statement that the total radiant heat energy emitted from a surface is proportional to the fourth power of its absolute temperature. Formulated in ... [4 related articles]
Found on
http://www.britannica.com/eb/a-z/s/158
In physics, a law that relates the energy, E, radiated away from a perfect emitter (a black body), to the temperature, T, of that body. It has the form E = σT4, where E is the energy radiated per unit area per second,
Found on
https://www.encyclo.co.uk/local/21221
the law stating that the total energy radiated from a blackbody is proportional to the fourth power of its absolute temperature. Also called
Found on
https://www.infoplease.com/dictionary/stefan-boltzmann-law
No exact match found.
