Stefan--Boltzmann law
= Stefan--Boltzmann law
{c}
{title2=$F=\epsilon\sigma T^4$}
{wiki}
The Stefan--Boltzmann law gives the thermal-radiation flux emitted by a surface as $F=\epsilon\sigma T^4$, where $\epsilon$ is its <emissivity> and $\sigma$ is the Stefan--Boltzmann constant.