Question:

The dimension of radiant emittance of a blackbody as per Stefan-Boltzmann law is:

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The Stefan-Boltzmann law relates radiant emittance to the fourth power of temperature, which gives the dimension of radiant emittance as \( M^1 L^0 T^{-3} \).
Updated On: Dec 26, 2025
  • \( M^0 L^1 T^{-1} \)
  • \( M^1 L^{-1} T^{-2} \)
  • \( M^1 L^2 T^{-2} \)
  • \( M^1 L^0 T^{-3} \)
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The Correct Option is D

Solution and Explanation

The Stefan-Boltzmann law states that the radiant emittance of a blackbody is proportional to the fourth power of its temperature. The radiant emittance \( E \) is given by: \[ E = \sigma T^4 \] where \( \sigma \) is the Stefan-Boltzmann constant, and \( T \) is the temperature. The dimensions of \( E \) are given by: \[ E = \frac{\text{Energy}}{\text{Area} \cdot \text{Time}} = \frac{M L^2 T^{-2}}{L^2 T} = M T^{-3} \] Thus, the dimension of radiant emittance is \( M^1 L^0 T^{-3} \). Final Answer: (D) \( M^1 L^0 T^{-3} \)
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