Year 12 Cambridge Physics: Classical Mechanics v Light Particle Collision

Click For Summary

Homework Help Overview

The discussion revolves around classical mechanics and light particle collision, specifically focusing on deriving expressions for pressure exerted by particles on a surface and understanding radiation pressure from a light bulb. The original poster presents a problem involving particles with kinetic energy and momentum, as well as a secondary question regarding the maximum radiation pressure from a light source.

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning

Approaches and Questions Raised

  • The original poster attempts to derive an expression for pressure based on particle properties and questions how to approach the light bulb scenario. Some participants affirm the correctness of the initial approach and suggest applying similar principles to the second part. Others introduce concepts of momentum transfer and energy density in relation to radiation pressure.

Discussion Status

Participants are actively engaging with the problem, providing hints and affirmations. Some guidance has been offered regarding the relationship between pressure, momentum, and intensity, while others are exploring the implications of different surface types on pressure calculations. There is a recognition of the need to clarify assumptions and correct misunderstandings in the original poster's reasoning.

Contextual Notes

Participants note potential errors in the original poster's assumptions regarding intensity and the application of the inverse square law. The discussion includes considerations of how the momentum of photons relates to their wavelength and energy, as well as the implications of surface characteristics on pressure outcomes.

johnconnor
Messages
62
Reaction score
0
Question:
A stream of particles, each of mass m and having kinetic energy E, is collimated into a parallel beam of cross-sectional area A. The particles are incident normally on a smooth plane surface at rate n and they rebound elastically. Derive an expression for the pressure on the surface in terms of A, m, E and n. Explain why the pressure would be different if the surface were rough so that the particles rebounded at various angles.

An electric light bulb emits 20W of radiation uniformly in all directions. What is the maximum radiation pressure on a surface placed 2.0m away from the bulb? State the conditions under which this will occur?

Attempt:
E_k = 0.5mu^2 \Rightarrow u=\sqrt{2E/m}
\text{Ft} = 2m\sqrt{2E/m}
F = Ftn
P= \dfrac{2mn\sqrt{2E/m}}{A}
P = \dfrac{2n\sqrt{2EM}}{A}

2nd part: incident momentum is added a factor of sin/cosine and therefore effective impulse decreases (blah blah blah..).

I don't know how to start the light bulb part. Does λ=h/p come into use? The wavelength of light covers a range of values; which should I choose? Can anyone please give me some hints? Thank you!
 
Physics news on Phys.org


Your first part seems correct to me. Apply the same principle for the second, too. The force exerted by light would be the momentum transferred per unit second to the object. Pressure, hence would be the momentum transferred per unit second per unit area. So,

Pressure = \frac{\Delta p}{At}

But the intensity is also the energy density. So, we have

P = \frac{I}{c}

where c is the speed of the photons. I think you should be able to do it from here :smile:
 


Infinitum said:
But the intensity is also the energy density. So, we have

P = \frac{I}{c}

where c is the speed of the photons. I think you should be able to do it from here :smile:

Ah. I didn't know about this formula. Maybe I've forgotten it. Thanks! Will work on it!
 


johnconnor said:
Ah. I didn't know about this formula. Maybe I've forgotten it. Thanks! Will work on it!

Oh, it is easily derivable :smile:

Did you notice I derived this for an absorbing surface?? Can you see what it would be for a reflecting surface?
 


Infinitum said:
Your first part seems correct to me. Apply the same principle for the second, too. The force exerted by light would be the momentum transferred per unit second to the object. Pressure, hence would be the momentum transferred per unit second per unit area. So,

Pressure = \frac{\Delta p}{At}

But the intensity is also the energy density. So, we have

P = \frac{I}{c}

where c is the speed of the photons. I think you should be able to do it from here :smile:
So I reattempted the final part in lieu of Infinitum's tip, and my working is as such:

Consider a beam of light with energy E incident on a flat surface area A 2.0m away from the light bulb.

E=hf; Power=E/t; a^2=A

Power = E/t

Power = hf/t

Since t = 2/c,

Power = hfc/2

Force x 2 x c/2 = hfc/2

Force/A = hf/2

Ah i just bullgarbageed. Sorry.
There are plenty of errors in my attempt: I didn't try to find the value of A, and I'm assuming that intensity remains the same after traveling 2metres (which contradicts the inverse square law). But what other mistakes have I made? What assumptions which I thought to be applicable but fallacious in this context?

Also, could you please elaborate on your post? Thank you...
 


johnconnor said:
So I reattempted the final part in lieu of Infinitum's tip, and my working is as such:

Consider a beam of light with energy E incident on a flat surface area A 2.0m away from the light bulb .

E=hf; Power=E/t; a^2=A

Power = [STRIKE]E/t[/STRIKE]

Power = [STRIKE]hf/t[/STRIKE]

Since t = 2/c,

Power = [STRIKE]hfc/2[/STRIKE]



E=hf is the energy of a single photon. The power of the source is the energy emitted in unit time. The power of the source has nothing to do with the time the photons reach from the source to the surface.
You get the number of photons N emitted in one second if you divide the power of the source by the energy of a single photon. These photons are emitted in every directions. You need to find the number of photons n falling on the area A at 2 m distance in unit time. How do you it?

To get the pressure you need to do the same as before: Find the change of the momentum Δp of a single photon upon collision. As n photon arrives in unit time the force they exert on the surface is F=nΔp. Divide it by the surface area to get the pressure.

Now the main thing: the momentum of a photon. It depends on the wavelength: p=h/λ, or p=hf/c in terms of the frequency.
(http://en.wikipedia.org/wiki/Photon) You certainly have learned it together with the formula for the energy of a photon E=hf.

ehild
 

Similar threads

  • · Replies 1 ·
Replies
1
Views
3K
  • · Replies 9 ·
Replies
9
Views
4K
  • · Replies 11 ·
Replies
11
Views
5K
  • · Replies 27 ·
Replies
27
Views
5K
  • · Replies 2 ·
Replies
2
Views
8K
  • · Replies 4 ·
Replies
4
Views
4K
  • · Replies 6 ·
Replies
6
Views
5K