Asked by Daniel Park
electromagnetic radiation models: apply
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GPT 3.5
1. Planck's law: Describes the spectral distribution of electromagnetic radiation emitted by a black body at a given temperature.
2. Stefan-Boltzmann law: Describes the total power radiated per unit area by a black body at a given temperature.
3. Wien's law: Describes the relationship between the temperature of a black body and the peak wavelength of the radiation emitted.
4. Rayleigh-Jeans law: Describes the spectral distribution of electromagnetic radiation at low frequencies, which is applicable to the Rayleigh-Jeans region of the black body spectrum.
5. Kirchhoff's law: Describes the relationship between the absorption and emission of electromagnetic radiation by a material at thermodynamic equilibrium.
2. Stefan-Boltzmann law: Describes the total power radiated per unit area by a black body at a given temperature.
3. Wien's law: Describes the relationship between the temperature of a black body and the peak wavelength of the radiation emitted.
4. Rayleigh-Jeans law: Describes the spectral distribution of electromagnetic radiation at low frequencies, which is applicable to the Rayleigh-Jeans region of the black body spectrum.
5. Kirchhoff's law: Describes the relationship between the absorption and emission of electromagnetic radiation by a material at thermodynamic equilibrium.
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