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Concepts Of Physics MCQ Edition [Volume 2]
Exam
Concepts Of Physics MCQ Edition [Volume 2]
Subject
Physics
Chapter
Photoelectric Effect and Wave–Particle Duality

Concepts Of Physics MCQ Edition [Volume 2] · Physics · Photoelectric Effect and Wave–Particle Duality

A sphere of radius 1.00 cm is positioned in the path of a parallel...

A sphere of radius 1.00 cm1.00 \text{ cm} is positioned in the path of a parallel beam of light of large aperture. The intensity of the light is 0.50 W cm−20.50 \text{ W cm}^{-2}. If the sphere is not perfectly absorbing, how does the force on the sphere due to the light falling on it compare to the case where it completely absorbs the radiation?

Options

  1. AThe force is greater than when it completely absorbs the radiation
  2. BThe force is the same as when it completely absorbs the radiation
  3. CThe force depends on the specific absorption coefficient of the sphere
  4. DThe force is less than when it completely absorbs the radiation

Correct answer

B. The force is the same as when it completely absorbs the radiation

Step-by-step solution

Let the intensity of the incident light be II and the radius of the sphere be RR.

For a perfectly absorbing sphere, the light is completely absorbed by the projected cross-sectional area πR2\pi R^2. The force exerted is the rate of change of momentum:
Fabs=IcπR2F_{abs} = \dfrac{I}{c} \pi R^2

For a perfectly reflecting sphere, consider an elemental ring on the surface of the sphere at an angle θ\theta with respect to the direction of the incident beam. The area of this element is dS=2πR2sin⁡θdθdS = 2\pi R^2 \sin \theta d\theta.

The power incident on this elemental area is P=Icos⁡θdSP = I \cos \theta dS.
Since the light is specularly reflected, the change in momentum per unit time (force) is directed along the normal to the surface:
dF=2Pccos⁡θ=2Iccos⁡2θdSdF = \dfrac{2P}{c} \cos \theta = \dfrac{2I}{c} \cos^2 \theta dS

The component of this force along the direction of the incident beam (z-axis) is:
dFz=dFcos⁡θ=2Iccos⁡3θdSdF_z = dF \cos \theta = \dfrac{2I}{c} \cos^3 \theta dS

Substituting dS=2πR2sin⁡θdθdS = 2\pi R^2 \sin \theta d\theta, we get:
dFz=4πR2Iccos⁡3θsin⁡θdθdF_z = \dfrac{4\pi R^2 I}{c} \cos^3 \theta \sin \theta d\theta

Integrating this over the illuminated hemisphere (from θ=0\theta = 0 to θ=π/2\theta = \pi/2):
Fref=4πR2Ic∫0π/2cos⁡3θsin⁡θdθF_{ref} = \dfrac{4\pi R^2 I}{c} \int_0^{\pi/2} \cos^3 \theta \sin \theta d\theta

Let cos⁡θ=t\cos \theta = t, then −sin⁡θdθ=dt-\sin \theta d\theta = dt. The limits change from 11 to 00:
Fref=4πR2Ic∫01t3dt=4πR2Ic[t44]01=πR2IcF_{ref} = \dfrac{4\pi R^2 I}{c} \int_0^1 t^3 dt = \dfrac{4\pi R^2 I}{c} \left[ \dfrac{t^4}{4} \right]_0^1 = \dfrac{\pi R^2 I}{c}

We can see that Fref=FabsF_{ref} = F_{abs}. The force on a perfectly reflecting sphere is exactly equal to the force on a perfectly absorbing sphere.

Since any opaque partially absorbing sphere can be considered as a combination of an absorbing fraction α\alpha and a reflecting fraction ρ\rho (where α+ρ=1\alpha + \rho = 1), the total force will be:
F=αFabs+ρFref=(α+ρ)πR2Ic=πR2IcF = \alpha F_{abs} + \rho F_{ref} = (\alpha + \rho) \dfrac{\pi R^2 I}{c} = \dfrac{\pi R^2 I}{c}

Therefore, the force on the sphere is the same as when it completely absorbs the radiation.
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