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1
Planck's law describes the spectral radiance of electromagnetic radiation emitted by a black body as a function of its temperature and wavelength, introducing energy quantization.
2
The Stefan–Boltzmann law states that the total energy radiated per unit surface area of a black body is directly proportional to the fourth power of its absolute temperature.
3
Wien's Displacement Law states that the peak wavelength of emitted electromagnetic radiation from a black body is inversely proportional to its absolute temperature.
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