(i) The Stefan-Boltzmann law : 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. 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.
(ii) Wien’s displacement law : The wavelength for which the emissive power of a blackbody is maximum, is inversely proportional to the absolute temperature of the blackbody.
OR
For a blackbody at an absolute temperature T, the product of T and the wavelength λm corresponding to the maximum radiation of energy is a constant.
λm T = b, a constant.
Notes:
(1) The law stated above was stated by Wilhelm Wien (1864-1928) German Physicist.
(2) The value of the constant b in Wien’s displacement law is 2.898 × 10-3 m.K.