Difficulty: Easy
Correct Answer: proportional to
Explanation:
Concept/ApproachStefan–Boltzmann law: E = σT⁴ for a black body, where σ is the Stefan–Boltzmann constant.
InterpretationThe phrasing is that emissive power is proportional to the fourth power of absolute temperature (with σ as the constant of proportionality).
Final Answerproportional to
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