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Space form : ウィキペディア英語版
Space form
In mathematics, a space form is a complete Riemannian manifold ''M'' of constant sectional curvature ''K''. The three obvious examples are Euclidean ''n''-space, the ''n''-dimensional sphere, and hyperbolic space, although a space form need not be simply connected.
==Reduction to generalized crystallography==

The Killing–Hopf theorem of Riemannian geometry states that the universal cover of an ''n''-dimensional space form M^n with curvature K = -1 is isometric to H^n, hyperbolic space, with curvature K = 0 is isometric to R^n, Euclidean ''n''-space, and with curvature K = +1 is isometric to S^n, the n-dimensional sphere of points distance 1 from the origin in R^.
By rescaling the Riemannian metric on H^n, we may create a space M_K of constant curvature K for any K < 0. Similarly, by rescaling the Riemannian metric on S^n, we may create a space M_K of constant curvature K for any K > 0. Thus the universal cover of a space form M with constant curvature K is isometric to M_K.
This reduces the problem of studying space form to studying discrete groups of isometries \Gamma of M_K which act properly discontinuously. Note that the fundamental group of M, \pi_1(M), will be isomorphic to \Gamma. Groups acting in this manner on R^n are called crystallographic groups. Groups acting in this manner on H^2 and H^3 are called Fuchsian groups and Kleinian groups, respectively.

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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