Heisenberg's Uncertainty - ΔλΔx

  • Context: Graduate 
  • Thread starter Thread starter Legaldose
  • Start date Start date
  • Tags Tags
    Uncertainty
Click For Summary
SUMMARY

The discussion centers on the relationship between Heisenberg's Uncertainty Principle and the behavior of light emitted from a blackbody through a small slit. Participants clarify that the correct formulation of the uncertainty principle is σxσp ≥ ħ/2, emphasizing that Δ should be interpreted as standard deviations rather than differentials. The concept of cavity radiation is introduced, explaining that EM waves inside a hollow body reach thermal equilibrium and that the small hole allows for blackbody radiation to escape. The conversation highlights the importance of notation and understanding the physics behind these principles.

PREREQUISITES
  • Understanding of Heisenberg's Uncertainty Principle (σxσp ≥ ħ/2)
  • Knowledge of blackbody radiation and cavity radiation concepts
  • Familiarity with standard deviation and Gaussian distribution in statistics
  • Basic principles of electromagnetic waves and their momentum (p = E/c)
NEXT STEPS
  • Study the implications of Heisenberg's Uncertainty Principle in quantum mechanics
  • Research the properties and applications of blackbody radiation
  • Learn about the derivation and significance of cavity radiation
  • Explore the differences between standard deviation and differential notation in physics
USEFUL FOR

Physics students, researchers in quantum mechanics, and anyone interested in the principles of blackbody radiation and uncertainty in measurements.

Legaldose
Messages
73
Reaction score
6
So we have a light bulb emitting through a small slit. I read somewhere that a blackbody shining through a small slit acts like a perfect emitter, and I wanted to know why. I figured it must have something to do with Heisenberg's Uncertainty. Here's how I went about it:

\Delta x\Delta p \geq \frac{\hbar}{2}

The momentum of light is just E/c, so

p = \frac{E}{c} = \frac{h}{\lambda}

and

\lambda^{2} = \frac{h^{2}c^{2}}{E^{2}}

To find Δp, just take the derivative wrt λ

\frac{\Delta p}{\Delta \lambda}=\frac{-h}{\lambda^{2}}

and

\Delta p = \frac{h}{\lambda^{2}}\Delta \lambda

I ignore the negative because this is uncertainty in either direction. So..

\Delta x \Delta p = \Delta x\frac{h}{\lambda^{2}}\Delta\lambda

Then I subbed back into the first eq and solved for ΔxΔλ

\Delta x \Delta \lambda \geq \frac{\lambda^{2}}{4\pi}

thus

\Delta x \Delta \lambda \geq \frac{h^{2}c^{2}}{4\pi E^{2}}

Is this why they say that the light shining through a small slit a near perfect emitter? Because since we don't know exactly where the light goes through the slit, it must have an uncertainty in the wavelength when it comes out. If so, what is that E for? Is it the energy of the photons before they enter the slit? Thanks.
 
Physics news on Phys.org
The correct equation is \sigma_x\sigma_p \geq \frac{\hbar}{2}, where \sigma denotes standard deviation. I'm not sure it's correct to treat them as \Deltas the way you did, treating them as differentials. Maybe if I knew statistics better I would be able to tell you.
 
Legaldose said:
So we have a light bulb emitting through a small slit. I read somewhere that a blackbody shining through a small slit acts like a perfect emitter, and I wanted to know why. I figured it must have something to do with Heisenberg's Uncertainty.
This is known as cavity radiation. EM waves inside a hollow body interact with the walls. Given enough time they come to thermal equilibrium. The hole gives them a way to escape and be observed. The fact that the hole is "small" retains them long enough to equilibrate into black body radiation. Uncertainty principle not involved.
 
MisterX said:
The correct equation is \sigma_x\sigma_p \geq \frac{\hbar}{2}, where \sigma denotes standard deviation. I'm not sure it's correct to treat them as \Deltas the way you did, treating them as differentials. Maybe if I knew statistics better I would be able to tell you.

In physics, we traditionally indicate uncertainties with Δ (e.g. Δx, Δy, Δp), with the understanding that they are standard deviations. Usually we assume a normal (Gaussian) distribution unless explicitly specified otherwise.
 
jtbell said:
In physics, we traditionally indicate uncertainties with Δ (e.g. Δx, Δy, Δp), with the understanding that they are standard deviations. Usually we assume a normal (Gaussian) distribution unless explicitly specified otherwise.

Well if you read the OP, (s)he also treated them as differentials e.g. \frac{\Delta f}{\Delta x} = \frac{d f}{d x}. My comment was addressing this.
 
MisterX said:
Well if you read the OP, (s)he...

It's he :p

So I'm not allowed to use them as differentials? My modern professor has done so on a few occasions to get at a couple more uncertainty relations.
 
Legaldose said:
It's he :p

So I'm not allowed to use them as differentials? My modern professor has done so on a few occasions to get at a couple more uncertainty relations.
I think there is the approximation

\frac{\sigma_{f(X)}}{\sigma_X} \approx f'(E[X])

Where E[X] is the mean value of X. However I think it's important that you understand the distinction. The expression on the left is not a derivative.

This is a relation between the standard deviations of a random variable and a function of that random variable that comes from a first order Taylor series expansion. It will not necessarily always give decent results.

source
 
Last edited:
Okay thanks a lot, I'll have to be more careful in the future. I'm going to start using the sigma notation instead of delta, just to remind myself.
 
I'm scratching my head here because the actual, relevant response to the entire premise has been completely overlooked. Bill K's response addresses directly the starting scenario, especially the part where this has nothing to do with the HUP.

Somehow, the emphasis on the distraction, i.e. the notation or the validity of the derivation took center stage.

Zz.
 
  • #10
Oh man I didn't even see his post. :rolleyes:

As it happens, after my original post, I read the Wiki page on black bodies, which has a section about cavity radiation. But I appreciate the answer and wish I'd have actually seen it.
 

Similar threads

  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 10 ·
Replies
10
Views
3K
  • · Replies 0 ·
Replies
0
Views
1K
  • · Replies 2 ·
Replies
2
Views
991
  • · Replies 8 ·
Replies
8
Views
2K
  • · Replies 15 ·
Replies
15
Views
3K
  • · Replies 2 ·
Replies
2
Views
1K
  • · Replies 5 ·
Replies
5
Views
2K
  • · Replies 1 ·
Replies
1
Views
868