Kelvin transform

From Wikipedia, the free encyclopedia

This is an old revision of this page, as edited by BG19bot (talk | contribs) at 06:28, 22 March 2016 (→‎References: Remove blank line(s) between list items per WP:LISTGAP to fix an accessibility issue for users of screen readers. Do WP:GENFIXES and cleanup if needed. Discuss this at Wikipedia talk:WikiProject Accessibility#LISTGAP). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

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

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

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

See also

References

  • J. L. Doob (2001). Classical Potential Theory and Its Probabilistic Counterpart. Springer-Verlag. ISBN 3-540-41206-9.
  • L. L. Helms (1975). Introduction to potential theory. R. E. Krieger. ISBN 0-88275-224-3.
  • O. D. Kellogg (1953). Foundations of potential theory. Dover. ISBN 0-486-60144-7.