The area under the curve drawn between the spectral emissive power Eλ, wavelength λ at a given temperature T for a black body is proportional to
A
T
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B
1T
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C
T4
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D
T5
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Solution
The correct option is BT4 The power emitted by a black body is given by Stefan's law: P=σAeT4 for a black body e=1; P=σAT4 And Energy spectral power =P=Eλ Which is proportional to T4