English

The topological rigidity theorem for submanifolds in space forms

Differential Geometry 2019-03-04 v1

Abstract

Let MM be an n(4)n(\geq 4)-dimensional compact submanifold in the simply connected space form Fn+p(c)F^{n+p}(c) with constant curvature c0c\geq 0, where HH is the mean curvature of MM. We verify that if the scalar curvature of MM satisfies R>n(n2)(c+H2)R>n(n-2)(c+H^2), and if RicM(n22σn2nσn)(c+H2)Ric_M\geq (n-2-\frac{2\sigma_n}{2n-\sigma_n})(c+H^2), then MM is homeomorphic to a sphere. Here σn=sgn(n4)((1)n+3)\sigma_n=sgn(n-4)((-1)^n+3), and sgn()sgn(\cdot) is the standard sign function. This improves our previous sphere theorem \cite{XG2}. It should be emphasized that our pinching conditions above are optimal. We also obtain some new topological sphere theorems for submanifolds with pinched scalar curvature and Ricci curvature.

Keywords

Cite

@article{arxiv.1903.00209,
  title  = {The topological rigidity theorem for submanifolds in space forms},
  author = {Juanru Gu and Hongwei Xu},
  journal= {arXiv preprint arXiv:1903.00209},
  year   = {2019}
}

Comments

16 pages

R2 v1 2026-06-23T07:55:10.572Z