# classical photons

27 Nov 2013the flux density of a blackbody would have form \(S(\omega) \propto \omega^3\exp\left(-\frac{\hbar\omega}{k_BT}\right)\) if the photons were classical distinguishable particles. Can you derive Wienâ€™s displacement law and the Stefan-Boltzmann law and point out the differences to the Planck-spectrum?