Heat equation

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(Redirected from Diffusion equation)

The heat equation or diffusion equation is an important partial differential equation which describes the variation of temperature in a given region over time. In the special case of heat propagation in an isotropic and homogeneous medium in the 3-dimensional space, this equation is

<math>u_t = k ( u_{xx} + u_{yy} + u_{zz} ) \quad <math>

where:

  • u(t, x, y, z) is temperature as a function of time and space;
  • ut is the rate of change of temperature at a point over time;
  • <math>u_{xx}<math>, <math>u_{yy}<math>, and <math>u_{zz}<math> are the second spatial derivatives (thermal conductions) of temperature in the x, y, and z directions, respectively

To solve the heat equation, we also need to specify boundary conditions for u.

Solutions of the heat equation are characterized by a gradual smoothing of the initial temperature distribution by the flow of heat from warmer to colder areas of an object.

The heat equation is the prototypical example of a parabolic partial differential equation.

Using the Laplace operator, the heat equation can be generalized to

<math>u_t = k \Delta u \quad <math>

Heat conduction in non-homogeneous anisotropic media

In general, the study of heat conduction is based on several principles. Heat flow is a form of energy flow, and as such it is meaningful to speak of the time rate of flow of heat into a region of space.

  • The time rate of heat flow into a region V is given by a time-dependent quantity qt(V). We assume q has a density, so that
<math> q_t(V) = \int_V Q(t,x)\,d x \quad <math>
  • Heat flow is a time-dependent vector function H(x) characterized as follows: the time rate of heat flowing through an infinitesimal surface element with area d S and with unit normal vector n is
<math> \mathbf{H}(x) \cdot \mathbf{n}(x) \, dS <math>

Thus the rate of heat flow into V is also given by the surface integral

<math> q_t(V)= - \int_{\partial V} \mathbf{H}(x) \cdot \mathbf{n}(x) \, dS <math>

where n(x) is the outward pointing normal vector at x.

  • The Fourier law states that heat energy flow has the following linear dependence on the temperature gradient
<math> \mathbf{H}(x) = -\mathbf{A}(x) \cdot [\operatorname{grad}(u)] (x) <math>
where A(x) is a 3 × 3 real matrix, which in fact is symmetric and non-negative.

By Green's theorem, the previous surface integral for heat flow into V can be transformed into the volume integral

<math> q_t(V) = - \int_{\partial V} \mathbf{H}(x) \cdot \mathbf{n}(x) \, dS <math>
<math> = \int_{\partial V} \mathbf{A}(x) \cdot [\operatorname{grad}(u)] (x) \cdot \mathbf{n}(x) \, dS <math>
<math> = \int_V \sum_{i, j} \partial_{x_i} a_{i j} \partial_{x_j} u (t,x)\,dx <math>
  • The time rate of temperature change at x is proportional to the heat flowing into an infinitesimal volume element, where the constant of proportionality is dependent on a constant κ
<math> \partial_t u(t,x) = \kappa(x) Q(t,x)\, dx<math>

Putting these equations together gives the general equation of heat flow:

<math> \partial_t u(t,x) = \kappa(x) \sum_{i, j} \partial_{x_i} a_{i j} \partial_{x_j} u (t,x) <math>

Remarks.

  • The constant κ(x) is the inverse of specific heat of the substance at x × density of the substance at x.
  • In the case of an isotropic medium, the matrix A is a scalar matrix equal to thermal conductivity.
  • The Jacobi theta function is the unique solution to the one-dimensional heat equation with periodic boundary conditions at t = 0.

External links

de:Wrmeleitungsgleichung ru:Уравнение диффузии sl:difuzijska enačba

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