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: ''This article is about a type of transform used in classical [[potential theory]], a topic in [[mathematics]]. ''
 
The '''Kelvin transform''' is a device used in classical [[potential theory]] to extend the concept of a [[harmonic function]], by allowing the definition of a function which is 'harmonic at infinity'. This technique is also used in the study of [[Subharmonic function|subharmonic]] and [[Superharmonic function|superharmonic]] functions.
 
In order to define the Kelvin transform ''f''<sup>*</sup> of a function ''f'', it is necessary to first consider the concept of inversion in a sphere in '''R'''<sup>''n''</sup> as follows.
 
It is possible to use inversion in any sphere, but the ideas are clearest when considering a sphere with centre at the origin.
 
Given a fixed sphere ''S''(0,''R'') with centre 0 and radius ''R'', the inversion of a point ''x'' in '''R'''<sup>''n''</sup> is defined to be
 
::<math>x^* = \frac{R^2}{|x|^2} x.</math>
 
A useful effect of this inversion is that the origin 0 is the image of <math>\infty</math>, and <math>\infty</math> is the image of 0. Under this inversion, spheres are transformed into spheres, and the exterior of a sphere is transformed to the interior, and vice versa.
 
The Kelvin transform of a function is then defined by:
 
If ''D'' is an open subset of '''R'''<sup>''n''</sup> which does not contain 0, then for any function ''f'' defined on ''D'', the Kelvin transform ''f''<sup>*</sup> of ''f'' with respect to the sphere ''S''(0,''R'') is
:<math>f^*(x^*) = \frac{|x|^{n-2}}{R^{2n-4}}f(x) = \frac{1}{|x^*|^{n-2}}f(x)=\frac{1}{|x^*|^{n-2}}f\left(\frac{R^2}{|x^*|^2} x^*\right).</math>
 
One of the important properties of the Kelvin transform, and the main reason behind its creation, is the following result:
 
:Let ''D'' be an open subset in '''R'''<sup>''n''</sup> which does not contain the origin 0. Then a function ''u'' is harmonic, subharmonic or superharmonic in ''D'' if and only if the Kelvin transform ''u''<sup>*</sup> with respect to the sphere ''S''(0,''R'') is harmonic, subharmonic or superharmonic in ''D''<sup>*</sup>.
 
This follows from the formula
:<math>\Delta u^*(x^*)=\frac{R^{4}}{|x^*|^{n+2}}(\Delta u)\left(\frac{R^2}{|x^*|^2} x^*\right).</math>
 
==See also==
 
*[[William Thomson, 1st Baron Kelvin]]
*[[Inversive geometry]]
 
==References==
 
*{{cite book | author = [[Joseph Leo Doob|J. L. Doob]] | title = Classical Potential Theory and Its Probabilistic Counterpart | publisher = Springer-Verlag | year = 2001 | isbn=3-540-41206-9 }}
 
*{{cite book | author = L. L. Helms | title = Introduction to potential theory | publisher = R. E. Krieger | year = 1975 | isbn=0-88275-224-3 }}
 
*{{cite book | author = [[Oliver Dimon Kellogg|O. D. Kellogg]] | title = Foundations of potential theory | publisher = Dover | year = 1953 | isbn=0-486-60144-7 }}
 
[[Category:Harmonic functions]]
[[Category:Transforms]]

Revision as of 19:19, 2 February 2014

This article is about a type of transform used in classical potential theory, a topic in mathematics.

The Kelvin transform is a device used in classical potential theory to extend the concept of a harmonic function, by allowing the definition of a function which is 'harmonic at infinity'. This technique is also used in the study of subharmonic and superharmonic functions.

In order to define the Kelvin transform f* of a function f, it is necessary to first consider the concept of inversion in a sphere in Rn as follows.

It is possible to use inversion in any sphere, but the ideas are clearest when considering a sphere with centre at the origin.

Given a fixed sphere S(0,R) with centre 0 and radius R, the inversion of a point x in Rn is defined to be

x*=R2|x|2x.

A useful effect of this inversion is that the origin 0 is the image of , and is the image of 0. Under this inversion, spheres are transformed into spheres, and the exterior of a sphere is transformed to the interior, and vice versa.

The Kelvin transform of a function is then defined by:

If D is an open subset of Rn which does not contain 0, then for any function f defined on D, the Kelvin transform f* of f with respect to the sphere S(0,R) is

f*(x*)=|x|n2R2n4f(x)=1|x*|n2f(x)=1|x*|n2f(R2|x*|2x*).

One of the important properties of the Kelvin transform, and the main reason behind its creation, is the following result:

Let D be an open subset in Rn which does not contain the origin 0. Then a function u is harmonic, subharmonic or superharmonic in D if and only if the Kelvin transform u* with respect to the sphere S(0,R) is harmonic, subharmonic or superharmonic in D*.

This follows from the formula

Δu*(x*)=R4|x*|n+2(Δu)(R2|x*|2x*).

See also

References

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  • 20 year-old Real Estate Agent Rusty from Saint-Paul, has hobbies and interests which includes monopoly, property developers in singapore and poker. Will soon undertake a contiki trip that may include going to the Lower Valley of the Omo.

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  • 20 year-old Real Estate Agent Rusty from Saint-Paul, has hobbies and interests which includes monopoly, property developers in singapore and poker. Will soon undertake a contiki trip that may include going to the Lower Valley of the Omo.

    My blog: http://www.primaboinca.com/view_profile.php?userid=5889534