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.
The given can be listed as, h= 20m g = 9.8m/s² To find, v = ? Solution -…
A wave in which the disturbance produced in the medium travels in a given …
(1) Constructive interference (brightness): There is constructive interfer…