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Laplacian field : ウィキペディア英語版
Harmonic function

In mathematics, mathematical physics and the theory of stochastic processes, a harmonic function is a twice continuously differentiable function ''f'' : ''U'' → R (where ''U'' is an open subset of R''n'') which satisfies Laplace's equation, i.e.
: \frac + \frac + \cdots + \frac = 0
everywhere on ''U''. This is usually written as
: \nabla^2 f = 0
or
:\textstyle \Delta f = 0
== Examples ==
Examples of harmonic functions of two variables are:
* The real or imaginary part of any holomorphic function
* The function \,\! f(x,y)=e^ \sin y; this is a special case of the example above, as f(x,y)=\operatorname(e^), and e^ is a holomorphic function.
* The function
::\,\! f(x_1,x_2)=\ln (x_1^2+x_2^2)
: defined on \mathbb^2 \setminus \lbrace 0 \rbrace (e.g. the electric potential due to a line charge, and the gravity potential due to a long cylindrical mass)
Examples of harmonic functions of three variables are given in the table below with r^2=x^2+y^2+z^2:
:
|Unit point charge at origin
|-
|align=center|\frac
|x-directed dipole at origin
|-
|align=center|-\ln(r^2-z^2)\,
|Line of unit charge density on entire z-axis
|-
|align=center|-\ln(r+z)\,
|Line of unit charge density on negative z-axis
|-
|align=center|\frac\,
|Line of x-directed dipoles on entire z axis
|-
|align=center|\frac\,
|Line of x-directed dipoles on negative z axis
|}
Harmonic functions that arise in physics are determined by their singularities and boundary conditions (such as Dirichlet boundary conditions or Neumann boundary conditions). On regions without boundaries, adding the real or imaginary part of any entire function will produce a harmonic function with the same singularity, so in this case the harmonic function is not determined by its singularities; however, we can make the solution unique in physical situations by requiring that the solution goes to 0 as you go to infinity. In this case, uniqueness follows by Liouville's theorem.
The singular points of the harmonic functions above are expressed as "charges" and "charge densities" using the terminology of electrostatics, and so the corresponding harmonic function will be proportional to the electrostatic potential due to these charge distributions. Each function above will yield another harmonic function when multiplied by a constant, rotated, and/or has a constant added. The inversion of each function will yield another harmonic function which has singularities which are the images of the original singularities in a spherical "mirror". Also, the sum of any two harmonic functions will yield another harmonic function.
Finally, examples of harmonic functions of ''n'' variables are:
* The constant, linear and affine functions on all of R''n'' (for example, the electric potential between the plates of a capacitor, and the gravity potential of a slab)
* The function \,\! f(x_1,\dots,x_n)=(^2+\cdots+^2)^ on \mathbb^n \setminus \lbrace 0 \rbrace for ''n'' > 2.

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
ウィキペディアで「Harmonic function」の詳細全文を読む



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