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1) The energy radiated by a blackbody element equals the energy received from the surrounding cavity at thermal equilibrium. The radiance R(ν) equals 4 times the energy density ρ(ν) divided by the speed of light. 2) Using classical physics, the average energy of standing waves depends only on temperature. But Planck hypothesized energy comes in multiples of hν. This leads to the Planck distribution and blackbody radiation formula. 3) In the high-temperature limit, the Planck distribution reduces to the
- Author
- darshan sethia
- Language
- EN