PHYSICS
Stefan-Boltzmann Law
The law states that the rate of emission of radiant energy per unit area or the power radiated per unit area of a perfect blackbody is directly proportional to the fourth power of its absolute temperature.
The law states that the rate of emission of radiant energy per unit area or the power radiated per unit area of a perfect blackbody is directly proportional to the fourth power of its absolute temperature.
While learning thermodynamics we come across many terms , out of that some…
we can list out the given as, Power P= 100W current , I = 3A To find , R…
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