The energy per unit area per unit time per wavelength interval emitted by a blackbody at a temperature T' is given by
At a specific temperature, the total power radiated per unit area of the blackbody is equal to the area under the corresponding Iλ versus A curve. Use this to derive the Stefan-Boltzmann Law. [Hint: To clean up the exponential, change variables in the integral so that
Use the fact that where the gamma function is given by and the Riemann zeta function for n = 3 is
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