A black body radiates energy at the rate of $E$ $W/m^2$ at a high temperature $TK$ . When the temperature is reduced to $\frac{T}{2}K$, the radiant energy will be
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(a) $E \propto {T^4} \Rightarrow \frac{{{E_1}}}{{{E_2}}} = \frac{{{T^4}}}{{{T^4}}} \times {2^4} \Rightarrow {E_2} = \frac{E}{{16}}$
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