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isothermal coordinates : ウィキペディア英語版
isothermal coordinates
In mathematics, specifically in differential geometry, isothermal coordinates on a Riemannian manifold
are local coordinates where the metric is
conformal to the Euclidean metric. This means that in isothermal
coordinates, the Riemannian metric locally has the form
: g = e^\varphi (dx_1^2 + \cdots + dx_n^2),
where \varphi is a smooth function.
Isothermal coordinates on surfaces were first introduced by Gauss. Korn and Lichtenstein proved that isothermal coordinates exist around any point on a two dimensional Riemannian manifold. On higher-dimensional Riemannian manifolds a necessary and sufficient condition for their local existence is the vanishing of the Weyl tensor and of the Cotton tensor.
==Isothermal coordinates on surfaces==
proved the existence of isothermal coordinates on an arbitrary surface with a real analytic metric, following results of
on surfaces of revolution. Results for Hölder continuous metrics were obtained by and . Later accounts were given by , , and . A particularly simple account using the Hodge star operator is given in .

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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