ<br />

2 4π<br />

8π µ E2ˆk<br />

0<br />

and the energy balance on a unit area of the boundary requires that:<br />

⃗S · ⃗u = S ⃗′ · ⃗u − S ⃗′′ · ⃗u<br />

S cos i = S ′ cos r + S ′′ cos i<br />

c 1<br />

8π µ nE2 0 cos i = c<br />

8π<br />

1<br />

µ ′ n′ E ′2<br />

0 cos r + c<br />

8π<br />

1<br />

µ nE′′2 0 cos i<br />

If we set again µ/µ ′ ≈ 1, then the transmission probability for the photon will be:<br />

( E<br />

′ ) 2<br />

T = 0 n ′ cos r<br />

E 0 n cos i<br />

and the corresponding probability to be reflected will be R =1− T .<br />

In case of reflection the relation between the incoming photon ( ⃗ k,⃗e), the refracted one ( ⃗ k ′ ,⃗e ′ ) and the<br />

reflected one ( ⃗ k ′′ ,⃗e ′′ ) is given by the following relations:<br />

⃗q = ⃗ k × ⃗u<br />

e ‖ =<br />

⃗e · ⃗u<br />

|q|<br />

e ⊥ =<br />

⃗e · ⃗q<br />

|q|<br />

e ′ 2n cos i<br />

‖ = e ‖<br />

n ′ cos i + n cos r<br />

e ′ 2n cos i<br />

⊥ = e ⊥<br />

n cos i + n ′ cos r<br />

e ′′<br />

‖ = n′<br />

n e′ ‖ − e ‖<br />

e ′′ ⊥ = e′ ⊥ − e ⊥<br />

After transmission or reflection of the photon, the polarisation vector is renormalised to 1. In the case where<br />

sin r = n sin i/n ′ > 1 then there cannot be a refracted wave, and in this case we have a total internal<br />

reflection according to the following formulas:<br />

⃗ k<br />

′′<br />

= ⃗ k − 2( ⃗ k · ⃗u)⃗u<br />

⃗e ′′ = −⃗e +2(⃗e · ⃗u)⃗u<br />

236 PHYS260 – 5

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