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Poincaré metric : ウィキペディア英語版
Poincaré metric
In mathematics, the Poincaré metric, named after Henri Poincaré, is the metric tensor describing a two-dimensional surface of constant negative curvature. It is the natural metric commonly used in a variety of calculations in hyperbolic geometry or Riemann surfaces.
There are three equivalent representations commonly used in two-dimensional hyperbolic geometry. One is the Poincaré half-plane model, defining a model of hyperbolic space on the upper half-plane. The Poincaré disk model defines a model for hyperbolic space on the unit disk. The disk and the upper half plane are related by a conformal map, and isometries are given by Möbius transformations. A third representation is on the punctured disk, where relations for q-analogues are sometimes expressed. These various forms are reviewed below.
==Overview of metrics on Riemann surfaces==
A metric on the complex plane may be generally expressed in the form
:ds^2=\lambda^2(z,\overline)\, dz\,d\overline
where λ is a real, positive function of z and \overline. The length of a curve γ in the complex plane is thus given by
:l(\gamma)=\int_\gamma \lambda(z,\overline)\, |dz|
The area of a subset of the complex plane is given by
:\text(M)=\int_M \lambda^2 (z,\overline)\,\frac\,dz \wedge d\overline
where \wedge is the exterior product used to construct the volume form. The determinant of the metric is equal to \lambda^4, so the square root of the determinant is \lambda^2. The Euclidean volume form on the plane is dx\wedge dy and so one has
:dz \wedge d\overline=(dx+i\,dy)\wedge (dx-i \, dy)= -2i\,dx\wedge dy.
A function \Phi(z,\overline) is said to be the potential of the metric if
:4\frac
\frac)=\lambda^2(z,\overline).
The Laplace–Beltrami operator is given by
:\Delta = \frac
\frac
\frac \left(
\frac +
\frac
\right).
The Gaussian curvature of the metric is given by
:K=-\Delta \log \lambda.\,
This curvature is one-half of the Ricci scalar curvature.
Isometries preserve angles and arc-lengths. On Riemann surfaces, isometries are identical to changes of coordinate: that is, both the Laplace–Beltrami operator and the curvature are invariant under isometries. Thus, for example, let ''S'' be a Riemann surface with metric \lambda^2(z,\overline)\, dz \, d\overline and ''T'' be a Riemann surface with metric \mu^2(w,\overline)\, dw\,d\overline. Then a map
:f:S\to T\,
with f=w(z) is an isometry if and only if it is conformal and if
:\mu^2(w,\overline) \;
\frac
\frac } =
\lambda^2 (z, \overline )
.
Here, the requirement that the map is conformal is nothing more than the statement
:w(z,\overline)=w(z),
that is,
:\frac{\partial \overline{z}} w(z) = 0.

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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