The splitting theorem for orbifolds
The splitting theorem for orbifolds
复制标题
轨道折叠定理
DOI:
10.1215/ijm/1256060999
复制
发表时间:
1994
影响因子:
0.6
通讯作者:
Shunhui Zhu
中科院分区:
文献类型:
--
作者:
Joseph E. Borzellino;Shunhui Zhu
In this paper we wish to examine a generalization of the splitting theorem of Cheeger–Gromoll [CG] to Riemannian orbifolds. Roughly speaking, a Riemannian orbifold is a metric space locally modelled on quotients of Riemannian manifolds by finite groups of isometries. The term orbifold was coined by W. Thurston [T] sometime around the year 1976–77. The term is meant to suggest the orbit space of a group action on a manifold. A similar concept was introduced by I. Satake in 1956, where he used the term V– manifold (See [S1]). The “V” was meant to suggest a cone–like singularity. Since then, orbifold has become the preferred terminology. Recall that if M is a complete connected n–dimensional Riemannian manifold with nonnegative Ricci curvature that contains a line, then the Cheeger– Gromoll Splitting Theorem [CG] states that that M is isometric to N × R. Recall that a line is a unit speed geodesic γ : R → M such that for any s, t ∈ R, d(γ(s), γ(t)) = |s− t|.