Sneaky photons

Light travels with different velocities and different wavelengths (and hence wave vectors) in different media. Since light is made out of photons, individual photons change their momentum as they change the media. One way to actually derive Snell's law is from the behavior of photons at the boundary between different dielectrics.

A photon is travelling from a medium with the refractive index n 1 = 1 n_1 = 1 (air) to a medium with the refractive index n 2 = 1.5 n_2 = 1.5 (glass). Its incident angle is 6 0 60^\circ , measured from the normal to the boundary between the two surfaces. For how much does the momentum of the photon change in 1 0 30 kg m/s 10^{-30}~\mbox{kg m/s} ?

Details and assumptions

  • The incident photon is green, i.e. its wavelength is 555 nm 555~\mbox{nm} .


The answer is 865.26.

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2 solutions

According to Snell's law: n 1 sin α = n 2 sin β n_1 \sin \alpha=n_2 \sin \beta , so β 35.2 6 \beta \approx 35.26^\circ .

The change of the direction of vector momentum is: ϕ = α β 24.7 4 \phi=\alpha-\beta \approx 24.74^\circ .

The change of vector momentum of the photon: Δ p = p 1 2 + p 2 2 2 p 1 p 2 cos ϕ \Delta p=\sqrt{p^2_1+p^2_2-2p_1p_2 \cos \phi}

= h λ n 2 + 1 2 n cos ϕ 865.26 ( k g m / s ) =\frac{h}{\lambda} \sqrt{n^2+1-2n \cos \phi} \approx 865.26 (kgm/s) .

Why can't we use

s i n ( θ 1 ) s i n ( θ 2 ) = λ 1 λ 2 \frac{sin(\theta_1)}{sin(\theta_2)} = \frac{\lambda_1}{\lambda_2}

to calculate the second wavelength ( = 370 n m = 370 nm ), and then

p 2 = h λ 2 = 1.791 1 0 27 ( k g m / s ) p_2 = \frac{h}{\lambda_2} = 1.791 * 10^{-27} (kg m / s)

p 1 = h λ 1 = 1.194 1 0 27 ( k g m / s ) p_1 = \frac{h}{\lambda_1} = 1.194 * 10^{-27} (kg m / s)

Δ p = 596.94 1 0 30 ( k g m / s ) \Delta p = 596.94 * 10^{-30} (kg m / s)

?

D G - 7 years, 9 months ago

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Because the direction of the photon changes, the momentum changes direction and you have to account for that.

Kevin Fei - 7 years, 9 months ago
Nhat Le
Sep 4, 2013

The angle of refraction is calculated using Snell's Law: n 1 sin θ 1 = n 2 sin θ 2 n_1\sin \theta_1=n_2\sin \theta_2 , so sin θ 2 = 1 × sin 6 0 1.5 = 0.57735 \sin \theta_2 = \frac{1\times \sin60^\circ}{1.5}=0.57735 , giving θ 2 = sin 1 0.57735 = 35.2 6 \theta_2 = \sin^{-1}0.57735=35.26^\circ

Now we calculate the magnitudes of the initial and final momenta. The initial momentum is p 1 = h λ 1 = 6.63 × 1 0 34 555 × 1 0 9 = 1.1946 × 1 0 27 k g m s 1 p_1=\frac{h}{\lambda_1}=\frac{6.63\times 10^{-34}}{555\times10^{-9}} =1.1946 \times 10^{-27} \ \mathrm{kgms^{-1}}

For the final momentum, note that the speed of the photon decreases by 1.5 1.5 times, and since v = f λ v=f\lambda while the frequency f f remains constant, the wavelength λ \lambda must decrease by 1.5 1.5 times. So we have p 2 = h λ 2 = h λ 1 / 1.5 = 1.5 p 1 = 1.7918 × 1 0 27 k g m s 1 p_2=\frac{h}{\lambda_2}=\frac{h}{\lambda_1/1.5} =1.5p_1=1.7918 \times 10^{-27} \ \mathrm{kgms^{-1}}

Since momentum is a vector quantity, we cannot simply subtract the magnitudes to find the vector change in momentum. We will have to consider two components - parallel to the surface and perpendicular to the surface.

Δ p / / = p 2 sin θ 2 p 1 sin θ 1 = 1.12096 × 1 0 31 k g m s 1 \Delta p_{//} =p_2\sin\theta_2 - p_1\sin\theta_1=-1.12096 \times 10^{-31} \ \mathrm{kgms^{-1}} Δ p = p 2 cos θ 2 p 1 cos θ 1 = 8.6586 × 1 0 28 k g m s 1 \Delta p_{\perp} =p_2\cos\theta_2 - p_1\cos\theta_1=8.6586 \times 10^{-28} \ \mathrm{kgms^{-1}}

And so the magnitude of the change in momentum is Δ p = Δ p / / 2 + Δ p 2 = 8.65 × 1 0 28 k g m s 1 |\Delta p| = \sqrt{\Delta p_{//}^2 + \Delta p_{\perp}^2}= 8.65 \times 10^{-28} \ \mathrm{kgms^{-1}}

The answer will be 865 \fbox{865}

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