Talk:Phy5645: Difference between revisions
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ScottMiller (talk | contribs) (New page: Given that Planck's energy distribution equation is: <math> \rho_{Planck} = \frac{2c^2}{\lambda^5}\frac{h}{e^\frac{hc}{\lambda k T}-1}</math> show that in the long wavelength limit this ...) |
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Given that Planck's energy distribution equation is: | Given that Planck's energy distribution equation is: | ||
<math> \rho_{Planck} = \frac{2c^2}{\lambda^5}\frac{h}{e^\frac{hc}{\lambda k T}-1}</math> | :<math> \rho_{\text{Planck}} = \frac{2c^2}{\lambda^5}\frac{h}{e^\frac{hc}{\lambda k T}-1}</math> | ||
show that in the long wavelength limit this reduces to the Rayleigh-Jeans equation: | show that in the long wavelength limit this reduces to the Rayleigh-Jeans equation: | ||
<math>\rho_{Rayleigh} = \frac{2ckT}{\lambda^4}</math> | :<math>\rho_{\text{Rayleigh}} = \frac{2ckT}{\lambda^4}</math> | ||
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<math>\displaystyle\lim_{\lambda\to\infty}</math> | <math>\displaystyle\lim_{\lambda\to\infty}</math> | ||
by expanding the exponential in the denominator for first order in lambda: | by expanding the exponential in the denominator for first order in <math> \lambda \!</math>: | ||
<math>e^\frac{hc}{\lambda k T}-1 \approx ( | :<math> | ||
<math>\frac{2c^2}{\lambda^5}\frac{h}{e^\frac{hc}{\lambda k T}-1} \approx \frac{2c^2}{\lambda^5}\left(\frac{h}{( | e^\frac{hc}{\lambda k T}-1 \approx (hc)/(\lambda kT) </math> | ||
:<math> \implies \frac{2c^2}{\lambda^5}\frac{h}{e^\frac{hc}{\lambda k T}-1} \approx \frac{2c^2}{\lambda^5}\left(\frac{h}{(hc)/(\lambda kT)}\right) | |||
</math> | |||
then | then | ||
<math>\frac{2c^2}{\lambda^5}\left(\frac{h}{( | :<math>\frac{2c^2}{\lambda^5}\left(\frac{h}{(hc)/(\lambda kT)}\right) = \frac{2 c k T }{\lambda^4}</math> |
Latest revision as of 00:26, 11 December 2009
Given that Planck's energy distribution equation is:
show that in the long wavelength limit this reduces to the Rayleigh-Jeans equation:
Solution:
Evaluate the limit:
by expanding the exponential in the denominator for first order in :
then