Definitions for "Stefan-Boltzmann law"
the rate at which an object radiates energy is proportional to its surface area and to the fourth power of its absolute temperature (see equation 11.11)
The radiation law that states that the energy emitted by a black body varies with the fourth power of the temperature.
Formula that relates the emission (E) of electromagnetic radiation by a blackbody to the fourth power of its temperature (T), E oc T4.