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Latest revision as of 16:27, 25 July 2021


A transformation of functions defined in domains of a Euclidean space , n \geq 3 , under which harmonic functions are transformed to harmonic functions. It was obtained by W. Thomson (Lord Kelvin, [1]).

If u is a harmonic function in a domain D \subset \mathbf R ^ {n} , then its Kelvin transform is the function

v ( y) = \ \left ( \frac{R}{| y | } \right ) ^ {n-2} u \left ( \frac{R ^ {2} }{| y | ^ {2} } y \right ) ,\ \ v ( \infty ) = 0 ,

which is harmonic in the domain D ^ {*} obtained from D by inversion in the sphere S _ {R} = \{ {x } : {| x | = R } \} , that is, by the mapping of \mathbf R ^ {n} defined by

x \rightarrow y = \ \frac{R ^ {2} }{| x | ^ {2} } x ,\ \ 0 \rightarrow \infty ,

where

x = ( x _ {1} \dots x _ {n} ) ,\ \ | x | = ( x _ {1} ^ {2} + \dots + x _ {n} ^ {2} ) ^ {1/2} .

Under the inversion, the point at infinity \infty of the Aleksandrov compactification \overline{ {\mathbf R ^ {n} }}\; is taken to the origin 0 and vice versa. Under the Kelvin transformation, harmonic functions u in domains D containing \infty that are regular at \infty , that is, are such that \lim\limits _ {| x | \rightarrow \infty } u ( x) = 0 , are transformed to harmonic functions v in bounded domains D ^ {*} containing the origin 0 , moreover, v ( 0) = 0 . Because of this property, the Kelvin transformation enables one to reduce exterior problems in potential theory to interior ones and vice versa (see [2], [3]).

Apart from under Kelvin transformation, harmonicity of functions in \mathbf R ^ {n} , n \geq 3 , is preserved under analytic transformations of the form v ( y) = \phi ( y) u ( \psi ( y) ) only in the case when \phi ( y) \equiv 1 and \psi is a homothety, a translation or a symmetry with respect to a plane; for n = 2 the large class of conformal mappings \psi has this property.

References

[1] W. Thomson, "Extraits de deux letters adressées à M. Liouville" J. Math. Pures Appl. , 12 (1847) pp. 256–264
[2] V.S. Vladimirov, "Equations of mathematical physics" , MIR (1984) pp. Chapt. 5 (Translated from Russian)
[3] M. Brélot, "Eléments de la théorie classique du potentiel" , Sorbonne Univ. Centre Doc. Univ. , Paris (1959)

Comments

These results hold for n = 2 as well. In this case, harmonicity of u at infinity corresponds to boundedness of u at 0 . See, e.g., [a1] or [a2].

References

[a1] L.L. Helms, "Introduction to potential theory" , Wiley (1969) (Translated from German)
[a2] J. Wermer, "Potential theory" , Lect. notes in math. , 408 , Springer (1974)
[a3] O.D. Kellogg, "Foundations of potential theory" , Dover, reprint (1954) (Re-issue: Springer, 1967)
[a4] J.L. Doob, "Classical potential theory and its probabilistic counterpart" , Springer (1984) pp. 390
How to Cite This Entry:
Kelvin transformation. Encyclopedia of Mathematics. URL: http://encyclopediaofmath.org/index.php?title=Kelvin_transformation&oldid=51764
This article was adapted from an original article by E.D. Solomentsev (originator), which appeared in Encyclopedia of Mathematics - ISBN 1402006098. See original article