Planck's law of black body radiation
In physics, the intensity spectrum of electromagnetic radiation from a black body at temperature T is given by the Planck's law of black body radiation:
- ν is the frequency
- I(ν) is the amount of energy per unit time per unit surface per unit solid angle emitted in the frequency range between ν and ν+δν [W m-2 Hz-1 sr-1];
- h is Planck's constant,:
- c is the speed of light and
- k is Boltzmann's constant.
The Rayleigh-Jeans law was particularly significant, since it was built on a strong theoretical framework, but suffered a serious flaw known as the ultraviolet catastrophe. This suggested that the theoretical framework of thermodynamics was faulty. Planck now attempted to produce a better fundamental theory which would supplement thermodynamics. He calculated that if the sum of different modes of charged oscillators in matter could only be counted where these oscillators have energy proportional to frequency, the new radiation law would fit all spectroscopic measurements.
- E = h ν
From the Planck's law of black body radiation we derive today the Stefan-Boltzmann law.
External link and references