Stefan-Boltzmann law

[stef-uh n bohlts-muh n; German shte-fahn bawlts-mahn] /ˈstɛf ən ˈboʊlts mən; German ˈʃtɛ fɑn ˈbɔlts mɑn/
noun, Physics.
the law stating that the total energy radiated from a blackbody is proportional to the fourth power of its absolute temperature.


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