Why does Planck's constant not appear in the Rayleigh-Jeans formula?

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Homework Help Overview

The discussion revolves around the derivation of the Rayleigh-Jeans formula from Planck's formula, particularly focusing on the absence of Planck's constant in the former. Participants are exploring the relationship between these two formulas in the context of blackbody radiation and thermodynamics.

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning, Problem interpretation

Approaches and Questions Raised

  • Participants are attempting to derive the Rayleigh-Jeans formula from the Planck formula by examining limits and conditions under which certain terms simplify. Questions arise regarding the behavior of the formulas as temperature approaches infinity and the implications of this on the derivation.

Discussion Status

The discussion is active, with multiple participants providing insights and suggestions for approaching the derivation. Some participants have pointed out potential errors in the original poster's understanding of the formulas, while others suggest methods for simplifying the expressions involved. There is no explicit consensus on the correct approach yet, as participants are exploring different interpretations and methods.

Contextual Notes

There is mention of the Stefan-Boltzmann Law and its relevance to the discussion, though its application is not fully resolved. Participants are also navigating the complexities of limits and series expansions in their attempts to connect the two formulas.

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I am to derive the incorrect Rayleigh-Jeans formula from the correct Planck formula to show why plank's constant does not appear in the Rayleigh-Jeans formula. I should also recall the Stefen-Boltmann Law

here's what I have but I'm stuck...

Rayleigh-Jeans formula: u(\lambda)=\frac{8 \pi k T }{\lambda^{4}}

Planks formula: u(\lambda)=\frac{8 \pi k T }{\lambda^{4}}\frac{hc/ \lambda}{e^{hc/ \lambda K T} - 1}

so I am thinking I am somehow supposed to get: \frac{hc/ \lambda}{e^{hc/ \lambda K T} - 1} = 1 but I don't know how to even begin. any ideas?
 
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First, the Planck formula is u(\lambda) = \frac{8 \pi}{\lambda^4} \frac{ h c / \lambda}{e^{hc/\lambda k T} - 1}. You have an extra factor of k T in your Planck formula which is the source of the confusion. It should now be a simple matter to obtain the Rayleigh-Jeans formula by taking the appropriate limit.
 
so that should lead me to prove that...

\frac{hc/ \lambda}{e^{hc/ \lambda K T} - 1} = kT

I am sorry but it is still not apparent how I should go about solving this... as T nears infinity, i get infinity on both sides, so does that prove that \frac{hc/ \lambda}{e^{hc/ \lambda K T} - 1} = kT?

and how does the Stefan-Boltzmann Law come into play?
 
For Rayleigh-Jeans, you need to look at what happens the \lambda becomes large.

For Stephan-Boltzmann, you need to look at the total contribution from all wavelengths, i.e., you need to look at

\int_{0}^{\infty} u \left( \lambda \right) d \lambda.

Make a change of integration variable so that T does not appear explicitly in the integrand. Evaluating the resulting integral requires some specialized knowledge of special function. If you only need to show proportionality to T^4, then the integral need not be evaluated. If you need the proportionality constant, use software (e.g., Maple) or tables to evaluate the integral

Regards,
George
 
Last edited:
\frac{hc/ \lambda}{e^{hc/ \lambda K T} - 1} = kT

when lambda --> infinity, the left hand side becomes 0/0 so I applied hospital's rule to get:

\frac{hc(-\frac{1}{ \lambda^2})}{\frac{hc}{kT} e^{hc/ \lambda K T}} = kT

\lambda \rightarrow \inf

\frac{hc}{\frac{hc}{kT}}=kT

kT=kT

I did not use the stefen-boltzmann law, did I do this correctly?
 
Last edited:
I guess I mistunderstood - I thought you wanted to derive Rayleigh-Jeans and Stefan-Boltzmann from Planck.

To derive Rayleigh-Jeans, expand as a series the exponential in Physics Monkey's expression, and find what happens when \lambda becomes large, but not infinite.

Regards,
George
 
the Rayleigh-Jeans formula is: u(\lambda)=\frac{8 \pi k T }{\lambda^{4}}

while Planck's formula consists of Rayleigh-Jeans but includes \frac{hc/ \lambda}{e^{hc/ \lambda K T} - 1} instead of kT

so what I did was set \frac{hc/ \lambda}{e^{hc/ \lambda K T} - 1} = kT and solved for when the wavelength was really big, which shows that indeed \frac{hc/ \lambda}{e^{hc/ \lambda K T} - 1} = kT

plugging this into Planck's equation, I will get the Rayleigh-Jeans formula:

u(\lambda)=\frac{8 \pi }{\lambda^{4}}\frac{hc/ \lambda}{e^{hc/ \lambda K T} - 1}

\frac{hc/ \lambda}{e^{hc/ \lambda K T} - 1} = kT

Rayleigh-Jeans formula: u(\lambda)=\frac{8 \pi k T }{\lambda^{4}}

did it do this right? was I supposed to include the stefen-boltzmann law somewhere in there?
 
I don't think so - it appears that you've just gone round in a circle.

You need to start with

u \left( \lambda \right) = \frac{8 \pi hc}{\lambda^{5} \left( e^{hc/ \lambda K T} - 1 \right)},

do what I suggested in my previous post, and arrive at

u \left( \lambda \right) = \frac{8 \pi k T }{\lambda^{4}}.

Regards,
George
 
If T is large, then the exponent in e^{hc/ \lambda kT} is small and you can use Bernoulli's formula

e^{x}=1+x valid for "x" very small.

Daniel.
 

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