Q.40. A black body radiates maximum energy at wavelength ‘λ’ and its emissive power is E. Now due to change in temperature of that body, it radiates maximum energy at wavelength \frac{2\lambda}{3} . At that temperature emissive power is
A. \frac{51E}{8}
B. \frac{81E}{16}
C. \frac{61E}{27}
D. \frac{71E}{19}
Answer :- B. \frac{81E}{16}
Explanation :-
From Wien’s Displacement Law,
\lambda_{\max } = \frac{b}{T} \Rightarrow T = \frac{b}{\lambda_{\max }}From Stefan-Boltzmann Law,
E = \sigma T^4 = \sigma \left( \frac{b}{\lambda_{\max }} \right)^4Let the new emissive power be \mathrm{E}^{\prime} .
\therefore \quad E^{\prime} = \sigma \left( \frac{b}{\frac{2 \lambda_{\max }}{3}} \right)^4