Deriving Wien's Law from Planck's Formula

In summary, the conversation discusses deriving Wien's displacement law from Planck's formula by differentiating and setting the derivative equal to 0. However, the presence of the term 5kT\lambda in the equation makes it a transcendental equation, which means that an exact solution cannot be found. This is explained further in the provided Wikipedia link.
  • #1
Dorje
25
0
As a refresher exercise in modern physics, I want to derive Wien's displacement law:

[tex]\lambda_{max}T=2.898x10^{-3}mK[/tex]

from Planck's formula:

[tex]R(\lambda)=(\frac{c}{4})(\frac{8\pi}{\lambda^4})(\frac{hc}{\lambda})(\frac{1}{\exp^(\frac{hc}{\lambda\kT})-1})[/tex]

by differentiating R([tex]\lambda[/tex]) and setting dR/d[tex]\lambda[/tex] = 0. I get to an expression like this:

[tex]\exp^(\frac{hc}{\lambda\kT})(hc - 5kT\lambda)+5kT\lambda=0[/tex]

If it wasn't for the "5kT[tex]\lambda[/tex]" term by itself on the left-hand side of the equation, the solution would simply be:

([tex]\lambda[/tex]) (T) = hc / 5k

which is Wien's law. There must be something wrong though, or maybe there's a trick involved that I'm not seeing?

Thanks
 
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  • #2
Yes, you're dealing with a typical transcendental equation, to which exact solutions cannot be found in most cases, this one included.

Daniel.
 
  • #3

Related to Deriving Wien's Law from Planck's Formula

1. What is Wien's Law and what does it describe?

Wien's Law is a formula that describes the relationship between the wavelength of peak emission and the temperature of a blackbody object. It states that the wavelength of peak emission is inversely proportional to the temperature of the object. In other words, as the temperature increases, the peak emission shifts to shorter wavelengths.

2. How is Wien's Law derived from Planck's Formula?

Planck's Formula is a mathematical expression that describes the energy distribution of a blackbody object at a given temperature. By taking the derivative of this formula with respect to wavelength and setting it equal to zero, we can find the wavelength at which the energy distribution is at its maximum. This wavelength is then used in Wien's Law to determine the relationship between peak emission and temperature.

3. Why is Wien's Law important in the field of astronomy?

Wien's Law is important in astronomy because it allows us to determine the temperature of celestial objects, such as stars, based on their peak emission wavelength. This information can then be used to study the physical properties and composition of these objects.

4. Are there any limitations to using Wien's Law?

Yes, there are limitations to using Wien's Law. It is only applicable to objects that behave like blackbodies, which absorb and emit all radiation that falls on them. In addition, Wien's Law only applies to objects that are in thermal equilibrium, meaning that their temperature is constant.

5. Can Wien's Law be applied to objects other than blackbodies?

Wien's Law can be applied to objects other than blackbodies, but only if their spectral energy distribution is known. In this case, the energy distribution can be substituted into Planck's Formula to find the wavelength of peak emission and then used in Wien's Law to determine the relationship with temperature.

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