PlanetPhysics/Derivation of Heat Equation
Let us consider the [[../Heat/|heat]] [[../Conduction/|conduction]] in a homogeneous matter with density and specific heat capacity .\, Denote by \,\, the [[../BoltzmannConstant/|temperature]] in the point \,\, at the time .\, Let be a simple closed surface in the matter and the spatial region restricted by it.
When the growth of the temperature of a [[../Volume/|volume]] element in the time is , the element releases the amount of heat, which is the heat [[../AbsoluteMagnitude/|flux]] through the surface of .\, Thus if there are no sources and sinks of heat in , the heat flux through the surface in is
On the other hand, the flux through in the time must be proportional to , to and to the derivative of the temperature in the direction of the normal line of the surface element , i.e. the flux is where is a positive constant (because the heat flows always from higher temperature to lower one).\, Consequently, the heat flux through the whole surface is which is, by the Gauss's [[../Formula/|theorem]], same as
Equating the expressions (1) and (2) and dividing by , one obtains Since this equation is valid for any region in the matter, we infer that Denoting\, ,\, we can write this equation as
This is the [[../DifferentialEquations/|differential equation]] of heat conduction, first derived by Fourier.