Step 1: The spectral density u(\lambda, T) of blackbody radiation is given by Planck's law, which is u(\lambda, T) = (8Ď€hc) / (\lambda^5 * (exp(hc / (\lambda * k * T)) - 1)), where h is the Planck constant, c is the speed of light, k is the Boltzmann constant, T is
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