Step 1: Newton's Law of Cooling.
Newton's Law of Cooling posits that an object's temperature change rate is proportional to the temperature difference between the object and its surroundings.
Step 2: Stefan's Law.
Stefan-Boltzmann Law states that a black body's radiated energy is proportional to the fourth power of its temperature (\(T^4\)). This law models an object's radiative cooling based on the temperature difference with its environment.
Step 3: Conclusion.
In conclusion, Newton’s Law of Cooling is a specific instance of Stefan's Law, applicable when the temperature differential is minimal, and radiation behaves linearly.
Final Answer: \[ \boxed{\text{Stefan's law}} \]