Stefan boltzmann law of radiation
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The Stefan–Boltzmann constant (also Stefan's constant), a physicalconstant denoted by the Greek letter σ (sigma), is theconstant of proportionality in the Stefan–Boltzmann law: "the total intensity radiated over all wavelengths increases as the temperature increases", of a black body which is proportional to the ...
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Answer:
The Stefan-Boltzmann law: The rate of emission
of radiant energy per unit area or the power radi-
ated per unit area of a perfect blackbody is directly
proportional to the fourth power of its absolute
temperature. OR
The quantity of radiant energy emitted by a
perfect blackbody per unit time per unit surface
area of the body is directly proportional to the
fourth power of its absolute temperature.
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