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Planck's law describes the spectral density of electromagnetic radiation emitted by a black body in thermal equilibrium at a given temperature. Formulated by Max Planck in 1900, it provides a theoretical foundation for understanding black body radiation. The law states that the intensity of radiation emitted at a specific wavelength is proportional to the wavelength and depends on the temperature of the black body.

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  1. Statistical mechanics
  2. Applied probability
  3. Applied mathematics
  4. Fields of mathematics
  5. Mathematics
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