What is the Stefan-Boltzmann law?
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The Stefan-Boltzmann law is a fundamental principle of thermodynamics that relates the total energy radiated by a blackbody to its temperature. It states that the total power radiated per unit surface area of a blackbody is proportional to the fourth power of its absolute temperature, as expressed by the equation P = σ * A * T^4, where P is the total power radiated, A is the surface area, T is the absolute temperature, and σ is the Stefan-Boltzmann constant.