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Communicated by D. Krupka
A Lorentzian manifold is defined here as a smooth pseudo-Riemannian manifold with a metric tensor of signature (2n+1,1). A Robinson manifold is a Lorentzian manifold M of dimension >=4 with a subbundle N of the complexification of TM such that the fibers of N\toM are maximal totally null (isotropic) and [SecN,SecN]\subsetSecN. Robinson manifolds are close analogs of the proper Riemannian, Hermite manifolds. In dimension 4, they correspond to space-times of general relativity, foliated by a family of null geodesics without shear. Such space-times, introduced in the 1950s by Ivor Robinson, played an important role in the study of solutions of Einstein's equations: plane and sphere-fronted waves, the Gödel universe, the Kerr solution, and their generalizations, are among them. In this survey article, the analogies between Hermite and Robinson manifolds are presented in considerable detail.
MSC: 32C81; 53B30; 32V30; 83C20Keywords: Lorentz manifolds; Robinson manifolds; Hermite manifolds; Twistor bundles
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