The energy per unit area per unit time per unit wavelength interval emitted by a blackbody at
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At a specific temperature, the total power radiated per unit area of the blackbody is equal to the area under the corresponding Iλ versus λ curve. Use this to derive the StefanBoltzmann Law.
Use the fact that
where the gamma function is given by Î(n + 1) = n! and the Riemann zeta function for n = 3 is
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