Riemannian counterparts to Lorentzian space forms

preprint2022arXivOpen access

Abstract

On a smooth nn-manifold MM with n≥3n \geq 3, we study pairs (g,T)(g,T) consisting of a Riemannian metric gg and a unit length closed vector field TT. Motivated by how Ricci solitons generalize Einstein metrics via a distinguished vector field, we propose to generalize space forms by considering those pairs (g,T)(g,T) whose corresponding Lorentzian metric gL=g−2T♭⊗T♭g_{\scriptscriptstyle L} = g - 2T^{\flat} \otimes T^{\flat} has constant curvature. We show by examples that such pairs exist when MM is noncompact, and that complete metrics exist among them. When MM is compact, however, the situation is more rigid. In the compact setting, we prove that the only pairs (g,T)(g,T) whose corresponding Lorentzian metric gLg_{\scriptscriptstyle L} is a space form are those where (M,g)(M,g) is flat and its universal covering splits isometrically as a product R×N\mathbb{R} \times N. The nonexistence of compact Lorentzian spherical space forms plays a key role in our proof.

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