We prove a Goldberg–Sachs theorem in dimension three. To be precise, given a three-dimensional Lorentzian manifold satisfying the topological massive gravity equations, we provide necessary and sufficient conditions on the tracefree Ricci tensor for the existence of a null line distribution whose orthogonal complement is integrable and totally geodetic. This includes, in particular, Kundt spacetimes that are solutions of the topological massive gravity equations.
No takes yet. Share an insight, caveat, or question.
Nurowski et al. (2015) studied this question.
Synapse has enriched one closely related paper. Consider it for comparative context: