How does the spectral distribution of blackbody radiation relate to Wien's law?

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SUMMARY

The discussion focuses on the spectral distribution of blackbody radiation and its relationship to Wien's law. Key equations derived include the relationships between frequency and wavelength, specifically dν = -c dλ / λ², and the Rayleigh-Jeans spectral distribution u_{RJ}(ν) aligning with Wien's law as u_{W}(ν) = W(λT)/λ⁵. The undetermined function W(λT) is established as W(λT) = 8πhc/(e^(hc/k(λT)) - 1) based on Planck's formula. Participants seek clarification on specific steps in the derivation process, particularly in part a)2).

PREREQUISITES
  • Understanding of blackbody radiation concepts
  • Familiarity with Wien's law and Rayleigh-Jeans law
  • Knowledge of Planck's formula for spectral distribution
  • Basic calculus for integration and differentiation
NEXT STEPS
  • Study the derivation of Planck's law in detail
  • Learn about the implications of the Rayleigh-Jeans law in thermodynamics
  • Explore the mathematical techniques for integrating spectral distributions
  • Investigate the physical significance of the undetermined function W(λT)
USEFUL FOR

Students and educators in physics, particularly those focusing on thermodynamics, quantum mechanics, and the study of blackbody radiation. This discussion is beneficial for anyone looking to deepen their understanding of spectral distributions and their mathematical foundations.

spaghetti3451
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Homework Statement



a) Show that for photons of frequency \nu and wavelength \lambda :

1) d\nu = - c d\lambda / \lambda^{2}
2) u(\lambda)d\lambda = - u(\nu)d\nu
3) u(\lambda)d\lambda = u(\nu) c d\lambda / \lambda^{2}

b) Show that the Rayleigh-Jeans spectral distribution of blackbody radiation, u_{RJ}(\nu), is of the form required by Wien's law, u_{W}(\nu) = \frac{W(\lambda T)}{\lambda ^{5}}

c) Obtain the correct form of Wien's undetermined function W(\lambda T) from Planck's formula.

Homework Equations



The Attempt at a Solution



Solution to a):

1) d\nu = \frac{d\nu}{d\lambda}d\lambda = - \frac{c}{\lambda^{2}}d\lambda
2) can't do
3) substitute d\nu in 1) to d\nu on the RHS of 2)

Solution to b):

u_{RJ}(\nu)d\nu = \frac{8\pi\nu^{2}}{c^{3}}kTd\nu
- u_{RJ}(\lambda)d\lambda = (\frac{8\pi\frac{c^{2}}{\lambda^{2}}}{c^{3}}kT)(-\frac{c}{\lambda^{2}}d\lambda)
u_{RJ}(\lambda)d\lambda = \frac{8\pi k(\lambda T)}{\lambda^{5}}d\lambda
So, W(\lambda T) = 8\pi k(\lambda T)

Solution to c):

u(\nu)d\nu = \frac{8\pi h \nu^{3}}{c^{3}} \frac{d\nu}{e^\frac{h\nu}{kT} - 1}
- u(\lambda)d\lambda = \frac{8 \pi h \frac{c^{3}}{\lambda^{3}}}{c^{3}} \frac{- \frac{c}{\lambda^{2}}d\lambda}{e^{\frac{hc}{\lambda kT}} - 1}
u(\lambda)d\lambda = \frac{8 \pi hc}{\lambda^{5}} \frac{d\lambda}{e^{\frac{hc}{\lambda kT}} - 1}
So, W(\lambda T) = \frac{8\pi hc}{e^{\frac{hc}{k(\lambda T)}} - 1}
Need help with a)2). Also, can you check the rest, please?
 
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failexam said:
Need help with a)2).

You know what you get when you integrate u(λ) dλ and u(v) dv. You can for example integrate first integral from 0 to some λ, and second one from v to ∞. Then these integrals are equal, right?
 

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