Heisenberg's Uncertainty - ΔλΔx

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Discussion Overview

The discussion revolves around the relationship between Heisenberg's Uncertainty Principle and the behavior of light emitted through a small slit from a blackbody source. Participants explore the implications of uncertainty in position and momentum, as well as the concept of cavity radiation and its connection to blackbody emission.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant proposes a derivation involving Heisenberg's Uncertainty Principle, suggesting that uncertainty in position leads to uncertainty in wavelength for light emitted through a slit.
  • Another participant corrects the notation used, stating that standard deviations (σ) should be used instead of differentials (Δ) in the context of uncertainties.
  • A different perspective is introduced, stating that the phenomenon of blackbody radiation through a small slit is related to cavity radiation and does not involve the uncertainty principle.
  • Some participants discuss the implications of using different notations for uncertainty, with one expressing confusion about the appropriateness of treating uncertainties as differentials.
  • One participant emphasizes that the main premise regarding the relationship to the uncertainty principle has been overlooked in favor of discussing notation and derivation validity.

Areas of Agreement / Disagreement

Participants express disagreement regarding the relevance of the uncertainty principle to the scenario described. While some focus on the derivation and notation, others argue that the connection to the uncertainty principle is not applicable in this context.

Contextual Notes

There are unresolved issues regarding the treatment of uncertainties as differentials versus standard deviations, and the implications of this choice on the validity of the derivation presented. Additionally, the discussion highlights a lack of consensus on the relevance of the uncertainty principle to the behavior of light emitted from a blackbody through a small slit.

Who May Find This Useful

This discussion may be of interest to those studying quantum mechanics, particularly in relation to the uncertainty principle and blackbody radiation, as well as those exploring the nuances of notation in physics.

Legaldose
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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.
 
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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.
 

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