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On the space of null geodesics of a spacetime: the compact case, Engel geometry and retrievability (2112.06955v4)

Published 13 Dec 2021 in math.DG, gr-qc, math-ph, math.MP, and math.SG

Abstract: We compute the contact manifold of null geodesics of the family of spacetimes ${(\mathbb{S}2\times\mathbb{S}1, g_\circ-\frac{d2}{c2}dt2)}_{d,c\in\mathbb{N}+\text{ coprime}}$, with $g_\circ$ the round metric on $\mathbb{S}2$ and $t$ the $\mathbb{S}1$-coordinate. We find that these are the lens spaces $L(2c,1)$ together with the pushforward of the canonical contact structure on $ST\mathbb{S}2\cong L(2,1)$ under the natural projection $L(2,1)\to L(2c,1)$. We extend this computation to $Z\times \mathbb{S}1$ for $Z$ a Zoll manifold. On the other hand, motivated by these examples, we show how Engel geometry can be used to describe the manifold of null geodesics of a certain class of three-dimensional spacetimes, by considering the Cartan deprolongation of their Lorentz prolongation. We characterize the three-dimensional contact manifolds that are contactomorphic to the space of null geodesics of a spacetime. The characterization consists in the existence of an overlying Engel manifold with a certain foliation and, in this case, we also retrieve the spacetime.

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