According to Stefan-Boltzmann law, the radiant energy emitted per unit area per unit time by a blackbody is proportional to
Options
- A. T
- B. T²
- C. T³
- D. T⁴
- E. None of the above
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Correct Answer (Detailed Explanation is Below)
D. T⁴
Detailed Explanation
Stefan-Boltzmann law states that the emissive power of a blackbody is proportional to the fourth power of its absolute temperature.
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