Algebraically special twisting gravitational fields and CR structures

Abstract
A natural framework based on the theory of Cauchy-Riemann structures (CR) is derived to study gravitational fields with twisting shear-free geodesic null congruences. The authors write down Einstein vacuum and pure radiation equations for these fields using Cartan's invariants of CR geometry. The case when the fields admit more than a two-dimensional conformal group of symmetries is solved completely. Among pure radiation solutions of this kind new solutions are obtained.

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