PlanetPhysics/Derivation of Heat Equation

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Let us consider the [[../Heat/|heat]] [[../Conduction/|conduction]] in a homogeneous matter with density ϱ and specific heat capacity c.\, Denote by \,u(x,y,z,t)\, the [[../BoltzmannConstant/|temperature]] in the point \,(x,y,z)\, at the time t.\, Let a be a simple closed surface in the matter and v the spatial region restricted by it.

When the growth of the temperature of a [[../Volume/|volume]] element dv in the time dt is du, the element releases the amount ducϱdv=u'tdtcϱdv of heat, which is the heat [[../AbsoluteMagnitude/|flux]] through the surface of dv.\, Thus if there are no sources and sinks of heat in v, the heat flux through the surface a in dt is

dtvcϱu'tdv.

On the other hand, the flux through da in the time dt must be proportional to a, to dt and to the derivative of the temperature in the direction of the normal line of the surface element da, i.e. the flux is kudadt, where k is a positive constant (because the heat flows always from higher temperature to lower one).\, Consequently, the heat flux through the whole surface a is dtakuda, which is, by the Gauss's [[../Formula/|theorem]], same as

dtvkudv=dtvk2udv.

Equating the expressions (1) and (2) and dividing by dy, one obtains vk2udv=vcϱu'tdv. Since this equation is valid for any region v in the matter, we infer that k2u=cϱu't. Denoting\, kcϱ=α2,\, we can write this equation as

α22u=ut.

This is the [[../DifferentialEquations/|differential equation]] of heat conduction, first derived by Fourier.

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