What is Stefan Boltzmann law?
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total energy emitted is proportional to (absolute temperature)⁴
MauryaAJ:
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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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