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