Paper · Jun 30, 2020
Riemannian counterparts to Lorentzian space forms
As on arXiv
Abstract
On a smooth -manifold with , we study pairs consisting of a Riemannian metric and a unit length closed vector field . Motivated by how Ricci solitons generalize Einstein metrics via a distinguished vector field, we propose to generalize space forms by considering those pairs whose corresponding Lorentzian metric has constant curvature. We show by examples that such pairs exist when is noncompact, and that complete metrics exist among them. When is compact, however, the situation is more rigid. In the compact setting, we prove that the only pairs whose corresponding Lorentzian metric is a space form are those where is flat and its universal covering splits isometrically as a product . The nonexistence of compact Lorentzian spherical space forms plays a key role in our proof.
- Submitted
- Jun 30, 2020
- Last revised
- Aug 28, 2022 (v2)
- Subjects
- math.DG
Comments: This preprint now occupies Section 3 of arXiv:2207.14701
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Read around it
Background reading
The guides for the topics of this paper: what each idea is, why it matters, and the papers to read first.
In the guidebook
- 11A.11Hamilton’s 1982 Theorem
Positive Ricci curvature in dimension 3 flows to a round metric.
- 11B.1Ricci Solitons
Self-similar solutions: the Gaussian, cylinders, the cigar and the Bryant soliton.
- 12B.2The Asymptotic Soliton and Three-Dimensional Shrinkers
Perelman's Proposition 11.2 proved with Morgan and Tian: the reduced-length bounds on κ-solutions, the limit of rescalings, the equality case, and the classification of shrinking solitons in dimensions two and three.