Heat conduction, or thermal conduction, is the spontaneous transfer of thermal energy through matter, from a region at higher temperature to a region at lower temperature. It thus acts to equalize temperature differences. It is also described as heat energy transferred from one material to another by direct contact.
Thermal energy, in the form of continuous random motion of particles of matter, is transferred by the same coulomb forces that act to support the structure of matter. For this reason, its transfer can be said to occur by physical contact between the particles.
Besides conduction, heat can also be transferred by radiation and convection, and often more than one of these processes may occur in a given situation.
The law of heat conduction, also known as Fourier's law, states that the time rate of heat transfer through a material is proportional to the negative gradient in the temperature and to the area at right angles, to that gradient, through which the heat is flowing. This law can be stated in two equivalent forms:
In the differential formulation of Fourier's law, the fundamental quantity is the local heat flux . This is the amount of energy flowing through an infinitesimal oriented surface per unit of time. The length of is given by the amount of energy per unit of time, and the direction is given by the vector perpendicular to the surface. As a vector equation, this leads to:
where (showing the terms in SI units)
Note that the thermal conductivity of a material generally varies with temperature, but the variation can be small over a significant range of temperatures for some common materials. In anisotropic materials, the thermal conductivity typically varies with direction; in this case, is a tensor.
By integrating the differential form over the material's total surface , we arrive at the integral form of Fourier's law:
where (showing the terms in SI units)
Consider a simple linear situation (see diagram), where there is uniform temperature across equally sized end surfaces and the sides are perfectly insulated. In such a case, integration of the above differential equation gives the heat flow rate between the end surfaces as:
This law forms the basis for derivation of the heat equation.
The R-value is the unit for heat resistance, the reciprocal of heat conductance.
Ohm's law is the electrical analog of Fourier's law.
The conductance () can be defined as:
where the units for are given in W/(m2 K).
Thus, Fourier's law can also be stated as:
The reciprocal of conductance is resistance, R. It is given by:
Resistance is additive when several conducting layers lie between the hot and cool regions, because A and Q are the same for all layers. In a multilayer partition, the total conductance is related to the conductance of its layers by the following equation:
So, when dealing with a multilayer partition, the following formula is usually used:
When heat is being conducted from one fluid to another through a barrier, it is sometimes important to consider the conductance of the thin film of fluid which remains stationary next to the barrier. This thin film of fluid is difficult to quantify, its characteristics depending upon complex conditions of turbulence and viscosity, but when dealing with thin high-conductance barriers it can sometimes be quite significant.
The previous conductance equations written in terms of extensive properties, can be reformulated in terms of intensive properties.
Ideally, the formulae for conductance should produce a quantity with dimensions independent of distance, like Ohm's Law for electrical resistance: , and conductance: .
From the electrical formula: , where ρ is resistivity, x = length, A cross sectional area, we have , where G is conductance, k is conductivity, x = length, A cross sectional area.
where U is the conductance.
Fourier's law can also be stated as:
analogous to Ohm's law: or
The reciprocal of conductance is resistance, R, given by:
analogous to Ohm's law:
The sum of conductances in series is still correct.
All links retrieved February 13, 2014.
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