Phy5645/UV catastrophe problem2: Difference between revisions
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YuhuiZhang (talk | contribs) (New page: (Submitted by Team 4-Yuhui Zhang) Try to use Boltzman-Maxwell statistics to deduce Plank Formula. (We have to consider quantum energy spectrum as Plank did.) If the energy spectrum is: <...) |
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(Submitted by Team 4-Yuhui Zhang) | (Submitted by Team 4-Yuhui Zhang) | ||
Try to use Boltzman-Maxwell statistics to deduce Plank Formula. (We have to consider quantum energy spectrum as Plank did.) | Try to use Boltzman-Maxwell statistics to deduce Plank Formula. (We have to consider quantum energy spectrum as Plank did.) | ||
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\frac{1}{{e^{\frac{{h\upsilon }}{{kT}}} - 1}} | \frac{1}{{e^{\frac{{h\upsilon }}{{kT}}} - 1}} | ||
</math>. (This is just the result of Bose-Einstein statistics.) | </math>. (This is just the result of Bose-Einstein statistics.) | ||
so: | so: | ||
<math> | <math> | ||
E(\upsilon ) = \frac{{8\pi }}{{h^3 }}\frac{1}{{e^{\frac{{h\upsilon }}{{kT}}} - 1}}p^2 dp = \frac{1}{{\pi ^2 c^3 }}\frac{{\hbar \omega ^3 }}{{e^{\frac{{h\upsilon }}{{kT}}} - 1}}d\omega = 8\pi \frac{{h\upsilon ^3 }}{{c^3 }}\frac{1}{{e^{\frac{{h\upsilon }}{{kT}}} - 1}}d\varepsilon | E(\upsilon ) = \frac{{8\pi }}{{h^3 }}\frac{1}{{e^{\frac{{h\upsilon }}{{kT}}} - 1}}p^2 dp = \frac{1}{{\pi ^2 c^3 }}\frac{{\hbar \omega ^3 }}{{e^{\frac{{h\upsilon }}{{kT}}} - 1}}d\omega = 8\pi \frac{{h\upsilon ^3 }}{{c^3 }}\frac{1}{{e^{\frac{{h\upsilon }}{{kT}}} - 1}}d\varepsilon | ||
</math>, this | </math>, | ||
this reflects the phenomenon of black body irradiation, which is called Plank Formula. |
Latest revision as of 15:55, 30 November 2009
(Submitted by Team 4-Yuhui Zhang)
Try to use Boltzman-Maxwell statistics to deduce Plank Formula. (We have to consider quantum energy spectrum as Plank did.)
If the energy spectrum is: , , , ...
Then use Boltzman-Maxwell statistics:
So, the average particle number in energy state is . (This is just the result of Bose-Einstein statistics.)
so:
,
this reflects the phenomenon of black body irradiation, which is called Plank Formula.