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Stefan's law.
Explanation:
From Stefan-Boltzman's law, the energy of the thermal radiation emitted per unit time by a blackbody of surface area A is given by,
$\text{u}=\sigma\text{AT}^4$
Where $\sigma$ is Stefan's constant.
Suppose a body at temperature T is kept in a room at temperature T0.
According to Stefan's law, energy of the thermal radiation emitted by the body per unit time is.
$\text{u}=\text{e}\sigma\text{AT}^4$
Here, e is the emissivity of the body.
The energy absorbed per unit time by the body is (due to the radiation emitted by the walls of the room)
$\text{u}_0=\text{e}\sigma\text{AT}^4_0$
Thus, the net loss of thermal energy per unit time is.
$\triangle\text{u}=\text{u}-\text{u}_0$
$\triangle\text{u}=\text{e}\sigma\text{A}(\text{T}^4-\text{T}_0^4)\ \dots(1)$
Newton law of cooling is given by,
$\frac{\text{dT}}{\text{dt}}=-\text{bA}(\text{T}-\text{T}_0)$
This can be obtained from equation (i) by considering the temperature difference to be small and doing the binomial expansion.